2. Introduction to Quantum MechanicsSOLO
Table of Content
2
Introduction to Quantum Mechanics
Classical Mechanics
Gravity
Optics
Electromagnetism
Quantum Weirdness
History
Physical Laws of Radiometry
Zeeman Effect, 1896
Discovery of the Electron, 1897
Planck’s Law 1900
Einstein in 1905
Bohr Quantum Model of the Atom 1913.
Einstein’s General Theory of Relativity 1915
Quantum Mechanics History
3. Introduction to Quantum MechanicsSOLO
Table of Content (continue – 1)
3
De Broglie Particle-Wave Law 1924
Wolfgang Pauli states the “Quantum Exclusion Principle” 1924
Heisenberg, Born, Jordan “Quantum Matrix Mechanics”, 1925
Wave Packet and Schrödinger Equation, 1926
Operators in Quantum Mechanics
Hilbert Space and Quantum Mechanics
Von Neumann - Postulates of Quantum Mechanics
Conservation of Probability
Expectations Value and Operators
The Expansion Theorem or Superposition Principle
Matrix Representation of Wave Functions and Operators
Commutator of two Operators A and B
Time Evolution Operator of the Schrödinger Equation
Heisenberg Uncertainty Relations
4. Introduction to Quantum MechanicsSOLO
Table of Content (Continue -2)
4
Time Independent Hamiltonian
The Schrödinger and Heisenberg Pictures
Transition from Quantum Mechanics to Classical Mechanics.
Pauli Exclusion Principle
Klein-Gordon Equation for a Spinless Particle
Non-relativistic Schrödinger Equation in an Electromagnetic Field
Pauli Equation
Dirac Equation
Light Polarization and Quantum Theory
Copenhagen Interpretation of Quantum Mechanics
Measurement in Quantum Mechanics
Schrödinger’s Cat
Solvay Conferences
Bohr–Einstein Debates
Feynman Path Integral Representation of Time Evolution Amplitudes
5. Introduction to Quantum MechanicsSOLO
Table of Content (Continue -3)
5
Quantum Field Theories
References
Aharonov–Bohm Effect
Wheeler's delayed choice experiment
Zero-Point Energy
Quantum Foam
De Broglie–Bohm Theory in Quantum Mechanics
Bell's Theorem
Bell Test Experiments
Wheeler's delayed choice experiment
Hidden Variables
6. Physics
The Presentation is my attempt to study and cover the fascinating
subject of Quantum Mechanics. The completion of this presentation
does not make me an expert on the subject, since I never worked in the
field.
I thing that I reached a good coverage of the subject and I want to
share it. Comments and suggestions for improvements are more than
welcomed.
6
SOLO
Introduction to Quantum Mechanics
7. Physics
NEWTON's
MECHANICS
!
ANALYTIC
MECHANICS FLUID & GAS
DYNAMICS
THERMODYNAMICS
MAXWELL
ELECTRODYNAMICS
CLASSICAL
THEORIES
NEWTON's
GRAVITY
OPTICS
1900
At the end of the 19th century, physics had evolved to the point at which classical
mechanics could cope with highly complex problems involving macroscopic situations;
thermodynamics and kinetic theory were well established; geometrical and physical optics
could be understood in terms of electromagnetic waves; and the conservation laws for
energy and momentum (and mass) were widely accepted. So profound were these and other
developments that it was generally accepted that all the important laws of physics had been
discovered and that, henceforth, research would be concerned with clearing up minor
problems and particularly with improvements of method and measurement.
"There is nothing new to be discovered in physics now. All that remains is more and more
precise measurement" - Lord Kelvin
1900:
This was just before Relativity and Quantum Mechanics appeared on the scene and
opened up new realms for exploration.
Completeness of a Theory
7
Return to Table of Content
SOLO
8. 8
Classical TheoriesSOLO
1.1 Newton’s Laws of Motion
“The Mathematical Principles of Natural Philosophy” 1687
First Law
Every body continues in its state of rest or of uniform motion in
straight line unless it is compelled to change that state by forces
impressed upon it.
Second Law
The rate of change of momentum is proportional to the force
impressed and in the same direction as that force.
Third Law
To every action there is always opposed an equal reaction.
td
rd
constF
==→=
→
:vv0
( )vm
td
d
p
td
d
F
==
2112 FF
−=
vmp
= td
pd
F
=
12F
1 2
21F
r
- Position
v:
mp = - Momentum
9. 9
SOLO
1.2 Work and Energy
The work W of a force acting on a particle m that moves as a result of this along
a curve s from to is defined by:
F
1r
2r
∫∫ ⋅
=⋅=
⋅∆ 2
1
2
1
12
r
r
r
r
rdrm
dt
d
rdFW
r
1r
2r
rd
rdr
+
1
2
F
m
s
rd
is the displacement on a real path.
⋅⋅∆
⋅= rrmT
2
1
The kinetic energy T is defined as:
1212
2
1
2
1
2
1
2
TTrrd
m
dtrr
dt
d
mrdrm
dt
d
W
r
r
r
r
r
r
−=
⋅=⋅
=⋅
= ∫∫∫
⋅
⋅
⋅⋅⋅⋅⋅
For a constant mass m
Classical Theories
10. 10
SOLO
Work and Energy (continue)
When the force depends on the position alone, i.e. , and the quantity
is a perfect differential
( )rFF
= rdF
⋅
( ) ( )rdVrdrF
−=⋅
The force field is said to be conservative and the function is known as the
Potential Energy. In this case:
( )rV
( ) ( ) ( ) 212112
2
1
2
1
VVrVrVrdVrdFW
r
r
r
r
−=−=−=⋅= ∫∫
∆
The work does not depend on the path from to . It is clear that in a conservative
field, the integral of over a closed path is zero.
12W 1r
2r
rdF
⋅
( ) ( ) 01221
21
1
2
2
1
=−+−=⋅+⋅=⋅ ∫∫∫ VVVVrdFrdFrdF
path
r
r
path
r
rC
Using Stoke’s Theorem it means that∫∫∫ ⋅×∇=⋅
SC
sdFrdF
0=×∇= FFrot
Therefore is the gradient of some scalar functionF
( ) rdrVdVrdF
⋅−∇=−=⋅
( )rVF
−∇=
Classical Theories
11. 11
SOLO
Work and Energy (continue)
and
⋅
→∆→∆
⋅−=⋅−=
∆
∆
= rF
dt
rd
F
t
V
dt
dV
tt
00
limlim
But also for a constant mass system
⋅⋅⋅⋅⋅⋅⋅⋅⋅⋅⋅⋅
⋅=⋅=
⋅+⋅=
⋅= rFrrmrrrr
m
rrm
dt
d
dt
dT
22
1
Therefore for a constant mass in a conservative field
( ) .0 constEnergyTotalVTVT
dt
d
==+⇒=+
Classical Theories
12. SOLO
1.5 Rotations and Angular Momentum
Classical Theories
md
td
rd
mdpd
== v
md
td
rd
pd
td
d
Fd 2
2
==
md
td
rd
pdHd CG
×=×= ρρ:
∫∫ ==
M
md
td
rd
pdP
∫∫ ==
M
md
td
rd
FdF 2
2
- Angular Rotation Rate of the Body (B) relative to Inertia (I)
- Force
∫∫ ×==
M
CGCG md
td
rd
HdH
ρ - Angular Momentum
Relative to C.G.
BBBBBBIIIIII zzyyxxzzyyxxr 111111 ++=++=
BIBBBIBBBIBB
III
zz
td
d
yy
td
d
xx
td
d
z
td
d
y
td
d
x
td
d
111111
0111
×=×=×=
===
←←← ωωω
IB←ω
- Momentum
12
13. SOLO
1.6 Lagrange, Hamilton, Jacobi
Classical Theories
Carl Gustav Jacob
Jacobi
(1804-1851)
William Rowan
Hamilton
1805-1865
Joseph Louis
Lagrange
1736-1813
Lagrangiams
Lagrange’s Equations: nicQ
q
L
q
L
dt
d m
k
k
ikin
ii
,,2,1
1
=+=
∂
∂
−
∂
∂
∑=
λ
mkcqc k
t
n
i
i
k
i ,,2,10
1
==+∑=
( ) ( ) ( )qVtqqTtqqL
−= ,,:,,
ni
cQ
q
H
p
p
H
q
m
j
j
iji
i
i
i
i
,,2,1
1
=
++
∂
∂
−=
∂
∂
=
∑=
λ
mkcqc k
t
n
i
i
k
i ,,2,10
1
==+∑=
Extended Hamilton’s Equations
Constrained Differential Equations
Hamiltonian ( )tqqTqpH
n
i
ii ,,:
1
−= ∑=
ni
q
T
p
i
i ,,2,1
=
∂
∂
=
Hamilton-Jacobi Equation 0,, =
∂
∂
+
∂
∂
k
k
q
S
qtH
t
S
∂
∂
= k
kjj
q
S
qtq ,,φ
kk
q
S
p
∂
∂
= 13
14. 14
SOLO
1.4 Basic Definitions
Given a System of N particles. The System is completely defined by Particles coordinates
and moments:
( ) ( ) ( ) ( )
( ) ( ) ( )
Nl
ktpjtpitp
td
rd
mp
ktzjtyitxzyxrr
zlylxl
l
ll
lllkkkll
,,2,1
,,
=
++==
++==
where are the unit vectors defining any Inertial Coordinate Systemkji
,,
r
1r
2r
rd
rdr
+
1
2
F
m
s
The path of the Particles are defined by Newton Second Law
NlF
td
rd
m
td
pd
l
l
l
l
,,2,12
2
=== ∑
Given , the Path of the Particle is completely defined and is
Deterministic (if we repeat the experiment, we obtain every time the same result).
( ) ( ) ( )tFandtptr lll ∑== 0,0
In Classical Mechanics:
•Time and Space are two Independent Entities.
•No limit in Particle Velocity
•Since every thing is Deterministic we can Measure all quantities simultaneously.
The outcome of all measurements are repeatable and depends only on the accuracy of
the measurement device.
•Causality: Every Effect hase a Cause that preceed it.
Classical Theories
Return to Table of Content
15. GRAVITY
Classical Theories
GF
GF
M m
EQPOISSON
G
GU
r
MG
UU
r
GM
g
gm
r
MG
mr
r
mM
GF
ρπ4&&
1
2
2
=∇=−∇=
−∇=
−=
∇=−=
Newton’s Law of Universal Gravity
Any two body attract one another with a
Force Proportional to the Product of the
Masses and inversely Proportional to the
Square of the Distance between them.
G = 6.67 x 10-8
dyne cm2
/gm2
the Universal Gravitational Constant
Instantaneous Propagation of the Force along the direction between the
Masses (“Action at a Distance”).
15
16. Newton was fully aware of the conceptual difficulties of his action-at-a-distance theory of gravity.
In a letter to Richard Bentley Newton wrote:
"It is inconceivable, that inanimate brute matter should, without the mediation
of something else, which is not material, operate upon, and affect other matter
without mutual contact; as it must do, if gravitation, ....,
be essential and inherent in it. And this is one reason,
why I desired you would not ascribe innate gravity to me.
That gravity should be innate, inherent, and essential to matter,
so that one body may act upon another, at a distance through vacuum,
without the mediation of anything else, by and through their action and force
may be conveyed from one to another, is to me so great an absurdity,
that I believe no man who has in philosophical matters a competent faculty of thinking,
can ever fall into it."
GRAVITY
Classical Theories
16
Return to Table of Content
17. 17
SOLO
Newton published “Opticks”1704
Newton threw the weight of his authority
on the corpuscular theory. This
conviction was due to the fact that light
travels in straight lines, and none of the
waves that he knew possessed this
property.
Newton’s authority lasted for one hundred years, and diffraction
results of Grimaldi (1665) and Hooke (1672), and the view of Huygens
(1678) were overlooked.
Optics
Every point on a primary wavefront serves the
source of spherical secondary wavelets such that
the primary wavefront at some later time is the
envelope o these wavelets. Moreover, the
wavelets advance with a speed and frequency
equal to that of the primary wave at each point
in space.
Christiaan Huygens
1629-1695
Huygens Principle 1678
Light: Waves or Particles
Classical Theories
18. 18
SOLO
In 1801 Thomas Young uses constructive and destructive interference
of waves to explain the Newton’s rings.
Thomas Young
1773-1829
1801 - 1803
In 1803 Thomas Young explains the fringes at the edges of shadows
using the wave theory of light. But, the fact that was belived that the
light waves are longitudinal, mad difficult the explanation of double
refraction in certain crystals.
Optics
Run This
Young Double Slit Experiment
Classical Theories
19. 19
POLARIZATION
Arago and Fresnel investigated the interference of
polarized rays of light and found in 1816 that two
rays polarized at right angles to each other never
interface.
SOLO
Dominique François
Jean Arago
1786-1853
Augustin Jean
Fresnel
1788-1827
Arago relayed to Thomas Young in London the results
of the experiment he had performed with Fresnel. This
stimulate Young to propose in 1817 that the oscillations
in the optical wave where transverse, or perpendicular
to the direction of propagation, and not longitudinal as
every proponent of wave theory believed. Thomas Young
1773-1829
1816-1817
longitudinal
waves
transversal
waves
Classical Theories
Run This
20. 20
SOLO
Augustin Jean
Fresnel
1788-1827
In 1818 Fresnel, by using Huygens’ concept of secondary wavelets
and Young’s explanation of interface, developed the diffraction
theory of scalar waves.
1818Diffraction - History
Classical Theories
21. 21
Diffraction
SOLO
Augustin Jean
Fresnel
1788-1827
In 1818 Fresnel, by using Huygens’ concept of secondary wavelets and
Young’s explanation of interface, developed the diffraction theory of scalar
waves.
P
0P
Q 1x
0x
1y
0y
η
ξ
Fr
Sr
ρ
r
O
'θ
θ
Screen
Image
plane
Source
plane
0O
1O
Sn1
Σ
Σ - Screen Aperture
Sn1 - normal to Screen
From a source P0 at a distance from a aperture a spherical wavelet propagates
toward the aperture: ( ) ( )Srktj
S
source
Q e
r
A
tU −
= '
' ω
According to Huygens Principle second wavelets will start at the aperture and will add at the image
point P.
( ) ( ) ( )( )
( ) ( )( )
∫∫ Σ
++−
Σ
+−−
== dre
rr
A
Kdre
r
U
KtU rrktj
S
sourcerkttjQ
P
S 2/2/'
',', πωπω
θθθθ
where: ( )',θθK obliquity or inclination factor ( ) ( )SSS nrnr 11cos&11cos' 11
⋅=⋅= −−
θθ
( )
( )
===
===
0',0
max0',0
πθθ
θθ
K
K Obliquity factor and π/2 phase were introduced by Fresnel to explain
experiences results.
Fresnel Diffraction Formula
Fresnel took in consideration the phase of each wavelet to obtain:
Run This
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Classical Theories
22. 22
MAXWELL’s EQUATIONS
SOLO
Magnetic Field IntensityH
[ ]1−
⋅mA
Electric DisplacementD
[ ]2−
⋅⋅ msA
Electric Field IntensityE
[ ]1−
⋅mV
Magnetic InductionB
[ ]2−
⋅⋅ msV
Electric Current DensityeJ
[ ]2−
⋅mA
Free Electric Charge Distributioneρ [ ]3−
⋅⋅ msA
1. AMPÈRE’S CIRCUIT LAW (A) 1821 eJ
t
D
H
+
∂
∂
=×∇
2. FARADAY’S INDUCTION LAW (F) 1831
t
B
E
∂
∂
−=×∇
3. GAUSS’ LAW – ELECTRIC (GE) ~ 1830
eD ρ=⋅∇
4. GAUSS’ LAW – MAGNETIC (GM) 0=⋅∇ B
André-Marie Ampère
1775-1836
Michael Faraday
1791-1867
Karl Friederich Gauss
1777-1855
James Clerk Maxwell
(1831-1879)
1865
Electromagnetism
MAXWELL UNIFIED ELECTRICITY AND MAGNETISM
Classical Theories
23. 23
SOLO
ELECTROMGNETIC WAVE EQUATIONS
For Homogeneous, Linear and Isotropic Medium
ED
ε=
HB
µ=
where are constant scalars, we haveµε,
t
E
t
D
H
t
t
H
t
B
E
ED
HB
∂
∂
=
∂
∂
=×∇
∂
∂
∂
∂
−=
∂
∂
−=×∇×∇
=
=
εµ
µ
ε
µ
Since we have also
tt ∂
∂
×∇=∇×
∂
∂
( )
( ) ( )
=⋅∇=
∇−⋅∇∇=×∇×∇
=
∂
∂
+×∇×∇
0&
0
2
2
2
DED
EEE
t
E
E
ε
µε
t
D
H
∂
∂
=×∇
t
B
E
∂
∂
−=×∇
For Source less
Medium
02
2
2
=
∂
∂
−∇
t
E
E
µε
Define
meme KK
c
KK
v ===
∆
00
11
εµµε
where ( )
smc /103
10
36
1
104
11 8
9700
×=
××
==
−−
∆
π
π
εµ
c is the velocity of light in free space.
Electromagnetism
Run This
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Classical Theories
24. Completeness of a Theory
SOLO
At the end of the 19th century, physics had evolved to the point at which classical
mechanics could cope with highly complex problems involving macroscopic situations;
thermodynamics and kinetic theory were well established; geometrical and physical optics
could be understood in terms of electromagnetic waves; and the conservation laws for
energy and momentum (and mass) were widely accepted. So profound were these and other
developments that it was generally accepted that all the important laws of physics had been
discovered and that, henceforth, research would be concerned with clearing up minor
problems and particularly with improvements of method and measurement.
"There is nothing new to be discovered in physics now. All that remains is more and more
precise measurement" - Lord Kelvin
1900:
1894:
"The more important fundamental laws and facts of physical science have all been
discovered, and these are now so firmly established that the possibility of their ever being
supplanted in consequence of new discoveries is exceedingly remote.... Our future
discoveries must be looked for in the sixth place of decimals."
- Albert. A. Michelson, speech at the dedication of Ryerson Physics Lab, U. of Chicago 1894
This was just before Relativity and Quantum Mechanics appeared on the scene and
opened up new realms for exploration. 24
Classical Theories
26. Many classical particles, both slits are open
http://www.mathematik.uni-
muenchen.de/~bohmmech/Poster/post/postE.htmlThe Double Slit Experiment
A single particle, both slits are open
Many particles, one slit is open.
Many atomic particles, both slits are open
http://en.wikipedia.org/wiki/Introduction_to_quantum_mechanics#Schr.C3.B6ding
er_wave_equation
SOLO
Run This
26
QUANTUM THEORIES
https://www.youtube.com/watch?v=Q1YqgPAtzho&src_vid=4C5pq7W5yRM&feature=iv&annotation_id=an
27. According to the results of the double slit experiment, if experimenters do something to learn
which slit the photon goes through, they change the outcome of the experiment and the behavior
of the photon. If the experimenters know which slit it goes through, the photon will behave as a
particle. If they do not know which slit it goes through, the photon will behave as if it were a wave
when it is given an opportunity to interfere with itself. The double-slit experiment is meant to
observe phenomena that indicate whether light has a particle nature or a wave nature.
Richard Feynman observed that if you wish to confront all of the mysteries of quantum
mechanics, you have only to study quantum interference in the two-slit experiment
The Double Slit Experiment
SOLO
Run This
27
QUANTUM THEORIES
28. QUANTUM THEORIES
Some trajectories of a harmonic oscillator
(a ball attached to a spring) in classical
mechanics (A–B) and
quantum mechanics (C–H). In quantum
mechanics (C–H), the ball has a wave
function, which is shown with real part in
blue and imaginary part in red. The
trajectories C,D,E,F, (but not G or H) are
examples of standing waves, (or
"stationary states"). Each standing-wave
frequency is proportional to a possible
energy level of the oscillator. This "energy
quantization" does not occur in classical
physics, where the oscillator can have any
energy
28
31. 31
SOLO
http://thespectroscopynet.com/educational/Kirchhoff.htm
Spectroscopy
1868
A.J. Ångström published a compilation of all visible lines in
the solar spectrum.
1869
A.J. Ångström made the first reflection grating.
Anders Jonas Angström a physicist in Sweden, in 1853 had presented theories about
gases having spectra in his work: Optiska Undersökningar to the Royal Academy of
Sciences pointing out that the electric spark yields two superposed spectra. Angström
also postulated that an incandescent gas emits luminous rays of the same
refrangibility as those which it can absorb. This statement contains a fundamental
principle of spectrum analysis.
http://en.wikipedia.org/wiki/Spectrum_analysis
32. 32
ParticlesSOLO 1874
George Johnstone Stoney
1826 - 1911
As early as 1874 George Stoney had calculated the magnitude of
his electron from data obtained from the electrolysis of water and
the kinetic theory of gases. The value obtained later became known
as a coulomb. Stoney proposed the particle or atom of electricity to
be one of three fundamental units on which a whole system of
physical units could be established. The other two proposed were
the constant universal gravitation and the maximum velocity of
light and other electromagnetic radiations. No other scientist dared
conceive such an idea using the available data. Stoney's work set
the ball rolling for other great scientists such as Larmor and
Thomas Preston who investigated the splitting of spectral lines in a
magnetic field. Stoney partially anticipated Balmer's law on the
hydrogen spectral series of lines and he discovered a relationship
between three of the four lines in the visible spectrum of hydrogen.
Balmer later found a formula to relate all four. George Johnstone
Stoney was acknowledged for his contribution to developing the
theory of electrons by H.A. Lorentz , in his Nobel Lecture in 1902.
George Stoney estimates the charge of the then unknown electron to be about 10-20
coulomb, close to the modern value of 1.6021892 x 10-19 coulomb. (He used the
Faraday constant (total electric charge per mole of univalent atoms) divided by
Avogadro's Number.
Return to Table of Content
33. 33
Physical Laws of RadiometrySOLO
Stefan-Boltzmann Law
Stefan – 1879 Empirical - fourth power law
Boltzmann – 1884 Theoretical - fourth power law
For a blackbody:
( ) ( )
( ) ( )
⋅
⋅==
=
−
==
−
∞∞
∫∫
42
12
32
45
2
4
0 2
5
1
0
10670.5
15
2
:
1/exp
1
Kcm
W
hc
k
cm
W
Td
Tc
c
dMM
BBBB
π
σ
σλ
λλ
λλ
LUDWIG
BOLTZMANN
(1844 - 1906)
Stefan-Boltzmann Law
JOSEF
STEFAN
(1835 – 1893)
1879 1884 1893
Wien’s Displacement Law
0=
λ
λ
d
Md
BB
Wien 1893
from which:
The wavelength for which the spectral emittance of a blackbody reaches the maximum
is given by:
mλ
KmTm
⋅= µλ 2898 Wien’s Displacement Law WILHELM
WIEN
(1864 - 1928)
Nobel Prize 1911
34. 34
SOLO
Johan Jakob Balmer presented an empirical formula describing
the position of the emission lines in the visible part of the
hydrogen spectrum.
Spectroscopy 1885
Johan Jakob Balmer
1825 - 1898
Balmer Formula ( )222
/ nmmB −=λ
,6,5,4,3,106.3654,2 8
=×== −
mcmBn
δH
violet blue - green red
1=n
2=n
3=n
4=n
5=n
∞=n
Lyman
serie
Balmer
serie
Paschen
serie
Brackett
serie
0=E
Energy
−= 2232
0
4
11
8
1
nnhc
em
f
ελ
1=fn 2=f
n 3=fn 4=f
n
Balmer was a mathematical teacher who, in his spare time, was
obsessed with formulae for numbers. He once said that, given
any four numbers, he could find a mathematical formula that
connected them. Luckily for physics, someone gave him the
wavelengths of the first four lines in the hydrogen spectrum.
35. 35
SOLO Spectroscopy 1887
Johannes Robert
Rydberg
1854 - 1919
Rydberg Formula
for Hydrogen 2 2
1 1 1
H
i f
R
n nλ
= − ÷ ÷
1=n
2=n
3=n
4=n
5=n
∞=n
Lyman
serie
Balmer
serie
Paschen
serie
Brackett
serie
0=E
Energy
−= 2232
0
4
11
8
1
nnhc
em
f
ελ
1=fn 2=fn 3=f
n 4=fn
34
6.62606876 10h J s−
= × gPlank constant
31
9.10938188 10em kg−
= ×Electron mass
19
1.602176452 10e C−
= ×Electron charge
12
0 8.854187817 10 /F mε −
= ×Permittivity of
vacuum
Rydberg generalized Balmer’s hydrogen spectral lines formula.
Theodore Lyman
1874 - 1954
2in = Balmer series (1885)
Johan Jakob Balmer
1825 - 1898
Friedric Paschen
1865 - 1947
3in = Paschen series (1908)
4in = Brackett series (1922)
Lyman series (1906)1in =
Rydberg Constant
for Hydrogen 17
x105395687310973.1 −
= mRH
4
2 3
08
e
H
m e
R
h cε
=
Later in the Bohr
Model was fund that
Frederick Sumner Brackett
1896 - 1988
36. 36
PhotoelectricitySOLO
In 1887 Heinrich Hertz, accidentally discovered the photoelectric effect.
Hertz conducted his experiments that produced radio waves. By chance he
noted that a piece of zinc illuminated by ultraviolet light became
electrically charged. Without knowing he discovered the Photoelectric
Effect.
1887
Heinrich Rudolf Hertz
1857-1894
-
-
-
-
-
-
-
-
--
-
-
-
-
metallic surface
ejected electrons
incoming
E.M. waves
http://en.wikipedia/wiki/Photoelectric_effect
http://en.wikipedia/wiki/Heinrich_Hertz
Return to Table of Content
37. 37
SpectroscopySOLO
Zeeman Effect
Pieter Zeeman observed that the spectral lines
emitted by an atomic source splited when the source is
placed in a magnetic field.
In most atoms, there exists several electron
configurations that have the same energy,
so that transitions between different configuration
correspond to a single line.
1896
Because the magnetic field interacts with the
electrons, this degeneracy is broken giving rice to
very close spectral lines.
no magnetic field
B = 0
cba ,,
fed ,,
a
b
c
d
e
f
magnetic field
B 0≠
http://en.wikipedia.org/wiki/Zeeman_effect
Pieter Zeeman
1865 - 1943
Nobel Prize 1902
Return to Table of Content
38. 38
Physical Laws of RadiometrySOLO
Wien Approximation to Black Body Radiation
Wien's Approximation (also sometimes called Wien's Law or the Wien
Distribution Law) is a law of physics used to describe the spectrum of thermal
radiation (frequently called the blackbody function). This law was first derived by
Wilhelm Wien in 1896. The equation does accurately describe the short
wavelength (high frequency) spectrum of thermal emission from objects, but it
fails to accurately fit the experimental data for long wavelengths (low frequency)
emission.
WILHELM
WIEN
(1864 - 1928)
Comparison of Wien's Distribution law with
the Rayleigh–Jeans Law and Planck's law,
for a body of 8 mK temperature
The Wien ‘s Law may be written as
where
• I(ν,T) is the amount of energy per unit surface area per
unit time per unit solid angle per unit frequency emitted
at a frequency ν.
• T is the temperature of the black body.
• h is Planck's constant.
• c is the speed of light.
• k is Boltzmann's constant
1896
Return to Table of Content
39. 39
SOLO Particles
J.J. Thomson showed in 1897 that the cathode rays are composed of electrons and
he measured the ratio of charge to mass for the electron.
Discovery of the Electron
1897
Joseph John Thomson
1856 – 1940
Nobel Prize 1922
The total charge on the collector (assuming all electrons are
stick to the cathode collector and no secondary emissions is:
e
qnQ ⋅=
The energy of the particles reaching the cathode is:
2/2
vmnE ⋅⋅=
Uvm
q
E
Q e 12
2
=
⋅
= U
v
m
qe
2
2
=
Thomson Atom Model Wavelike Behavior for Electrons
Return to Table of Content
40. 40
Physical Laws of RadiometrySOLO
Rayleigh–Jeans Law
Comparison of Rayleigh–Jeans law with
Wien approximation and Planck's law, for
a body of 8 mK temperature
In 1900, the British physicist Lord Rayleigh derived
the λ−4
dependence of the Rayleigh–Jeans law based on
classical physical arguments.[3]
A more complete
derivation, which included the proportionality constant,
was presented by Rayleigh and Sir James Jeans in
1905. The Rayleigh–Jeans law revealed an important
error in physics theory of the time. The law predicted
an energy output that diverges towards infinity as
wavelength approaches zero (as frequency tends to
infinity) and measurements of energy output at short
wavelengths disagreed with this prediction.
John William Strutt,
3rd Baron Rayleigh
1842- 1919
James Hopwood Jeans
1877 - 1946
Rayleigh considered the radiation inside a cubic
cavity of length L and temperature T whose walls
are perfect reflectors as a series of standing
electromagnetic waves. At the walls of the cube, the
parallel component of the electric field and the
orthogonal component of the magnetic field must
vanish. Analogous to the wave function of a
particle in a box, one finds that the fields are
superpositions of periodic functions. The three
wavelengths λ1, λ2 and λ3, in the three directions
orthogonal to the walls can be: ,2,1,,
2
=== i
i
i
nzyxi
n
Lλ
1900 1905
41. 41
Physical Laws of RadiometrySOLO
Rayleigh–Jeans Law (continue )
The Rayleigh–Jeans law agrees with experimental results
at large wavelengths (or, equivalently, low frequencies) but
strongly disagrees at short wavelengths (or high
frequencies). This inconsistency between observations and
the predictions of classical physics is commonly known as
the ultraviolet catastrophe.
Comparison of Rayleigh–Jeans law and
Planck's law
The term "ultraviolet catastrophe" was first used in 1911
by Paul Ehrenfest, although the concept goes back to 1900
with the first derivation of the λ − 4
dependence of the
Rayleigh–Jeans law;
Solution
Max Planck solved the problem by postulating that electromagnetic energy did not follow the classical description,
but could only oscillate or be emitted in discrete packets of energy proportional to the frequency, as given by
Planck's law. This has the effect of reducing the number of possible modes with a given energy at high frequencies
in the cavity described above, and thus the average energy at those frequencies by application of the equipartition
theorem. The radiated power eventually goes to zero at infinite frequencies, and the total predicted power is finite.
The formula for the radiated power for the idealized system (black body) was in line with known experiments, and
came to be called Planck's law of black body radiation. Based on past experiments, Planck was also able to
determine the value of its parameter, now called Planck's constant. The packets of energy later came to be called
photons, and played a key role in the quantum description of electromagnetism.
( ) ( ) λ
λ
π
λ
λ
λλ d
Tk
d
V
N
Tkdu 4
8
== Rayleigh–Jeans Law
Return to Table of Content
42. 42
Physical Laws of RadiometrySOLO
MAX
PLANCK
(1858 - 1947)
4242( ) ν
ννπ
νν ν
d
e
h
c
du
kT
h
1
8
3
2
−
=
( ) ν
νπ
νν
ν
de
c
h
du kT
h
−
= 3
3
8
WILHELM
WIEN
(1864 - 1928)
Wien’s Law 1896
( ) ν
νπ
νν dTk
c
du 3
2
8
=
Rayleigh–Jeans Law
1900 - 1905
John William Strutt,
3rd Baron Rayleigh
1842- 1919
James Hopwood Jeans
1877 - 1946
Comparison of Rayleigh–Jeans law
with Wien approximation and
Planck's law, for a body of 8 mK
temperature
Tkh <<ν
Tkh >>ν
43. 43
Physical Laws of RadiometrySOLO
MAX
PLANCK
(1858 - 1947)
Planck’s Law 1900
( ) ν
ννπ
νν ν
d
e
h
c
du
kT
h
1
8
3
2
−
=
Planck derived empirically, by fitting the observed black body
distribution to a high degree of accuracy, the relation
By comparing this empirical correlation with the Rayleigh-Jeans
formula Planck concluded that the error in
classical theory must be in the identification of the average oscillator
energy as kT and therefore in the assumption that the oscillator
energy is distributed continuously. He then posed the following
question:
If the average energy is defined as
how is the actual oscillator energies distributed?
( ) ν
νπ
νν dTk
c
du 3
2
8
=
1/
−
= kTh
e
h
E ν
ν
KT
KWk
Wh
ineTemperaturAbsolute-
constantBoltzmannsec/103806.1
constantPlanksec106260.6
23
234
−⋅⋅=
−⋅⋅=
−
−
44. 44
Physical Laws of RadiometrySOLO
MAX
PLANCK
(1858 - 1947)
If the average energy is defined as
how is the actual oscillator energies distributed?
1/
−
= kTh
e
h
E ν
ν
Planck deviated appreciable from the concepts of classical physics by
assuming that the energy of the oscillators, instead of varying
continuously, can assume only certain discrete values
νε hnn =
Let determine the average energy
( )
( )
+++
++
=== −−
−−
∞
=
−
∞
=
−
∞
=
−
∞
=
−
∑
∑
∑
∑
kThkTh
kThkTh
n
kTnh
n
kTnh
n
kTE
n
kTE
n
ee
eeh
e
enh
e
eE
E
n
n
/2/
/2/
0
/
0
/
0
/
0
/
1
2
νν
νν
ν
ν
ν
ν
From Statistical Mechanics we know that the probability of a system
assuming energy between ε and ε+dε is proportional to exp (-ε/kT) dε
x
ee
kTh
ex
kThkTh
−
=+++
−
=
−−
1
1
1
/
/2/
ν
νν
( )
( )2
0
/2/
0
/
11
1
2
/
x
x
h
xxd
d
xhxn
xd
d
xheehenh
n
n
ex
kThkTh
n
kTnh
kTh
−
=
−
==++= ∑∑
∞
=
=
−−
∞
=
−
−
ννννν
ν
ννν
where n is an integer (n = 0, 1, 2, …), and h =6.6260.
10-14
W.
sec2
is a constant introduced empirically by Planck , the Planck’s Constant.
45. 45
Physical Laws of RadiometrySOLO
MAX
PLANCK
(1858 - 1947)
Planck’s Postulate:
The energy of the oscillators, instead of varying continuously, can
assume only certain discrete values
νε hnn =
where n is an integer (n = 0, 1, 2, …). We say that the oscillators
energy is Quantized.
( )
11
1
1
1
//
/
/
2/
/
0
/
0
/
0
/
0
/
−
=
−
=
−
−
=== −
−
−
−
−
∞
=
−
∞
=
−
∞
=
−
∞
=
−
∑
∑
∑
∑
kThkTh
kTh
kTh
kTh
kTh
n
kTnh
n
kTnh
n
kTE
n
kTE
n
e
h
e
e
h
e
e
e
h
e
enh
e
eE
E
n
n
νν
ν
ν
ν
ν
ν
ν
ν
ν
νν
The average energy is
46. 46
Physical Laws of RadiometrySOLO
Plank’s Law
( ) 1/exp
1
2
5
1
−
=
Tc
c
M
BB
λλ
λ
Plank’s Law applies to blackbodies; i.e. perfect radiators.
The spectral radial emittance of a blackbody is given by:
( )
KT
KWk
Wh
kmc
Kmkhcc
mcmWchc
ineTemperaturAbsolute-
constantBoltzmannsec/103806.1
constantPlanksec106260.6
lightofspeedsec/458.299792
10439.1/
107418.32
23
234
4
2
4242
1
−⋅⋅=
−⋅⋅=
−=
⋅⋅==
⋅⋅⋅==
−
−
−
µ
µπ
Plank’s Law
1900
MAX
PLANCK
1858 - 1947
Nobel Prize 1918
Return to Table of Content
47. 47
SOLO Particles
J.J. Thomson showed in 1897 that the cathode rays are composed of electrons and
he measured the ratio of charge to mass for the electron.
In 1904 he suggested a model of the atom as a
sphere of positive matter in which electrons are
positioned by electrostatic forces.
Thomson Atom Model
1904
--
--
--
--
--
--
--
--
--
--
Joseph John Thomson
1856 – 1940
Nobel Prize 1922
Plum Pudding Model
Return to Table of Content
48. 48
PhotoelectricitySOLO
Einstein and Photoelectricity
Albert Einstein explained the photoelectric effect
discovered by Hertz in 1887 by assuming that the light
is quantized (using Plank results) in quantities that
later become known as photons.
1905
-
-
-
-
-
-
-
-
--
-
-
-
-
metallic surface
ejected electrons
incoming
E.M. waves
k
E
0
ν ν
0
2
2
1
νν hhvmE ek −==
The kinetic energy Ek of the ejected electron is:
where:
functionworksec
frequencylight
constantPlanksec106260.6
0
234
−⋅
−
−⋅⋅= −
Wh
Hz
Wh
ν
ν
Albert Einstein
1879 - 1955
Nobel Prize 1921
To eject an electron the frequency of the incoming EM wave
v must be above a threshold v0 (depends on metallic surface).
Increasing the Intensity of the EM Wave will increase the
number of electrons ejected, but not their energy.
Return to Table of Content
50. EINSTEIN’s SPECIAL THEORY OF RELATIVITY (Continue)
First Postulate:
It is impossible to measure or detect the Unaccelerated Translation
Motion of a System through Free Space or through any Aether-like
Medium.
Second Postulate:
Velocity of Light in Free Space, c, is the same for all Observers,
independent of the Relative Velocity of the Source of Light and the
Observers.
Second Postulate (Advanced):
Speed of Light represents the Maximum Speed of transmission of
any Conventional Signal.
Special Relativity Theory
50
51. 51
SOLO
x
z
y
'x
'z
'y
v
'u
'OO
'u−
A B
Consequence of Special Theory of Relativity
The relation between the mass m of a particle having a
velocity u and its rest mass m0 is:
2
2
0
1
c
u
m
m
−
=
Special Relativity Theory
EINSTEIN’s SPECIAL THEORY OF RELATIVITY (Continue)
The Kinetic Energy of a free moving particle having a momentum p = m u,
a velocity u and its rest mass m0 is:
42
0
222
cmcpT +=
The velocity of a photon is u = c, therefore, from the first equation, it has a rest mass
00 =photonm
And has a Kinetic Energy and Total Energy of νhEcpT
VTE
V
===
+=
=0
Therefore if v is the photon Frequency and λ is photon Wavelength, we have
cm
h
p
hc cmph
cp
=
=
===
ν
ν
λ
52. Locality and NonlocalitySOLO
Event inside
Light Cone
EVENT HERE
AND NOW
Simultaneous Event
at different place
A Light Cone is the path that a flash of light,
emanating from a single Event (localized to a single
point in space and a single moment in time) and
traveling in all directions, would take through
space-time. The Light Cone Equation is
( ) 022222
=−++ tczyx
Events Inside the Light Cone
( ) 022222
<−++ tczyx
Events Outside the Light Cone
( ) 022222
>−++ tczyx
Einstein’s Theory of Special Relativity Postulates that no Signal can travel with a speed
higher than the Speed of Light c.
Thousands of experiments performed with Particles (Photons, Electrons. Neutrons,…) complied
to this Postulate. However no experiments could be performed with Sub-particles, so, in my
opinion the confirmation of this Postulate is still an open issue.
Light Cone
52
53. Locality and NonlocalitySOLO Event inside
Light Cone
EVENT HERE
AND NOW
Simultaneous Event
at different place
According to Einstein only Events within Light Cone
(shown in the Figure) can communicate with an event at
the Origin, since only those Space-time points can be
connected by a Signal traveling with the Speed of Light c
or less. We call those Events “Local” although they may be
separated in Space-time.
Locality
The Postulates of Relativity require that all frames of reference to be equivalent. So, if the
Events are “Local” in any realizable frame of reference, they must be “Local” in all equivalent
Frame of Reference. Two Space-time Points within Light Cone are called “timelike”.
Nonlocality
Two Space-time Points outside Light Cone are said to have “Spacelike Separation”.
“Nonlocality” connected Points outside the Light Cone. They have Space-time separation.
Simultaneously Events (Time = 0), in any given Reference Frame , cannot be causally connected
unless the signal between them travels at superluminal speed.
Some physicists use the term “Holistic” instead of “Nonlocal”.
“Holistic” = “Nonlocal”
53
Return to Table of Content
54. 54
SOLO
1908 Geiger-Marsden Experiment.
Ernest Rutherford
1871 - 1937
Nobel Prize 1908
Chemistry
Hans Wilhelm
Geiger
1882 – 1945
Nazi Physicist
Sir Ernest
Marsden
1889 – 1970
Geiger-Marsden working with Ernest Rutherford performed
in 1908 the alpha-particle scattering experiment. H. Geiger
and E. Marsden (1909), “On a Diffuse Reflection of the α-
particle”, Proceedings of the Royal Society Series A 82:495-
500
A small beam of α-particles was directed at a thin gold foil.
According to J.J. Thomson atom-model it was anticipated that
most of the α-particles would go straight through the gold foil,
while the remainder would at most suffer only slight deflections.
Geiger-Marsden were surprised to find out that, while most of
the α-particles were not deviated, some were scattered through
very large angles after passing the foil.
QUANTUM THEORIES
55. 55
ParticlesSOLO
Electron Charge
R.A. Millikan measured the charge of the electron
by equalizing the weight m g of a charged oil drop
with an electric field E.
1909
Robert Andrews Millikan
1868 – 1953
Nobel Prize 1923
56. 56
SOLO
Rutherford Atom Model
1911 Ernest Rutherford finds the first evidence of protons.
To explain the Geiger-Marsden Experiment of 1908 he
suggested in 1911 that the positively charged atomic
nucleus contain protons.
Ernest Rutherford
1871 - 1937
Nobel Prize 1908
Chemistry
Hans Wilhelm
Geiger
1882 – 1945
Nazi Physicist
Sir Ernest
Marsden
1889 – 1970
--
--
--
--
--
--
--
--
--
--
+2
+2
+2
Rutherford assumed that the atom model consists of a small
nucleus, of positive charge, concentrated at the center, surrounded
by a cloud of negative electrons. The positive α-particles that passed
close to the positive nucleus were scattered because of the electrical
repealing force between the positive charged α-particle and the nucleus .
QUANTUM MECHANICS
Return to Table of Content
57. 57
1913
SOLO
Niels Bohr presents his quantum model of the atom.
Niels Bohr
1885 - 1962
Nobel Prize 1922
QUANTUM MECHANICS
Bohr Quantum Model of the Atom.
58. 58
1913
SOLO
Niels Bohr
1885 - 1962
Nobel Prize 1922
Explanation of Bohr Hydrogen Model
In 1911, Bohr travelled to England. He met with J. J. Thomson of the Cavendish
Laboratory and Trinity College, Cambridge, and New Zealand's Ernest
Rutherford, whose 1911 Rutherford model of the atom had challenged Thomson's
1904 Plum Pudding Model.[
Bohr received an invitation from Rutherford to
conduct post-doctoral work at Victoria University of Manchester. He adapted
Rutherford's nuclear structure to Max Planck's quantum theory and so created
his Bohr model of the atom.[
In 1885, Johan Balmer had come up with his Balmer series to describe
the visible spectral lines of a hydrogen atoms:
that was extended by Rydberg in 1887, to
Additional series by Lyman (1906), Paschen (1908)
( )222
/ nmmB −=λ
2 2
1 1 1
H
i f
R
n nλ
= − ÷ ÷
Bohr Model of the Hydrogen Atom consists on a electron, of
negative charge, orbiting a positive charge nucleus.
The Forces acting on the orbiting electron are
AttractionofForceticElectrosta
r
e
F
ForcelCentripeta
r
m
F
e
c
2
0
2
2
4
v
επ
=
=
m – electron mass
v – electron orbital velocity
r – orbit radius
e – electron charge
( )229
0
/109
4
1
coulombmN ⋅×=
επ
QUANTUM MECHANICS
59. 59
1913
SOLO
Niels Bohr
1885 - 1962
Nobel Prize 1922
Explanation of Bohr Hydrogen Model (continue – 1)
The Conditions for Orbit Stability are
2
0
22
4
v
r
e
r
m
FF ec
επ
=
=
rm
e
04
v
επ
=
The Total Energy E, of the Electron, is the sum of the Kinetic
Energy T and the Potential Energy V
r
e
r
e
r
e
r
em
VTE
0
2
0
2
0
2
0
22
84842
v
επεπεπεπ
−=−=−=+=
To get some quantitative filing let use the fact that to separate
the electron from the atom we need 13.6 eV (this is an
experimental result), then E = -13.6 eV = 2.2x10-18
joule.
Therefore
( )
( )
( )
m
joule
coulombmN
coulomb
E
e
r 11
18
229
219
0
2
103.5
102.2
/109
2
106.1
8
−
−
−
×=
×−
⋅×
×
−=−=
επ
QUANTUM MECHANICS
60. 1913
SOLO
Niels Bohr
1885 - 1962
Nobel Prize 1922
Explanation of Bohr Hydrogen Model (continue – 2)
The problem with this Model is, since the electron accelerates with a =v2
/r,
according to Electromagnetic Theory it will radiate energy given by
Larmor Formula (1897)
( )
sec/109.2sec/106.4
43
2
43
2 109
4233
0
6
3
0
22
evjoule
rmc
e
c
ae
P ×=×=== −
επεπ
As the electron loses energy the Total
Energy becomes more negative and the
radius decreases, and since P is
proportional to 1/r4
, the electron radiates
energy faster and faster as it spirals
toward the nucleus.
Bohr had to add something to
explain the stability of the orbits.
He knew the results of the discrete
Hydrogen Spectrum lines and the
quantization of energy that Planck
introduced in 1900 to obtain the
Black Body Radiation Equation.
Sir Joseph Larmor FRS
(1857 – 1942)
QUANTUM MECHANICS
60
61. 1913
SOLO
Niels Bohr
1885 - 1962
Nobel Prize 1922
Explanation of Bohr Hydrogen Model (continue – 3)
To understand Bohr novelty let look at an Elastic Wire
that vibrates transversally. At Steady State the
Wavelengths always fit an integral number of times into
the Wire Length. This is true if we bend the Wire and
even if we obtain a Closed Loop Wire. If the Wire is
perfectly elastic the vibration will continue indefinitely.
This is Resonance.
Bohr noted that the Angular Momentum of the Orbiting
electron in the Atom Hydrogen Model had the same
dimensions as the Planck’s Constant. This led him to
postulate that the Angular Momentum of the Orbiting
Electrons must be multiple of Planck’s Constant divided
by 2 π.
,3,2,1
24
v
0
=== n
h
nr
rm
e
mrm n
n
n
πεπ
,3,2,12
0
22
== n
em
hn
rn
π
ε
therefore
QUANTUM MECHANICS
61
62. 1913
SOLO
Niels Bohr
1885 - 1962
Nobel Prize 1922
Explanation of Bohr Hydrogen Model (continue – 4)
Energy Levels and Spectra
We obtained
,3,2,1
1
88 222
0
4
0
2
=
−=−= n
nh
em
r
e
E
n
n
εεπ
,3,2,12
0
22
== n
em
hn
rn
π
ε
and Energy Levels:
The Energy Levels are all negative signifying that the
electron does not have enough energy to escape from the
atom.
The lowest energy level E1 is called the Ground State.
The higher levels E2, E3, E4,…, are called Excited States.
In the limit n →∞, E∞=0 and the electron is no longer
bound to the nucleus to form an atom.
QUANTUM MECHANICS
62
63. 63
1913
SOLO
Niels Bohr
1885 - 1962
Nobel Prize 1922
Explanation of Bohr Hydrogen Model (continue – 5)
According to the Bohr Hydrogen Model when
the electron is excited he drops to a lower state,
and a single photon of light is emitted
Initial Energy – Final Energy = Photon Energy
vh
nnh
em
nh
em
nh
em
EE
iffi
fi =
−=
+
−=− 2222
0
4
222
0
4
222
0
4
11
8
1
8
1
8 εεε
where v is the photon frequency.
If λ is the Wavelength of the photon we have
−=
−=
−
== 222232
0
4
1111
8
1
if
H
if
fi
nn
R
nnch
em
ch
EE
c
v
ελ
2in = Balmer series (1885)
3in = Paschen series (1908)
4in = Brackett series (1922)
Lyman series (1906)1in =
We recovered the Rydberg Formula (1887)
( )
( ) ( )
17
3348212
41931
32
0
4
10097.1
sec1063.6/103/1085.88
106.1101.9
8
−
−−
−−
×=
−××××××
×××
=
m
joulesmmfarad
coulombkg
ch
em
ε
QUANTUM MECHANICS
64. 64
1913
SOLO
Niels Bohr
1885 - 1962
Nobel Prize 1922
Explanation of Bohr Hydrogen Model (continue – 6)
2. The Bohr model treats the electron as if it were a miniature planet, with definite radius
and momentum. This is in direct violation of the uncertainty principle (formulated by
Werner Heisenberg in 1927) which dictates that position and momentum cannot be
simultaneously determined.
1. It fails to provide any understanding of why certain spectral lines are brighter than others.
There is no mechanism for the calculation of transition probabilities.
While the Bohr model was a major step toward understanding the quantum theory of the
atom, it is not in fact a correct description of the nature of electron orbits. Some of the
shortcomings of the model are:
The electrons in free atoms can will be found in only certain discrete energy
states. These sharp energy states are associated with the orbits or shells of
electrons in an atom, e.g., a hydrogen atom. One of the implications of these
quantized energy states is that only certain photon energies are allowed when
electrons jump down from higher levels to lower levels, producing the
hydrogen spectrum. The electron must jump instantaneously because if he
moves gradually it will radiate and lose energy in the process. The Bohr
model successfully predicted the energies for the hydrogen atom, but had
significant failures.
Quantized Energy States
QUANTUM MECHANICS
Return to Table of Content
65. 1915Einstein’s General Theory of Relativity
The “General” Theory of Relativity takes in consideration the action of Gravity
and does not assume Unaccelerated Observer like “Special” Theory of Relativity.
Principle of Equivalence – The Inertial Mass and the Gravitational Mass of the
same body are always equal.
(checked by experiments first performed by Eötvos in 1890)
Principle of Covariance -- The General Laws of Physics can be expressed in a
form that is independent of the choise of the coordinate system.
Principle of Mach -- The Gravitation Field and Metric (Space Curvature)
depend on the distribution of Matter and Energy.
SOLO GENERAL RELATIVITY
Dissatisfied with the Nonlocality (Action at a Distance) of
Newton’s Law of GravityEinstein developed the General
Theory of Gravity.
Albert Einstein
1879 - 1955
Nobel Prize 1921
65
66. GENERAL RELATIVITY
Einstein’s General Theory Equation
TENSOR
MOMENTUMENERGY
CURVATURETIMESPACE
TG
c
RgR
−
−
=− µνµνµν
π
2
8
2
1
The Matter – Energy Distribution produces the Bending (Curvature) of the Space-Time.
All Masses are moving on the Shortest Path (Geodesic) of the Curved Space-Time.
In the limit (Weak Gravitation Fields) this Equation reduce to the
Poisson’s Equation of Newton’s Gravitation Law
SOLO
66
68. GENERAL RELATIVITY
Einstein’s General Theory of Relativity (Summary)
• Gravity is Geometry
• Mass Curves Space – Time
• Free Mass moves on the
Shortest Path
in Curved Space – Time.
SOLO
Newton’s Gravity
The Earth travels around the Sun because it is pulled
by the Gravitational Force exerted by the Mass of the Sun.
Mass (somehow) causes a Gravitational Force which propagates
instantaneously (Action at a Distance) and causes True Acceleration.
Einstein’s Gravity
The Earth travels around the Sun because is the Shortest Path in the
Curved Space – Time produced by the Mass of the Sun. Mass (somehow)
causes a Warping, which propagates with the Speed of Light, and results in
Apparent Acceleration.
68
Return to Table of Content
69. 69
Photons EmissionSOLO
Theory of Light Emission. Concept of Stimulated Emission
1916
Albert Einstein
1879 - 1955
Nobel Prize 1921
http://members.aol.com/WSRNet/tut/ut4.htm
Spontaneous Emission
& Absorption
Stimulated Emission
& Absorption
“On the Quantum Mechanics of Radiation”
Run This
Einstein’s work laid the
foundation of the Theory
of LASER (Light
Amplification by
Stimulated Emission)
Return to Table of Content
70. E. RUTHERFORD OTTO STERN W. GERLACH A. COMPTON L. de BROGLIE W. PAULI
QUANTUM MECHANICS
1919: ERNEST RUTHERFORD FINDS THE FIRST EVIDENCE OF PROTONS.
HE SUGGESTED IN 1914 THAT THE POSITIVELY CHARGED ATOMIC
NUCLEUS CONTAINS PROTONS.
1922: OTTO STERN AND WALTER GERLACH SHOW “SPACE QUANTIZATION”
1923: ARTHUR COMPTON DISCOVERS THE QUANTUM NATURE OF X RAYS,
THUS CONFIRMS PHOTONS AS PARTICLES.
1924: LOUIS DE BROGLIE PROPOSES THAT MATTER HAS WAVE PROPERTIES.
1924: WOLFGANG PAULI STATES THE QUANTUM EXCLUSION PRINCIPLE.
70
71. W. HEISENBERG MAX BORN P. JORDAN S. GOUDSMITH G. UHLENBECK E. SCHRODINGER
QUANTUM MECHANICS
1925: WERNER HEISENBERG, MAX BORN, AND PASCAL JORDAN FORMULATE
QUANTUM MATRIX MECHANICS.
1925: SAMUEL A. GOUDSMITH AND GEORGE E. UHLENBECK POSTULATE THE
ELECTRON SPIN
1926: ERWIN SCHRODINGER STAES THE NONRELATIVISTIC
QUANTUM WAVE EQUATION AND FORMULATES THE
QUANTUM MECHANICS. HE PROVES THAT WAVE AND
MATRIX FORMULATIONS ARE EQUIVALENT
71
72. W. HEISENBERGMAX BORN PAUL DIRAC J. von NEUMANN
QUANTUM MECHANICS
1926: MAX BORN GIVES A PROBABILISTIC INTERPRATATION
OF THE WAVE FUNCTION.
1927: WERNER HEISENBERG STATES THE QUANTUM
UNCERTAINTY PRINCIPLE.
1928: PAUL DIRAC STATES HIS RELATIVISTIC QUANTUM WAVE
EQUATION. HE PREDICTS THE EXISTENCE OF THE
POSITRON.
1932: JHON von NEUMANN WROTE “THE FOUNDATION OF QUANTUM MECHANICS”
72
Return to Table of Content
73. 73
SOLO
1922 Otto Stern and Walter Gerlach show “Space Quantization”
Walter Gerlach
1889 - 1979
They designed the Stern-Gerlach
Experiment that determine if a particle
has angular momentum.
http://en.wikipedia.org/wiki/Stern-Gerlach_experiment
Otto Stern
1888 – 1969
Nobel Prize 1943
They directed a beam of neutral silver atoms
from an oven trough a set of collimating slits
into an inhomogeneous magnetic field. A
photographic plate recorded the configuration
of the beam.
They found that the beam split into two parts,
corresponding to the two opposite spin
orientations, that are permitted by space
quantization.
Run This
QUANTUM MECHANICS
74. 74
SOLO
1923
Arthur Compton discovers the quantum nature of X rays, thus confirms photons
as particles.
Arthur Holly Compton
1892 - 1962
Nobel Prize 1927
incident photon
( )
( ) chp
hE
photon
photon
/ν
ν
=−
=−
( )
( ) 0
2
0
=−
=−
electron
electron
p
cmE
target electron
Compton effect consists of a X ray (incident
photons) colliding with rest electrons
incident photon
scatteredphoton
( )
( ) chp
hE
photon
photon
/ν
ν
=−
=−
( )
( ) 0
2
0
=−
=−
electron
electron
p
cmE
( )
( ) chp
hE
photon
photon
/'
'
ν
ν
=+
=+
( ) ( )
( )
( )'
2 2
0
2
2242
0
νν −=
+=+
−+=+
hT
TcmTp
cpcmE
electron
photonelectron
ϕ
θ
( )ϕ
νν
λλ cos1
'
'
0
−=−=−
cm
hcc
scatteredelectron
target electron
is scattered in the φ direction (detected by an X-ray
spectrometer) and the electrons in the θ direction.
Run This
QUANTUM MECHANICS
Return to Table of Content
75. 75
SOLO
1924
Louis de Broglie proposes that matter has wave properties and
using the relation between Wavelength and Photon mass:
Louis de Broglie
1892 - 1987
Nobel Prize 1929
cm
h
p
hc cmph
cp
=
=
===
ν
ν
λ
He postulate that any Particle of mass m and velocity v has an associate Wave
with a Wavelength λ.
QUANTUM MECHANICS
76. SOLO
Niels Bohr
1885 - 1962
Nobel Prize 1922
Explanation of Bohr Model using de Broglie Relation
To understand Bohr novelty let look at an Elastic Wire
that vibrates transversally. At Steady State the
Wavelengths always fit an integral number of times into
the Wire Length. This is true if we bend the Wire and
even if we obtain a Closed Loop Wire. If the Wire is
perfectly elastic the vibration will continue indefinitely.
This is Resonance.
,3,2,12
4 0
=== nr
m
r
e
h
nn n
n
π
επ
λ
,3,2,12
0
22
== n
em
hn
rn
π
ε
We found the Electron
Orbital Velocity
Return to Bohr Hydrogen Model using de Broglie Relation
Louis de Broglie
1892 - 1987
Nobel Prize 1929
rm
e
04
v
επ
=
Using de Broglie Relation
m
r
e
h
m
h 04
v
επ
λ ==
At Steady State the Wavelengths always fit an
integral number of times into the Wire Length.
We obtain the same relation as Bohr for the Orbit radius:
QUANTUM MECHANICS
76
Return to Table of Content
77. 77
SOLO
1924
Wolfgang Pauli states the “Quantum Exclusion Principle”
Wolfgang Pauli
1900 - 1958
Nobel Prize 1945
QUANTUM MECHANICS
Return to Table of Content
78. QUANTUM THEORIES
Werner Heisenberg, Max Born, and Pascal Jordan formulate Quantum
Matrix Mechanics.
QUANTUM MATRIX MECHANICS.
Werner Karl Heisenberg
(1901 – 1976)
Nobel Price 1932
Max Born
(1882–1970)
Nobel Price 1954
Ernst Pascual Jordan
(1902 – 1980)
Nazi Physicist
http://en.wikipedia.org/wiki/Matrix_mechanics
1925
Matrix mechanics was the first conceptually autonomous and
logically consistent formulation of quantum mechanics. It extended the
Bohr Model by describing how the quantum jumps occur. It did so by
interpreting the physical properties of particles as matrices that evolve
in time. It is equivalent to the Schrödinger wave formulation of
quantum mechanics, and is the basis of Dirac's bra-ket notation for the
wave function.
SOLO
In 1928, Einstein nominated Heisenberg, Born, and Jordan for the
Nobel Prize in Physics, but Heisenberg alone won the 1932 Prize "for
the creation of quantum mechanics, the application of which has led to
the discovery of the allotropic forms of hydrogen",[47]
while
Schrödinger and Dirac shared the 1933 Prize "for the discovery of new
productive forms of atomic theory".[47]
On 25 November 1933, Born
received a letter from Heisenberg in which he said he had been delayed
in writing due to a "bad conscience" that he alone had received the
Prize "for work done in Gottingen in collaboration — you, Jordan and
I."[48]
Heisenberg went on to say that Born and Jordan's contribution
to quantum mechanics cannot be changed by "a wrong decision from
the outside." 78
Return to Table of Content
79. 1925
SAMUEL A. GOUDSMITH AND GEORGE E. UHLENBECK POSTULATE THE
ELECTRON SPIN
George Eugene
Uhlenbeck
(1900 – 1988)
Samuel Abraham
Goudsmit
(1902 – 1978)
Two types of experimental evidence which arose in the 1920s
suggested an additional property of the electron.
One was the closely spaced splitting of the hydrogen spectral
lines, called fine structure.
The other was the Stern-Gerlach experiment which showed
in 1922 that a beam of silver atoms directed through an
inhomogeneous magnetic field would be forced into two
beams. Both of these experimental situations were consistent
with the possession of an intrinsic angular momentum and a
magnetic moment by individual electrons. Classically this
could occur if the electron were a spinning ball of charge,
and this property was called electron spin.
In 1925, the Dutch Physicists S.A. Goudsmith and G.E. Uhlenbeck
realized that the experiments can be explained if the electron has an
magnetic property of Rotation or Spin. They work actually showed that
the electron has a quantum-mechanical notion of spin that is similar
to the mechanical rotation of particles.
http://hyperphysics.phy-astr.gsu.edu/hbase/spin.html
no magnetic field
B = 0
cba ,,
fed ,,
a
b
c
d
e
f
magnetic field
B 0≠
Zeeman’s Effect
QUANTUM MECHANICS
79
80. Spin
In quantum mechanics and particle physics, Spin is an intrinsic form of angular
momentum carried by elementary particles, composite particles (hadrons), and
atomic nuclei. Spin is a solely quantum-mechanical phenomenon; it does not have a
counterpart in classical mechanics (despite the term spin being reminiscent of
classical phenomena such as a planet spinning on its axis).[
Spin is one of two types of angular momentum in quantum mechanics, the other
being orbital angular momentum. Orbital angular momentum is the quantum-
mechanical counterpart to the classical notion of angular momentum: it arises
when a particle executes a rotating or twisting trajectory (such as when an electron
orbits a nucleus).The existence of spin angular momentum is inferred from
experiments, such as the Stern–Gerlach experiment, in which particles are observed
to possess angular momentum that cannot be accounted for by orbital angular
momentum alone.[
http://en.wikipedia.org/wiki/Spin_(physics)
In some ways, spin is like a vector quantity; it has a definite “magnitude”; and it has
a "direction" (but quantization makes this "direction" different from the direction
of an ordinary vector). All elementary particles of a given kind have the same
magnitude of spin angular momentum, which is indicated by assigning the particle a
spin quantum number.[2]
However, in a technical sense, spins are not strictly vectors,
and they are instead described as a related quantity: a Spinor. In particular, unlike a
Euclidean vector, a spin when rotated by 360 degrees can have its sign reversed
QUANTUM MECHANICS
80
81. ERWIN SCHRÖDINGER STAES THE NONRELATIVISTIC
QUANTUM WAVE EQUATION AND FORMULATES THE
QUANTUM MECHANICS. HE PROVES THAT WAVE AND
MATRIX FORMULATIONS ARE EQUIVALENT
1926
In January 1926, Schrödinger published in Annalen der Physik the paper
"Quantisierung als Eigenwertproblem" [“Quantization as an Eigenvalue Problem”]
on wave mechanics and presented what is now known as the Schrödinger equation. In
this paper, he gave a "derivation" of the wave equation for time-independent systems
and showed that it gave the correct energy eigenvalues for a hydrogen-like atom. This
paper has been universally celebrated as one of the most important achievements of the
twentieth century and created a revolution in quantum mechanics and indeed of all
physics and chemistry. A second paper was submitted just four weeks later that solved
the quantum harmonic oscillator, rigid rotor, and diatomic molecule problems and
gave a new derivation of the Schrödinger equation. A third paper in May showed the
equivalence of his approach to that of Heisenberg.
http://en.wikipedia.org/wiki/Erwin_Schr%C3%B6dinger
QUANTUM MECHANICS
Erwin Rudolf Josef
Alexander Schrödinger
(1887 – 1961)
Nobel Prize 1933
SOLO
81
82. MAX BORN GIVES A PROBABILISTIC INTERPRATATION
OF THE WAVE FUNCTION.
1926
Max Born
(1882–1970)
Nobel Price 1954
Max Born wrote in 1926 a short paper on collisions between particles,
about the same time as Schrödinger paper “Quantization as an
Eigenvalue Problem”. Born rejected the Schrödinger Wave Field
approach. He had been influenced by a suggestion made by Einstein
that, for photons, the Wave Field acts as strange kind of ‘phantom’ Field
‘guiding’ the photon particles on paths which could therefore be
determined by Wave Interference Effects.
Max Born reasoned that the Square of the Amplitude of the Waveform in some specific region
of configuration space is related to the Probability of finding the associated quantum particle in
that region of configuration space.
Since Probability is a real number, and the integral of all Probabilities over all regions of
configuration space, the Wave Function must satisfy
1*
=∫
+∞
∞−
dVψψ Condition of Normalization of the Wave Function
Therefore the probability of finding the particle
between a and b is given by
[ ] ( ) ( )∫=≤≤
b
a
xdxxbXaP ψψ *
Einstein rejected this interpretation. In a 1926 letter to Max Born, Einstein
wrote: "I, at any rate, am convinced that He [God] does not throw dice."[
QUANTUM MECHANICS
SOLO
82
Return to Table of Content
83. QUANTUM MECHANICS
In December 1926 Einstein wrote a letter to Bohr which
contains a phrase that has since become symbolic of
Einstein’s lasting dislike of the element of chance
implied by the quantum theory:
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press, 1992, pp. 28-29
SOLO
1926
http://en.wikipedia.org/wiki/Max_Born
“Quantum mechanics is very impressive. But an inner
voice tells me that it is not the real thing. The theory
produce a good deal but hardly brings us closer to the
secret of the Old One. I am at all events convinced that
He does not play dice.”
83
84. 84
SOLO
Wavelike Behavior for Electrons
In 1927, the wavelike behavior of the electrons was demonstrated
by Davisson and Germer in USA and by G.P. Thomson in Scotland.
Quantum 1927
Clinton Joseph Davisson
1881 – 1958
Nobel Prize 1937
Lester Halbert Germer
1896 - 1971
85. 85
SOLO
Wavelike Behavior for Electrons
Quantum 1927
G.P. Thomson carried a series of experiments using an apparatus
called an electron diffraction camera. With it he bombarded very
thin metal and celluloid foils with a narrow electron beam. The
beam then was scattered into a series of rings.
George Paget Thomson
1892 – 1975
Nobel Prize 1937
Using these results G.P. Thomson proved
mathematically that the electron particles acted
like waves, for which he received the Nobel
Prize in 1937.
J.J. Thomson the father of G.P. proved that the electron is a
particle in 1897, for which he received the Nobel Prize in 1906.
Discovery of the Electron
Results of a double-slit-
experiment performed by
Dr. Tonomura showing
the build-up of an
interference pattern of
single electrons. Numbers
of electrons are 11 (a), 200
(b), 6000 (c), 40000 (d),
140000(e).
86. 86
SOLO
Optics HistoryRaman Effect 1928
http://en.wikipedia.org/wiki/Raman_scattering
http://en.wikipedia.org/wiki/Chandrasekhara_Venkata_Raman
Nobel Prize 1930
Chandrasekhara Venkata
Raman
1888 – 1970
Raman Effect was discovered in 1928 by C.V. Raman in
collaboration with K.S. Krishnan and independently by
Grigory Landsberg and Leonid Mandelstam.
Monochromatic light is scattered when hitting
molecules. The spectral analysis of the scattered light
shows an intense spectral line matching the wavelength of
the light source (Rayleigh or elastic scattering).
Additional, weaker lines are observed at wavelength
which are shifted compared to the wavelength of the light
source. These are the Raman lines.
Virtual
Energy States
IR
Absorbance
Excitation
Energy
Rayleigh
Scattering
Stokes - Raman
Scattering
Anti-Stokes -
Raman
Scattering
87. 87
SOLO
Stimulated Emission and Negative Absorption
1928
Rudolph W. Landenburg confirmed existence
of stimulated emission and Negative Absorption
Lasers History
Rudolf Walter Ladenburg (June 6, 1882 – April 6,
1952) was a German atomic physicist. He emigrated
from Germany as early as 1932 and became a Brackett
Research Professor at Princeton University. When the
wave of German emigration began in 1933, he was the
principal coordinator for job placement of exiled
physicist in the United States.
Albert Einstein and Rudolf Ladenburg,
Princeton Symposium, on the occasion of
Ladenburg's retirement, May 28, 1950.
Hedwig Kohn is in the background on the
left. Photo courtesy of AIP Emilio Segrè
Visual Archives.
Return to Table of Content
88. QUANTUM MECHANICS
SOLO
Wave Packet
A wave packet (or wave train) is a short "burst" or "envelope" of localized wave action
that travels as a unit. A wave packet can be analyzed into, or can be synthesized from, an
infinite set of component sinusoidal waves of different wavenumbers, with phases and
amplitudes such that they interfere constructively only over a small region of space, and
destructively elsewhere
Depending on the evolution equation, the wave packet's envelope may remain constant
(no dispersion, see figure) or it may change (dispersion) while propagating.
As an example of propagation without dispersion, consider wave solutions to the following
wave equation:
ψ
ψ 2
2
2
2
v
1
∇=
∂
∂
t
where v is the speed of the wave's propagation in a given medium.
The wave equation has plane-wave solutions ( ) ( )trki
eAtr ω
ψ −⋅
=
,
( ) v,/1111 2222
kkkkknPropagatioWaveofDirectionkzkykxkk zyxzyx =++=++= ω
A wave packet without dispersion A wave packet with dispersion
( ) ( ) ( )tcxiktcx
etx −+−−
= 0
2
,ψ
88
Run This
89. QUANTUM MECHANICS
SOLO
Wave Packet
The wave equation has plane-wave solutions ( ) ( )rkti
eAtr
⋅−−
= ω
ψ ,
( ) v,/1111 2222
kkkkknPropagatioWaveofDirectionkzkykxkk zyxzyx =++=++= ω
( )rptE
h
r
k
k
ktE
h
rkt
hv
⋅−
/
=⋅−=⋅−
=
=
122
/E
π
ω
νπω
( )
p
h
p
h
v
k
hhphv
/
=====
=/== 122
v
2
v
2/://v πλλ π
λ
ππω
( ) ( ) ( ) ( )rptEhirkti
eAeAtr
⋅−/−⋅−−
== /
, ω
ψ
where v is the velocity , v is the frequency, λ is the Wavelength of the Wave Packet.
The Energy E and Momentum p of the Particle are
( ) ( )
λ
π
λ
νπν
ππ
hh
phhE
hhhh
/
==/==
=/=/
2
&2
2/:2/:
de Broglie RelationEinstein Relation
The wave packet travels to the direction for ω = kv and to direction for ω = - kv.k1 k1−
89
90. QUANTUM MECHANICS
SOLO
Wave Packet
A wave packet is a localized disturbance that results from the sum of many different wave
forms. If the packet is strongly localized, more frequencies are needed to allow the
constructive superposition in the region of localization and destructive superposition
outside the region. From the basic solutions in one dimension, a general form of a wave
packet can be expressed as
( )
( )
( ) ( ) ( )
( ) ( ) tEhirptEhi
erepApd
h
tr //−
+∞
∞−
⋅−//−
=
/
= ∫
//3
3
2
1
,
ψ
π
ψ
( )
( )
( ) ( )
( )perrd
h
pA rphi
Φ=
/
= ∫
+∞
∞−
⋅/−
:0,
2
1 /3
3
ψ
π
The factor comes from Fourier Transform conventions. The amplitude
contains the coefficients of the linear superposition of the plane-wave solutions.
Using the Inverse Fourier Transform we obtain:
( )3
2/1 π ( )pA
( )
( )
( ) ( )
∫
+∞
∞−
⋅//
/
= rphi
epApd
h
r
/3
3
2
1
π
ψwhere
zyx pdpdpdpd =3
dzdydxrd =3
Define ( )
( )
( ) ( )
∫
+∞
∞−
⋅//−
/
=Φ rphi
etrrd
h
tp
/3
3
,
2
1
:, ψ
π
Wave Function in
Momentum Space 90
Return to Table of Content
91. ERWIN SCHRÖDINGER STAES THE NONRELATIVISTIC
QUANTUM WAVE EQUATION AND FORMULATES THE
QUANTUM MECHANICS. HE PROVES THAT WAVE AND
MATRIX FORMULATIONS ARE EQUIVALENT
1926
Following Max Planck's quantization of light (see black body radiation),
Albert Einstein interpreted Planck's quanta to be photons, particles of light,
and proposed that the energy of a photon is proportional to its frequency, one
of the first signs of wave–particle duality. Since energy and momentum are
related in the same way as frequency and wavenumber in special relativity, it
followed that the momentum p of a photon is proportional to its wavenumber k.
c
k
h
hwherekh
h
p
c πν
λ
π
πλ
νλ 22
:,
2
:
/=
===//==
Louis de Broglie hypothesized that this is true for all particles, even particles such as electrons. He
showed that, assuming that the matter waves propagate along with their particle counterparts,
electrons form standing waves, meaning that only certain discrete rotational frequencies about the
nucleus of an atom are allowed.[7]
These quantized orbits correspond to discrete energy levels, and
de Broglie reproduced the Bohr model formula for the energy levels. The Bohr model was based on
the assumed quantization of angular momentum:
hn
h
nL /==
π2
According to de Broglie the electron is described by a wave and a whole number of wavelengths
must fit along the circumference of the electron's orbit: n λ = 2 π r
http://en.wikipedia.org/wiki/Schr%C3%B6dinger_equation
Historical Background and Development
QUANTUM MECHANICS
Erwin Rudolf Josef
Alexander Schrödinger
(1887 – 1961)
Nobel Prize 1933
SOLO
91
92. ERWIN SCHRÖDINGER STAES THE NONRELATIVISTIC
QUANTUM WAVE EQUATION AND FORMULATES THE
QUANTUM MECHANICS. HE PROVES THAT WAVE AND
MATRIX FORMULATIONS ARE EQUIVALENT
1926
( ) ( ) ( )λνπ
νπω
νλ
ω
ψ /2
2
/v
v/
, xtixti
eAeAtx −−
=
=
−−
==
http://en.wikipedia.org/wiki/Schr%C3%B6dinger_equation
Historical Background and Development (continue – 1)
Following up on de Broglie's ideas, physicist Peter Debye made
an offhand comment that if particles behaved as waves, they
should satisfy some sort of wave equation. Inspired by Debye's
remark, Schrödinger decided to find a proper 3-dimensional wave
equation for the electron.
He was guided by William R. Hamilton's analogy between mechanics and optics, encoded in the
observation that the zero-wavelength limit of optics resembles a mechanical system — the
trajectories of light rays become sharp tracks that obey Fermat's principle, an analog of the
principle of least action.
For a general form of a Progressive Wave Function in + x direction with velocity v and frequency v:
The Energy E and Momentum p of the Particle are
λ
π
λ
νπν
hh
phhE
/
==/==
2
2
( ) ( ) ( )xptEhi
eAtx −/−
= /
,ψTherefore
QUANTUM MECHANICS
Erwin Rudolf Josef
Alexander Schrödinger
(1887 – 1961)
Nobel Prize 1933
SOLO
92
93. ERWIN SCHRÖDINGER STAES THE NONRELATIVISTIC
QUANTUM WAVE EQUATION AND FORMULATES THE
QUANTUM MECHANICS. HE PROVES THAT WAVE AND
MATRIX FORMULATIONS ARE EQUIVALENT
1926
Erwin Rudolf Josef
Alexander Schrödinger
(1887 – 1961)
Historical Background and Development (continue – 2)
We want to find the Differential Equation yielding the Wave Function .
We have
Wave Function:
( ) ( )
ψ
ψ
2
2
/
2
2
2
2
h
p
eA
h
p
x
xptEhi
/
−=
/
−=
∂
∂ −/−
At particle speeds small compared to speed of light c, the Total Energy E is the sum of the
Kinetic Energy p2
/2m and the Potential Energy V (function of position and time):
ψψψ
ψ
V
m
p
EV
m
p
E +=⇒+=
×
22
22
2
2
22
x
hp
∂
∂
/−=
ψ
ψ ti
h
E
∂
∂/
−=
ψ
ψ
cV
xm
h
ti
h
<<−
∂
∂/
=
∂
∂/
v
2 2
22
ψ
ψψ
QUANTUM MECHANICS
SOLO
( ) ( ) ( )xptEhi
eAtx −/−
= /
,ψ
93
94. ERWIN SCHRÖDINGER STAES THE NONRELATIVISTIC
QUANTUM WAVE EQUATION AND FORMULATES THE
QUANTUM MECHANICS. HE PROVES THAT WAVE AND
MATRIX FORMULATIONS ARE EQUIVALENT
1926
Erwin Rudolf Josef
Alexander Schrödinger
(1887 – 1961)
Historical Background and Development (continue – 3)
cV
xm
h
ti
h
<<−
∂
∂/
=
∂
∂/
v
2 2
22
ψ
ψψ
Non-Relativistic
One-Dimensional
Time Dependent
Schrödinger Equation
In the same way
cV
m
h
ti
h
<<−∇
/
=
∂
∂/
v
2
2
2
ψψ
ψ
Non-Relativistic
Three-Dimensional
Time Dependent
Schrödinger Equation
QUANTUM MECHANICS
SOLO
This is a Linear Partial Differential Equation. It is
also a Diffusion Equation (with an Imaginary
Diffusion Coefficient), but unlike the Heat
Equation, this one is also a Wave Equation given
the imaginary unit present in the transient term.
94
95. 1926 Schrödinger Equation
Time-dependent Schrödinger equation
(single non-relativistic particle)
A wave function that satisfies the
non-relativistic Schrödinger
equation with V=0. In other
words, this corresponds to a
particle traveling freely through
empty space. The real part of the
wave function is plotted here
Each of these three rows is a wave function which satisfies the
time-dependent Schrödinger equation for a harmonic
oscillator. Left: The real part (blue) and imaginary part (red)
of the wave function. Right: The probability distribution of
finding the particle with this wave function at a given position.
The top two rows are examples of stationary states, which
correspond to standing waves. The bottom row an example of
a state which is not a stationary state. The right column
illustrates why stationary states are called "stationary".
QUANTUM MECHANICS
Erwin Rudolf Josef
Alexander Schrödinger
(1887 – 1961)
Nobel Prize 1933
SOLO
95
96. Schrödinger Equation: Steady State Form
Using
ti
h
E
∂
∂/
−=
ψ
ψ
and the Time-dependent Schrödinger equations
cV
xm
h
ti
h
<<−
∂
∂/
=
∂
∂/
v
2 2
22
ψ
ψψ
Non-Relativistic
One-Dimensional
Time Dependent
Schrödinger Equation
cV
m
h
ti
h
<<−∇
/
=
∂
∂/
v
2
2
2
ψψ
ψ Non-Relativistic
Three-Dimensional
Time Dependent
Schrödinger Equationwe can write
( ) cVE
h
m
x
<<=−
/
+
∂
∂
v0
2
22
2
ψ
ψ
Non-Relativistic
One-Dimensional
Steady-State
Schrödinger Equation
( ) cVE
h
m
<<−
/
+∇ v
2
2
2
ψψ
Non-Relativistic
Three-Dimensional
Steady-State
Schrödinger Equation
QUANTUM MECHANICS
Erwin Rudolf Josef
Alexander Schrödinger
(1887 – 1961)
Nobel Prize 1933
1926
SOLO
96
Return to Table of Content
97. Operators in Quantum Mechanics
Since, according to Born, ψ*ψ represents Probability of finding the associated quantum particle in
a region we can compute the Expectation (Mean) Value of the Total Energy E and of the
Momentum p in that region using
( ) ( ) ( ) ( )∫
+∞
∞−
= xdtxtxEtxtE ,,,*
ψψ
( ) ( ) ( ) ( )∫
+∞
∞−
= dxtxtxptxtp ,,,*
ψψ
But those integrals can not compute exactly, since p (x,t) is unknown if x is know, according to
Uncertainty Principle. A way to find is by differentiating the Free-Particle Wave
Function
pandE
( ) ( )xptEhi
eA −/−
= /
ψ
( ) ( )
( ) ( )
ψ
ψ
ψ
ψ
E
h
i
eAE
h
i
t
p
h
i
eAp
h
i
x
xptEhi
xptEhi
/
−=
/
−=
∂
∂
/
=
/
=
∂
∂
−/−
−/−
/
/
Rearranging we obtain
ψψ
ψψ
t
hiE
xi
h
p
∂
∂
/=
∂
∂/
=
t
hiE
xi
h
p
∂
∂
/=
∂
∂/
=
:ˆ
:ˆ
QUANTUM MECHANICS
SOLO
We can look at p and E as Operators on ψ
(the symbol means “Operator”)∧
Note: One other way to arrive to this result by manipulating the integrals will be given in
the following presentations.
97
98. Operators in Quantum Mechanics (continue – 1)
We obtained
Moment Operatorxi
h
p
∂
∂/
=:ˆ
t
hiE
∂
∂
/=:ˆ Total Energy Operator
Although we derived those operators for free particles, they are entire general results, equivalent
to Schrödinger Equation. To see this let write the Operator Equation
Operator
Energy
Potential
Operator
Energy
Kinetic
Operator
Energy
Total
VTE ˆˆˆ +=
2
2222
22
1
2
ˆ
xm
h
xi
h
mm
p
T
Operator
Energy
Kinetic ∂
∂/
−=
∂
∂/
==We have
V
xm
h
t
hiE
Operator
Energy
Total
+
∂
∂/
−=
∂
∂
/= 2
22
2
ˆ
Applying this Operator on Wave Function ψ we recover the Schrödinger Equation
ψ
ψψ
V
xm
h
t
hi +
∂
∂/
−=
∂
∂
/ 2
22
2
The two descriptions (Operator and Schrödinger’s) are equivalent.
QUANTUM MECHANICS
SOLO
98
99. QUANTUM MECHANICS
Operators in Quantum Mechanics (continue – 3)
We obtained
Moment Operatorxi
h
p
∂
∂/
=:ˆ
t
hiE
∂
∂
/=:ˆ Total Energy Operator
Because p and E can be replaced by their Operators in an equation, we can use those Operators
to obtain Expectation Values for p and E.
∫∫∫
∞+
∞−
∞+
∞−
∞+
∞− ∂
∂/
=
∂
∂/
== dx
xi
h
dx
xi
h
dxpp
ψ
ψψψψψ ***
ˆ
∫∫∫
∞+
∞−
∞+
∞−
∞+
∞− ∂
∂
/=
∂
∂
/== xd
x
hixd
x
hixdEE
ψ
ψψψψψ *** ˆ
Let define the Hamiltonian Operator V
xm
h
H ˆ
2
:ˆ
2
22
+
∂
∂/
−=
Schrödinger Equation in Operator form is ψψ EH ˆˆ =
This Equation has a form of an Eigenvalue Equation of the Operator with Eigenvalue Ê
and Eigenfunction as the Wavefunction ψ.
Hˆ
SOLO
99
100. Dirac bracket notation
Paul Adrien Maurice
Dirac
( 1902 –1984)
A elegant shorthand notation for the integrals used to define Operators
was introduced by Dirac in 1939
onWavefunctiket nn ψψ ⇔""
Instead of dealing with Wavefunctions ψn, we defined a related Quantum “State”,
denoted |ψ› which is called a “ket”, “ket vector”, “state” or “state vector”.
The complex conjugate of |ψ› is called the “bra” and is denoted by ‹ψ|.
onWavefunctibra nn
*
"" ψψ ⇔
ket
m
bra
n ψψ
When a “bra” is combined with a “ket” we obtain a “bracket”.
The following integrals are represented by “bra” and “ket”
mnmn AdA ψψτψψ |ˆ|ˆ*
≡∫
mnmn d ψψτψψ |*
≡∫
nnnnnn aAaA ψψψψ =⇔= ˆˆ
Operators in Quantum Mechanics (continue – 5)
( ) ( ) ( ) ( ) mnmnmnmnmn AAdAAdA ψψψψτψψψψτψψ |ˆ|ˆ|ˆ|ˆˆ ***
==== ∫∫
nnnnnn aAaA ψψψψ ****** ˆˆ =⇔=
QUANTUM MECHANICS
SOLO
100
Return to Table of Content
101. QUANTUM THEORIES
HILBERT SPACE AND QUANTUM MECHANICS.
Ernst Pascual Jordan
(1902 – 1980)
Nazi Physicist
http://en.wikipedia.org/wiki/Matrix_mechanics
Born had also learned Hilbert’s theory of integral
equations and quadratic forms for an infinite number of
variables as was apparent from a citation by Born of
Hilbert’s work “Grundzüge einer allgemeinen Theorie
der Linearen Integralgleichungen” published in 1912.
Jordan, too was well equipped for the task. For a
number of years, he had been an assistant to Richard
Courant at Göttingen in the preparation of Courant and
David Hilbert’s book Methoden der mathematischen
Physik I, which was published in 1924. This book,
fortuitously, contained a great many of the
mathematical tools necessary for the continued
development of quantum mechanics.
In 1926, John von Neumann became assistant to David
Hilbert, and he would coin the term Hilbert Space to
describe the algebra and analysis which were used in the
development of quantum mechanics
Max Born
(1882–1970)
Nobel Price 1954
John von Neumann
(1903 –1957)
David Hilbert
(1862 –1943)
Richard Courant
(1888 –1972)
SOLO
101
102. 102
Functional AnalysisSOLO
Vector (Linear) Space: E is a Linear Space if Addition and Scalar Multiplication are Defined
Addition
Scalar Multiplication
From those equations follows:
The null element 0 ∈ E is unique.
The addition inverse |η› of |ψ›,
(|ψ›+|η›= 0) is unique.
E∈∀=⋅ ψψ 00
|η› = (-1) |ψ› is the multiplication
inverse of |ψ›.
αβ −=
E∈∀+=+ χψψχχψ ,1 Commutativity
ψψ +=+∈∃ 00..0 tsE3 Identity
0.. =+∈∃∈∀ χψχψ tsEE4 Inverse
E∈∀=⋅ ψψψ15 Normalization
( ) ( ) βαψψβαψβα ,& ∀∈∀= E6
Associativity
8 ( ) αηψηαψαηψα ∀∈∀+=+ &, E Distributivity
7 ( ) βαψψβψαψβα ,& ∀∈∀+=+ E Distributivity
2 Associativity( ) ( ) E∈∀++=++ ηχψηψχηχψ ,,
The same apply for “bra” ‹ψ| the “conjugate” of the “ket” |ψ›.
See also “Functional Analysis ” Presentation for a detailed description
103. 103
Functional AnalysisSOLO
Vector (Linear) Space: E is a Linear Space if Addition and Scalar Multiplication are Defined
Linear Independence, Dimensionality and Bases
∈≠
=
⇒=∑=
CsomefortrueifDependentLinear
allifonlytrueiftIndependenLinear
i
in
i ii
0
0
01
α
α
ψα
A set of vectors |ψi› (i=1,…,n) that satisfy the relation
Dimension of a Vector Space E , is the maximum number N of Linear Independent Vectors
in this space. Thus, between any set of more that N Vectors |ψi› (i=1,2,…,n>N), there exist a
relation of Linear Dependency.
Any set of N Linearly Independent Vectors |ψi› (i=1,2,…,N), form a Basis of the Vector
Space E ,of Dimension N, meaning that any vector |η› ∈ E can be written as a Linear
Combination of those Vectors.
Ci
N
i ii ∈≠= ∑=
αψαη 01
In the case of an Infinite Dimensional Space (N→∞), the space will be defined by a
“Complete Set” of Basis Vectors. This is a Set of Linearly Independent Vectors of the
Space, such that if any other Vector of the Space is added to the set, there will exist a
relation of Linear Dependency to the Basis Vectors.
104. SOLO Functional Analysis
Use of bra-ket notation of Dirac for Vectors.
ketbra
TransposeConjugateComplexHfefeefef HH
−
=⋅==⋅= ,|
operatorkete
operatorbraf
|
|
Paul Adrien Maurice Dirac
(1902 – 1984)
Assume the are a basis and the a reciprocal basis for the Hilbert
space. The relation between the basis and the reciprocal basis is described, in
part, by:
je| |if
ketbra
ji
ji
efef jij
H
iji
−
=
≠
===
1
0
| ,δ
104
The Inner Product of the Vectors f and e is defined as
Inner Product Using Dirac Notation
( ) ( )**
& ψψψψ ==
To every “ket” corresponds a “bra”.
105. 105
Functional AnalysisSOLO
Inner Product Using Dirac Notation
If E is a complex Linear Space, for the Inner Product (bracket) < | >
between the elements (a complex number) is defined by:
E∈∀ 321 ,, ψψψ
*
1221 || >>=<< ψψψψ1 Commutative Law
Using to we can show that:1 4
If E is an Inner Product Space, than we can induce the Norm: [ ] 2/1
111 , ><= ψψψ
2 Distributive Law><+>>=<+< 3121321 ||| ψψψψψψψ
3 C∈><>=< αψψαψψα 2121 ||
4
00|&0| 11111 =⇔>=<≥>< ψψψψψ
( ) ( ) ( )
><+><=><+><=>+<=>+< 1312
1
*
31
*
21
2
*
321
1
132 |||||| ψψψψψψψψψψψψψψ
( ) ( ) ( )
><=><=><=>< 21
*
1
*
12
*
3
*
12
1
21 |||| ψψαψψαψψαψαψ
( ) ( )
*
1
1
111
2
11 |000|0|0|00|0| ><=>=<⇒><+><=>+>=<< ψψψψψψ
106. 106
Functional AnalysisSOLO
Inner Product
ηψηψ ≤>< |
Cauchy, Bunyakovsky, Schwarz Inequality known as Schwarz Inequality
Let |ψ›, |η› be the elements of an Inner Product space E, than :
x
y
><=
><
y
y
x
y
yx
,
,
y
y
y
y
xxy
y
yx
x ><−=
><
− ,
,
2
0|||||
2*
≥><+><+><+>>=<++< ηηλψηληψλψψηλψηλψ
Assuming that , we choose:0|
2/1
≠= ηηη
><
><
−=
ηη
ηψ
λ
|
|
we have:
0|
|
|
|
||
|
||
| 2
2*
≥><
><
><
+
><
><><
−
><
><><
−>< ηη
ηη
ηψ
ηη
ψηηψ
ηη
ηψηψ
ψψ
which reduce to:
0
|
|
|
|
|
|
|
222
≥
><
><
+
><
><
−
><
><
−><
ηη
ηψ
ηη
ηψ
ηη
ηψ
ψψ
or:
><≥⇔≥><−><>< ηψηψηψηηψψ |0|||
2
q.e.d.
Augustin Louis Cauchy
)1789-1857(
Viktor Yakovlevich
Bunyakovsky
1804 - 1889
Hermann Amandus
Schwarz
1843 - 1921
Proof:
107. 107
Functional Analysis
SOLO
Hilbert Space
A Complete Space E is a Metric Space (in our case ) in which every
Cauchy Sequence converge to a limit inside E.
( ) 2121, ψψψψρ −=
David Hilbert
1862 - 1943
A Linear Space E is called a Hilbert Space if E is an Inner Product Space that is
complete with respect to the Norm induced by the Inner Product ||ψ1||=[< ψ1, ψ1>]1/2
.
Equivalently, a Hilbert Space is a Banach Space (Complete Metric Space) whose
Norm is induced by the Inner Product ||ψ1||=[< ψ1, ψ1>]1/2
.
Orthogonal Vectors in a Hilbert Space:
Two Vectors |η› and |ψ› are Orthogonal if 0|| == ηψψη
Theorem: Given a Set of Linearly Independent Vectors in a Hilbert
Space |ψi› (i=1,…,n) and any Vector |ψm› Orthogonal to all |ψi›,
than it is also Linearly Independent.
Proof: Suppose that the Vector |ψm› is Linearly Dependent on |ψi› (i=1,…,n)
∑=
=≠
n
i iim 1
0 ψαψ
But ∑=
==≠
n
i imimm 1
0
00
ψψαψψ
We obtain a inconsistency, therefore |ψm› is Linearly Independent on |ψi› (i=1,…,n)
Therefore in a Hilbert Space, of Finite or Infinite Dimension, by finding the Maximum
Set of Orthogonal Vectors we find a Basis that “Complete” covers the Space.
q.e.d.
108. 108
Functional Analysis
SOLO
Hilbert Space
Orthonormal Sets
Let |ψ1›, |ψ2›, ,…, |ψn›, denote a set of elements in the Hilbert Space H.
( )
><><><
><><><
><><><
=
nnnn
n
n
nG
ψψψψψψ
ψψψψψψ
ψψψψψψ
ψψψ
,,,
,,,
,,,
:,,,
21
22212
12111
21
Jorgen Gram
1850 - 1916
Define the Gram Matrix of the set:
Theorem: A set of functions |ψ1›, |ψ2›, ,…, |ψn› of the Hilbert Space H is linearly dependent
if and only if the Gram determinant of the set is zero.
zeroequalallnot inn αψαψαψα 02211 =+++ Proof: Linearly Dependent Set:
Multiplying (inner product) this equation consecutively by |ψ1›, |ψ2›, ,…, |ψn›, we obtain:
( ) 0,,,det
0
0
0
,,,
,,,
,,,
21
2
1
21
22212
12111
=⇔
=
><><><
><><><
><><><
n
Solution
nontrivial
nnnnn
n
n
G ψψψ
α
α
α
ψψψψψψ
ψψψψψψ
ψψψψψψ
q.e.d.
109. 109
Functional Analysis
SOLO
Hilbert Space
Orthonormal Sets (continue – 2)
Theorem: A set of functions |ψ1›, |ψ2›, ,…, |ψn›, of the Hilbert space H is linearly dependent
if and only if the Gram Determinant of the Set is zero.
Proof: The Gram Matrix of an Orthogonal Set has only nonzero diagonal; therefore
Determinant G (|ψ1›, |ψ2›, ,…, |ψn› ).=║|ψ1 ›║2
║ |ψ2 › ║2
… ║ |ψn › ║2
≠ 0, and the Set is Linearly
Independent.
q.e.d.
Corollary: The rank of the Gram Matrix equals the dimension of the Linear Manifold
L (|ψ1›, |ψ2›, ,…, |ψn› ). If Determinant G (ψ1›, |ψ2›, ,…, |ψn›) is nonzero, the Gram Determinant of
any other Subset is also nonzero.
Definition 1: Two elements |ψ›,|η› of a Hilbert Space H are said to be orthogonal if <ψ|η>=0.
Definition 2: Let S be a nonempty Subset of a Hilbert Space H. S is called an Orthogonal
Set if |ψ›┴|η› for every pair |ψ›,|η› є S and |ψ› ≠ |η›. If in addition ║ |ψ›║=1 for every |ψ› є S, then
S is called an Orthonormal Set.
Lemma: Every Orthogonal Set is Linearly Independent. If |η› is Orthogonal to every
element of the Set (|ψ1›, |ψ2›, ,…, |ψn› ), then |η› is Orthogonal to Manifold L (|ψ1›, |ψ2›, ,…, |ψn› ).
If then for every we have:nii ,,2,10, =∀=>< ψη ( )n
n
i
ii L ψψψαχ ,,1
1
∈= ∑=
0,,
1
=><>=< ∑=
n
i
ii
ψηαχη
110. 110
Functional AnalysisSOLO
Hilbert Space
Orthonormal Sets (continue – 3)
Gram-Schmidt Orthogonalization Process
Jorgen Gram
1850 - 1916
Erhard Schmidt
1876 - 1959
Let Ψ=(|ψ1›, |ψ2›, ,…, |ψn› ) any finite Set of Linearly Independent Vectors
and L (|ψ1›, |ψ2›, ,…, |ψn› ) the Manifold spanned by the Set Ψ.
The Gram-Schmidt Orthogonalization Process derive a Set
(|e1›, |e2›, ,…, |en› ) of Orthonormal Elements from the Set Ψ.
11 : ψη =
1
11
21
22
11
21
21
1121212112122
,
,
,
,
,,,0:
η
ηη
ψη
ψη
ηη
ψη
α
ηηαψηηψαψη
><
><
−=⇒
><
><
=⇒
><−>>=<=<⇒−= y
∑
∑∑
−
=
−
=
−
=
><
><
−=⇒
><
><
=⇒
><−>>=<=<⇒−=
1
1
1
1
1
1
,
,
,
,
,,,0:
i
j
j
ji
ji
ii
kk
ki
ik
i
j
jkkjikki
i
j
jijii
kj
η
ηη
ηψ
ψη
ηη
ηψ
α
ηηαψηηηηαψη
δ
111. 111
Functional AnalysisSOLO
Hilbert Space
Orthonormal Sets (continue – 4)
Gram-Schmidt Orthogonalization Process (continue)
Jorgen Gram
1850 - 1916
Erhard Schmidt
1876 - 1959
11 : ψη =
1
11
21
22
,
,
: η
ηη
ψη
ψη
><
><
−=
∑
−
= ><
><
−=
1
1 ,
,
:
i
j
j
ji
ji
ii η
ηη
ηψ
ψη
2/1
11
1
1
,
:
><
=
ηη
η
e
Orthogonalization Normalization
∑
−
= ><
><
−=
1
1 ,
,
:
n
j
j
ji
jn
nn η
ηη
ηψ
ψη
2/1
22
2
2
,
:
><
=
ηη
η
e
2/1
,
:
><
=
ii
i
ie
ηη
η
2/1
,
:
><
=
nn
n
ne
ηη
η
112. 112
Functional AnalysisSOLO
Hilbert Space
Discrete |ei› and Continuous |wα› Orthonormal Bases
From those equations we obtain
ijji ee δ=|
The Orthonormalization Relation
( )'| ' ααδαα −=ww
A Vector |ψ› will be represented by
( ) ψψψψ ∑∑∑∑ ====
====
n
i ii
n
i ii
n
i ii
n
i ii eeeeeeec 1111
||
( )ψαψαψααψ αααααααα ∫∫∫∫ ==== wwdwwdwwdwcd
i
n
j jiji
n
j jj ceeceec
ij
==⇒= ∑∑ == 11
δ
ψψ
( )
α
ααδ
αααααα αψαψ cwwcdwwcd ==⇒= ∫∫
−
'
'''''
Therefore
Iee
n
i ii =∑=1
Iwwd =∫ ααα
The Closure Relations
I – the Identity Operator
(its action on any state
leaves it unchanged).
α- a real number or vector, not complex-valued
The Vectors in Hilbert Space can be Countable (Discrete) or Uncountable (Continuous).
113. 113
Functional AnalysisSOLO
Hilbert Space
Series Expansions of Arbitrary Functions
Definitions:
Approximation in the Mean by an Orthonormal Series |ψ1›, |ψ2›, ,…, |ψn› :
Let |η› be any function. The numbers:
are called the Expansions Coefficients or Components of |η› with respect to the given
Orthonormal System
nn ψηα ,:=
From the relation
we obtain
or 2
1
2
, ηηηα =≤∑=
n
i
i
0|
11
2
1
≥
−
−=
− ∑∑∑ ===
n
i
ii
n
i
ii
n
i
ii ψαηψαηψαη
0|2|
|||
1
*
1
*
1
*
1
*
11
*
≥−=+−=
+−−
∑∑∑
∑∑∑
===
===
n
i
ii
n
i
ii
n
i
ii
n
i
ii
n
i
ii
n
i
ii
ααηηααααηη
ααηψαψηαηη
114. 114
Functional AnalysisSOLO
Hilbert Space
Series Expansions of Arbitrary Functions
Approximation in the Mean by an Orthonormal Series |ψ1›, |ψ2›, |ψ3›,… :
Let |η› be any function. The numbers:
are called the Expansions Coefficients or Components of |η› with respect to the given
Orthonormal System
nnc ψη,:=
2
1
2
ηα ≤∑=
n
i
i
Since the sum on the right is independent on n, is true also
for n →∞, we have 2
1
2
ηα ≤∑
∞
=i
i Bessel’s Inequality
Bessel’s Inequality is true for every Orthonormal System. It proves that the sum of the
square of the Expansion Coefficients always converges.
Friedrich Wilhelm
Bessel
1784 - 1846
115. 115
Functional AnalysisSOLO
Hilbert Space
Series Expansions of Arbitrary Functions
Approximation in the Mean by an Orthonormal Series |ψ1›, |ψ2›, |ψ3›,… :
If for a given Orthonormal System |ψ1›, |ψ2›, |ψ3›,… any piecewise continuous function |η›
can be approximated in the mean to any desired degree of accuracy ε by choosing a n large
enough ( n>N (ε) ), i.e.:
( )εεψαη Nnfor
n
i
ii >≤− ∑=1
then the Orthonormal System |ψ1›, |ψ2›, |ψ3›,… is said to be Complete.
For a Complete Orthonormal System |ψ1›, |ψ2›, |ψ3›,… the Bessel’s Inequality becomes an
Equality:
2
1
2
ηα =∑
∞
=i
i
Parseval’s Equality applies for
Complete Orthonormal Systems
This relation is known as the “Completeness Relation”.
( )( ) ∑∑∑∑∑
∞
=
∞
=
∞
=
∞
=
∞
=
+++=++=+
++=++=+
1
*
1
*
1
*
1
*
1
,2,
i
ii
i
ii
i
ii
i
ii
i
iiii dcdc βββαβαααχη
χχηηχηχηχη
∑∑
∞
=
∞
=
+=
1
*
1
*
,2
i
ii
i
ii βαβαχη
A more general form, for , can be derived as follows:∑∑
∞
=
∞
=
==
1
*
1
*
&
i
ii
i
ii ββχααη
Marc-Antoine
Parseval des Chênes
1755 - 1836
116. Functional AnalysisSOLO
Hilbert Space
Linear Operators in Hilbert Space
An Operator L in Hilbert Space acting on a Vector |ψ›, produces a Vector |η›.
ψη L
=
L
ψη =
The arrow over L means that the Operator is acting on the Vector on the Left, ‹ψ|.
An Operator L is Linear if it Satisfies ( ) CLLL ∈+=+ βαηβψαηβψα ,
Consider the quantities . They are in general not equal.( ) ( ) ψηψη || LandL
Eigenvalues and Eigenfunction of a Linear Operator are defined by
CL ∈= λψλψ
The Eigenfunction |ψ› is transformed by the Operator L into multiple of itself, by the
Eigenvalue λ. The conjugate equation is
( ) CLL ∈== λψλψψ **
The corresponding Operator which transforms the “bra” ‹ψ| , called the
Adjoint Operator, is
L
The arrow over means that the Operator is acting on the Vector
on the Right, |ψ›.
L
116
117. Functional AnalysisSOLO
Hilbert Space
Adjoint or Hermitian Conjugates Operators
An Operator L1 in Hilbert Space acting on a Vector |ψ›, produces a Vector |η›.
Let have another Operator in Hilbert Space acting on the Vector |η›, and produce a Vector |χ›.
( ) 1111 LLorLL
=⇔
1L
Operator ψη 1L
=
1L
Adjoint Operator 1L
ψη =
22 & LL
ηχηχ ==
Therefore
2112 & LLLL
ψχψχ ==
( ) 21122112 LLLLorLLLL
=⇔
The Adjoint of a Product of Operators is obtained by Reversing the order of the
Product of Adjoint of Operators.
117
118. Functional AnalysisSOLO
Hilbert Space
ILLLLILLLL ==== −−−− 1111
&
Inverse Operator
Given
ψη L
= L
ψη =
The Inverse Operator on is the Operator that will return .ψL
ψ1−
L
ψψη == −−
LLL
11
Therefore
ηψη ==−
LLL
1
The Inverse Operator on is the Operator that will return .L
ψ ψ1−
L
ψψη == −− 11
LLL
In the same way
ηψη ==−
LLL
1
Not all Operators have an Inverse.
118
119. Functional AnalysisSOLO
Hilbert Space
( ) ( ) ( ) ηψηψψηψη ,|||
*
∀== LLL
Hermitian Operator
In Quantum Mechanics the Operators for which are equal present a
great importance. They are called Hermitian or Self-Adjoint Operators.
( ) ( ) ψηψη || LandL
Properties of Hermitian Operators
From the definition we can see that the direction of the arrow is not important and we can
write
( ) ( ) ηψηψψηψηψη ,||||:||
*
∀=== LLLL
1
2 All the Eigenvalues of a Hermitian Operator are Real
( ) ( ) ( ) ( ) ( ) ψηψηψηηψψη |||||| *******
LLLLL
====
( ) ψψλψψλψλψ || =⇒∈= LCL
( ) ψψλψψλψλψ || **
=⇒∈= LCL
Hermitian Operator : ( ) ( ) ( ) *
0
*
0||| λλψψλλψψψψ =⇒=−⇒=
>
LL
An Operator is Hermitian if it is equal to its Adjoint:
Hermitian or Self-Adjoint Operators ( ) LLL
==
119
120. Functional AnalysisSOLO
Hilbert Space
( ) ( ) ( ) ηψηψψηψη ,|||
*
∀== LLL
Hermitian Operator
In Quantum Mechanics the Operators for which are equal present a
great importance. They are called Hermitian Operators.
( ) ( ) ψηψη || LandL
Properties of Hermitian Operators
If all the Eigenvalues of an Operator are Real the Operator is Hermitian3
iiii
i
iiiiiiii
iiiiiiii
iii
iii
LL
L
L
i
L
L ii
ψψψψ
ψψλψψλψψ
ψψλψλψψψ
ψλψ
ψλψ λλ
||
|||
||| *
*
*
=⇒
==
==
⇒∀
=
= =
∀
Hermitian Operator
120
121. Functional AnalysisSOLO
Hilbert Space
( ) ( ) ( ) ηψηψψηψη ,|||
*
∀== LLL
Hermitian Operator
In Quantum Mechanics the Operators for which are equal present a
great importance. They are called Hermitian Operators.
( ) ( ) ψηψη || LandL
Properties of Hermitian Operators
4 All the Eigenfunctions of a Hermitian Operator corresponding to different Eigenvalues
are Orthogonal, the others can be Orthogonalized using the Gram-Schmidt Procedure.
Therefore for a Hermitian Operator we can obtain a “complete Set” of Orthogonal
(and Linearly Independent) Eigenfunctions
==
=
⇒
==
==
**
*
|||
||
nmmmnmmn
nmnnm
mmmmm
nnnnn
L
L
L
L
ψψλψψλψψ
ψψλψψ
λλψλψ
λλψλψ
If |ψn› and |ψm› are two Eigenfunctions of the Hermitian Operator L, with eigenvalues λn
and λm, respectively
Hermitian Operator: nmmnmnmnnm LL ψψλψψλψψψψ |||| =⇒=
If λm ≠ λn this equality is possible only if ψn and ψm are Orthogonal 0| =nm ψψ
If λm = λn we can use the Gram-Schmidt Procedure to obtain a new Eigenfunction
Orthogonal to |ψn›.
n
nn
mn
mm ψ
ψψ
ψψ
ψψ
−=
|
|
:~ 0|
|
|
|~| =
−= nn
nn
mn
mnmn ψψ
ψψ
ψψ
ψψψψ
The Hermitian Operators have Real Eigenvalues and Orthogonal Eigenfunctions.
λm ≠ λn
121
122. Functional AnalysisSOLO
Hilbert Space
1−
=UU
Unitary Operator
Properties of Unitary Operators
A Unitary Operator U is defined by the relation where I is the Identity Operator.IUUUU ==
A Unitary Matrix is such that it’s Adjoint is equal to it’s Inverse.
All Eigenvalues of a Unitary Matrix have absolute values equal to 1.
Suppose |ψi› is an Eigenfunction and λi is the corresponding Eigenvalue of a Unitary Operator.
iUU
U
U
iiiiiii
I
i
iii
iii
∀=⇒=⇒
=
=
1| **
*
λλψψλλψψ
ψλψ
ψλψ
1
2
ψηψηψη ,| ∀=
I
UU
For all <η| and |ψ› the Inner Product of equals‹η|ψ›ψη UandU
3 ψψψ ∀=U
ψψψψψψψψ ∀===
2/1
2/1
2/1
||
I
UUUUU
122
Beiser, “Perspectives of Modern Physics”, McGraw Hill-Kogakusha, International Student Edition, 1961, Ch. 6
T. Hey, P. Walters, “The Quantum Universe”, Cambridge University Press, 1987, pp.39-40
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Beiser, “Perspectives of Modern Physics”, McGraw Hill-Kogakusha, International Student Edition, 1961, Ch.5-6
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Beiser, “Perspectives of Modern Physics”, McGraw Hill-Kogakusha, International Student Edition, 1961, Ch.5-6
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Beiser, “Perspectives of Modern Physics”, McGraw Hill-Kogakusha, International Student Edition, 1961, Ch.5-6
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Beiser, “Perspectives of Modern Physics”, McGraw Hill-Kogakusha, International Student Edition, 1961, Ch.5-6
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Beiser, “Perspectives of Modern Physics”, McGraw Hill-Kogakusha, International Student Edition, 1961, Ch.5-6
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Arthur Beiser, “Perspectives of Modern Physics”, McGraw-Hill, International Student Edition, 1969, “Schrödinger’s Equation: Time-dependent Form”, pp. 153-156
Arthur Beiser, “Perspectives of Modern Physics”, McGraw-Hill, International Student Edition, 1969, “Schrödinger’s Equation: Time-dependent Form”, pp. 153-156
Arthur Beiser, “Perspectives of Modern Physics”, McGraw-Hill, International Student Edition, 1969
Arthur Beiser, “Perspectives of Modern Physics”, McGraw-Hill, International Student Edition, 1969
Arthur Beiser, “Perspectives of Modern Physics”, McGraw-Hill, International Student Edition, 1969
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977, Ch. II, “The Mathematical Tools of Quantum Mechanics”
Arthur Beiser, “Perspectives of Modern Physics”, McGraw-Hill, International Student Edition, 1969
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977, pg.122
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B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.96, 213
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Courant, R., Hilbert, D., “Methods of Mathematical Physics”, Vol. I, Interscience Publishers, 1953
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.96, 213
Courant, R., Hilbert, D., “Methods of Mathematical Physics”, Vol. I, Interscience Publishers, 1953
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.96, 213
Courant, R., Hilbert, D., “Methods of Mathematical Physics”, Vol. I, Interscience Publishers, 1953
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.96, 213
Courant, R., Hilbert, D., “Methods of Mathematical Physics”, Vol. I, Interscience Publishers, 1953
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.96, 213
Courant, R., Hilbert, D., “Methods of Mathematical Physics”, Vol. I, Interscience Publishers, 1953
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.96, 213
Courant, R., Hilbert, D., “Methods of Mathematical Physics”, Vol. I, Interscience Publishers, 1953
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.96, 213
Courant, R., Hilbert, D., “Methods of Mathematical Physics”, Vol. I, Interscience Publishers, 1953
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.96, 213
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977, Ch. II, “The Mathematical Tools of Quantum Mechanics”
Arthur Beiser, “Perspectives of Modern Physics”, McGraw-Hill, International Student Edition, 1969
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.96, 213
4J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977, Ch. II, “The Mathematical Tools of Quantum Mechanics”
Arthur Beiser, “Perspectives of Modern Physics”, McGraw-Hill, International Student Edition, 1969
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.96, 213
C. Cohen-Tannoudji, B. Diu, F. Laloe, “Quantum Mechanics”, John Wiley & Sons, 1977
Jim Baggott, “The Meaning of Quantum Theory”, Oxford University Press, 1992, pp. 42-48
C. Cohen-Tannoudji, B. Diu, F. Laloe, “Quantum Mechanics”, John Wiley & Sons, 1977
Jim Baggott, “The Meaning of Quantum Theory”, Oxford University Press, 1992, pp. 42-48
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, John Wiley & Sons, 1977
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000
http://en.wikipedia.org/wiki/Wave_packet
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000
http://en.wikipedia.org/wiki/Probability_current
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977, Ch. II, “The Mathematical Tools of Quantum Mechanics”
Arthur Beiser, “Perspectives of Modern Physics”, McGraw-Hill, International Student Edition, 1969
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.96, 213
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, John Wiley & Sons, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.96, 213
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, John Wiley & Sons, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.96, 213
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, John Wiley & Sons, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.96, 213
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, John Wiley & Sons, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.96, 213
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, John Wiley & Sons, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.96, 213
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, John Wiley & Sons, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.96, 213
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, John Wiley & Sons, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.96, 213
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, John Wiley & Sons, 1977
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.232-233
P.R. Wallace, “Mathematical Analysis of Physical Problems”, Dover Publications, 1984, pp. 472-474
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, John Wiley & Sons, 1977, pp. 308-311
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http://n.wikipedia.org/wiki/Schrödinger equation- Wikipedia, the free encyclopedia.mht
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P.R. Wallace, “Mathematical Analysis of Physical Problems”, Dover Publications, 1984, pp. 468-470
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, John Wiley & Sons, 1977, pp. 312-314
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.238-240
P.R. Wallace, “Mathematical Analysis of Physical Problems”, Dover Publications, 1984, pp. 468-470
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, John Wiley & Sons, 1977, pp. 312-314
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp.238-240
P.R. Wallace, “Mathematical Analysis of Physical Problems”, Dover Publications, 1984, pp. 468-470
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, John Wiley & Sons, 1977, pp. 312-314
http://en.wikipedia.org/wiki/Ehrenfest_theorem
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977, pp. 242-244
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp. 97-100
http://en.wikipedia.org/wiki/Ehrenfest_theorem
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977, pp. 242-244
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp. 97-100
http://en.wikipedia.org/wiki/Ehrenfest_theorem
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977, pp. 242-244
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp. 97-100
http://en.wikipedia.org/wiki/Ehrenfest_theorem
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977, pp. 242-244
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp. 97-100
http://en.wikipedia.org/wiki/Ehrenfest_theorem
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977, pp. 242-244
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp. 97-100
http://en.wikipedia.org/wiki/Ehrenfest_theorem
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977, pp. 242-244
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp. 97-100
http://en.wikipedia.org/wiki/Ehrenfest_theorem
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977, pp. 242-244
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp. 97-100
http://en.wikipedia.org/wiki/Ehrenfest_theorem
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977, pp. 242-244
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp. 97-100
http://en.wikipedia.org/wiki/Ehrenfest_theorem
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, Volume I, Wiley Interscience, 1977, pp. 242-244
B.H. Bransden, C.J. Joachain, “Quantum Mechanics”, 2nd Ed., Prentice Hall, 1989,2000, pp. 97-100
http://en.wikipedia.org/wiki/Pauli_exclusion_principle
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, John Wiley & Sons, 1977
http://en.wikipedia.org/wiki/Pauli_exclusion_principle
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, John Wiley & Sons, dden from occupying
http://en.wikipedia.org/wiki/Pauli_exclusion_principle
C. Cohen-Tannoudji, B. Diu, F. Laloë, “Quantum Mechanics”, John Wiley & Sons, dden from occupying
http://en.wikipedia.org/wiki/Klein%E2%80%93Gordon_equation
R.H. Landau, “Quantum Mechanics II, A Second Course in Quantum Mechanics”, John Wiley & Sons, 1996
http://en.wikipedia.org/wiki/Maxwell&apos;s_equations
L.D. Landau, E.M. Lifshitz, “The Classical Theory of Fields”, 4th Revised English Edition, Pergamon Press, 1975
J.D. Jackson, “Classical Electrodynamics”, John Wiley & Sons, 3th Ed., 1999
http://en.wikipedia.org/wiki/Maxwell&apos;s_equations
L.D. Landau, E.M. Lifshitz, “The Classical Theory of Fields”, 4th Revised English Edition, Pergamon Press, 1975
J.D. Jackson, “Classical Electrodynamics”, John Wiley & Sons, 3th Ed., 1999
http://en.wikipedia.org/wiki/Pauli_equation
T. Frankel, “The Geometry of Physics, An Introduction”, Cambridge University Press, 1997, Chapter 19, “The Dirac Equation”, pp.491-521
R.P. Feynman, “Quantum Electrodynamics”, W.A. Benjamin, Inc., New York, 1961
P.R. Wallace, “Mathematical Analysis of Physical Problems”, Dover Publications, 1972, 1984, ch. 5, Sec. 20 “Spin of Scalar Vector Field”, pp. 288 – 291
A.O. Barut, “Electrodynamics and Classical Theory of Fields and Particles”, Dover, 1964, 1980, pp.22-29, 36-38, 81, 97-99
C. Cohen-Tannoudji, B. Diu, F. Laloe, “Quantum Mechanics”, John Wiley & Sons, 1977, Ch. 6, General Properties of Angular Momentum in Quantum Mechanics”, pp. 641-772
A. Lasenby, C. Doran, “A Lecture Course in Geometric Algebra”, http://www.mrao.cam.ac.uk/~clifford/ptlllcourse/
http://en.wikipedia.org/wiki/Pauli_equation
T. Frankel, “The Geometry of Physics, An Introduction”, Cambridge University Press, 1997, Chapter 19, “The Dirac Equation”, pp.491-521
R.P. Feynman, “Quantum Electrodynamics”, W.A. Benjamin, Inc., New York, 1961
P.R. Wallace, “Mathematical Analysis of Physical Problems”, Dover Publications, 1972, 1984, ch. 5, Sec. 20 “Spin of Scalar Vector Field”, pp. 288 – 291
A.O. Barut, “Electrodynamics and Classical Theory of Fields and Particles”, Dover, 1964, 1980, pp.22-29, 36-38, 81, 97-99
C. Cohen-Tannoudji, B. Diu, F. Laloe, “Quantum Mechanics”, John Wiley & Sons, 1977, Ch. 6, General Properties of Angular Momentum in Quantum Mechanics”, pp. 641-772
A. Lasenby, C. Doran, “A Lecture Course in Geometric Algebra”, http://www.mrao.cam.ac.uk/~clifford/ptlllcourse/
http://en.wikipedia.org/wiki/Pauli_equation
T. Frankel, “The Geometry of Physics, An Introduction”, Cambridge University Press, 1997, Chapter 19, “The Dirac Equation”, pp.491-521
R.P. Feynman, “Quantum Electrodynamics”, W.A. Benjamin, Inc., New York, 1961
P.R. Wallace, “Mathematical Analysis of Physical Problems”, Dover Publications, 1972, 1984, ch. 5, Sec. 20 “Spin of Scalar Vector Field”, pp. 288 – 291
A.O. Barut, “Electrodynamics and Classical Theory of Fields and Particles”, Dover, 1964, 1980, pp.22-29, 36-38, 81, 97-99
C. Cohen-Tannoudji, B. Diu, F. Laloe, “Quantum Mechanics”, John Wiley & Sons, 1977, Ch. 6, General Properties of Angular Momentum in Quantum Mechanics”, pp. 641-772
A. Lasenby, C. Doran, “A Lecture Course in Geometric Algebra”, http://www.mrao.cam.ac.uk/~clifford/ptlllcourse/
http://en.wikipedia.org/wiki/Pauli_equation
T. Frankel, “The Geometry of Physics, An Introduction”, Cambridge University Press, 1997, Chapter 19, “The Dirac Equation”, pp.491-521
R.P. Feynman, “Quantum Electrodynamics”, W.A. Benjamin, Inc., New York, 1961
P.R. Wallace, “Mathematical Analysis of Physical Problems”, Dover Publications, 1972, 1984, ch. 5, Sec. 20 “Spin of Scalar Vector Field”, pp. 288 – 291
A.O. Barut, “Electrodynamics and Classical Theory of Fields and Particles”, Dover, 1964, 1980, pp.22-29, 36-38, 81, 97-99
C. Cohen-Tannoudji, B. Diu, F. Laloe, “Quantum Mechanics”, John Wiley & Sons, 1977, Ch. 6, General Properties of Angular Momentum in Quantum Mechanics”, pp. 641-772
A. Lasenby, C. Doran, “A Lecture Course in Geometric Algebra”, http://www.mrao.cam.ac.uk/~clifford/ptlllcourse/
R.H. Landau, “Quantum Mechanics II, A Second Course in Quantum Mechanics”, Jhon Wiley & Sons, 1996, pp. 243-244
http://en.wikipedia.org/wiki/Pauli_equation
T. Frankel, “The Geometry of Physics, An Introduction”, Cambridge University Press, 1997, Chapter 19, “The Dirac Equation”, pp.491-521
R.P. Feynman, “Quantum Electrodynamics”, W.A. Benjamin, Inc., New York, 1961
P.R. Wallace, “Mathematical Analysis of Physical Problems”, Dover Publications, 1972, 1984, ch. 5, Sec. 20 “Spin of Scalar Vector Field”, pp. 288 – 291
A.O. Barut, “Electrodynamics and Classical Theory of Fields and Particles”, Dover, 1964, 1980, pp.22-29, 36-38, 81, 97-99
C. Cohen-Tannoudji, B. Diu, F. Laloe, “Quantum Mechanics”, John Wiley & Sons, 1977, Ch. 6, General Properties of Angular Momentum in Quantum Mechanics”, pp. 641-772
A. Lasenby, C. Doran, “A Lecture Course in Geometric Algebra”, http://www.mrao.cam.ac.uk/~clifford/ptlllcourse/
R.H. Landau, “Quantum Mechanics II, A Second Course in Quantum Mechanics”, Jhon Wiley & Sons, 1996, pp. 243-244
http://en.wikipedia.org/wiki/Pauli_equation
T. Frankel, “The Geometry of Physics, An Introduction”, Cambridge University Press, 1997, Chapter 19, “The Dirac Equation”, pp.491-521
R.P. Feynman, “Quantum Electrodynamics”, W.A. Benjamin, Inc., New York, 1961
P.R. Wallace, “Mathematical Analysis of Physical Problems”, Dover Publications, 1972, 1984, ch. 5, Sec. 20 “Spin of Scalar Vector Field”, pp. 288 – 291
A.O. Barut, “Electrodynamics and Classical Theory of Fields and Particles”, Dover, 1964, 1980, pp.22-29, 36-38, 81, 97-99
C. Cohen-Tannoudji, B. Diu, F. Laloe, “Quantum Mechanics”, John Wiley & Sons, 1977, Ch. 6, General Properties of Angular Momentum in Quantum Mechanics”, pp. 641-772
A. Lasenby, C. Doran, “A Lecture Course in Geometric Algebra”, http://www.mrao.cam.ac.uk/~clifford/ptlllcourse/
R.H. Landau, “Quantum Mechanics II, A Second Course in Quantum Mechanics”, Jhon Wiley & Sons, 1996, pp. 243-244
http://en.wikipedia.org/wiki/Pauli_equation
T. Frankel, “The Geometry of Physics, An Introduction”, Cambridge University Press, 1997, Chapter 19, “The Dirac Equation”, pp.491-521
R.P. Feynman, “Quantum Electrodynamics”, W.A. Benjamin, Inc., New York, 1961
P.R. Wallace, “Mathematical Analysis of Physical Problems”, Dover Publications, 1972, 1984, ch. 5, Sec. 20 “Spin of Scalar Vector Field”, pp. 288 – 291
A.O. Barut, “Electrodynamics and Classical Theory of Fields and Particles”, Dover, 1964, 1980, pp.22-29, 36-38, 81, 97-99
C. Cohen-Tannoudji, B. Diu, F. Laloe, “Quantum Mechanics”, John Wiley & Sons, 1977, Ch. 6, General Properties of Angular Momentum in Quantum Mechanics”, pp. 641-772
A. Lasenby, C. Doran, “A Lecture Course in Geometric Algebra”, http://www.mrao.cam.ac.uk/~clifford/ptlllcourse/
http://en.wikipedia.org/wiki/Paul_Dirac
http://en.wikipedia.org/wiki/Dirac_equation
T. Frankel, “The Geometry of Physics, An Introduction”, Cambridge University Press, 1997, Chapter 19, “The Dirac Equation”, pp.491-521
R.P. Feynman, “Quantum Electrodynamics”, W.A. Benjamin, Inc., New York, 1961
P.R. Wallace, “Mathematical Analysis of Physical Problems”, Dover Publications, 1972, 1984, ch. 5, Sec. 20 “Spin of Scalar Vector Field”, pp. 288 – 291
A.O. Barut, “Electrodynamics and Classical Theory of Fields and Particles”, Dover, 1964, 1980, pp.22-29, 36-38, 81, 97-99
C. Cohen-Tannoudji, B. Diu, F. Laloe, “Quantum Mechanics”, John Wiley & Sons, 1977, Ch. 6, General Properties of Angular Momentum in Quantum Mechanics”, pp. 641-772
A. Lasenby, C. Doran, “A Lecture Course in Geometric Algebra”, http://www.mrao.cam.ac.uk/~clifford/ptlllcourse/
http://en.wikipedia.org/wiki/Paul_Dirac
http://en.wikipedia.org/wiki/Dirac_equation
T. Frankel, “The Geometry of Physics, An Introduction”, Cambridge University Press, 1997, Chapter 19, “The Dirac Equation”, pp.491-521
R.P. Feynman, “Quantum Electrodynamics”, W.A. Benjamin, Inc., New York, 1961
P.R. Wallace, “Mathematical Analysis of Physical Problems”, Dover Publications, 1972, 1984, ch. 5, Sec. 20 “Spin of Scalar Vector Field”, pp. 288 – 291
A.O. Barut, “Electrodynamics and Classical Theory of Fields and Particles”, Dover, 1964, 1980, pp.22-29, 36-38, 81, 97-99
C. Cohen-Tannoudji, B. Diu, F. Laloe, “Quantum Mechanics”, John Wiley & Sons, 1977, Ch. 6, General Properties of Angular Momentum in Quantum Mechanics”, pp. 641-772
A. Lasenby, C. Doran, “A Lecture Course in Geometric Algebra”, http://www.mrao.cam.ac.uk/~clifford/ptlllcourse/
http://en.wikipedia.org/wiki/Paul_Dirac
http://en.wikipedia.org/wiki/Dirac_equation
T. Frankel, “The Geometry of Physics, An Introduction”, Cambridge University Press, 1997, Chapter 19, “The Dirac Equation”, pp.491-521
R.P. Feynman, “Quantum Electrodynamics”, W.A. Benjamin, Inc., New York, 1961
P.R. Wallace, “Mathematical Analysis of Physical Problems”, Dover Publications, 1972, 1984, ch. 5, Sec. 20 “Spin of Scalar Vector Field”, pp. 288 – 291
A.O. Barut, “Electrodynamics and Classical Theory of Fields and Particles”, Dover, 1964, 1980, pp.22-29, 36-38, 81, 97-99
C. Cohen-Tannoudji, B. Diu, F. Laloe, “Quantum Mechanics”, John Wiley & Sons, 1977, Ch. 6, General Properties of Angular Momentum in Quantum Mechanics”, pp. 641-772
A. Lasenby, C. Doran, “A Lecture Course in Geometric Algebra”, http://www.mrao.cam.ac.uk/~clifford/ptlllcourse/
http://en.wikipedia.org/wiki/Paul_Dirac
http://en.wikipedia.org/wiki/Dirac_equation
T. Frankel, “The Geometry of Physics, An Introduction”, Cambridge University Press, 1997, Chapter 19, “The Dirac Equation”, pp.491-521
R.P. Feynman, “Quantum Electrodynamics”, W.A. Benjamin, Inc., New York, 1961
P.R. Wallace, “Mathematical Analysis of Physical Problems”, Dover Publications, 1972, 1984, ch. 5, Sec. 20 “Spin of Scalar Vector Field”, pp. 288 – 291
A.O. Barut, “Electrodynamics and Classical Theory of Fields and Particles”, Dover, 1964, 1980, pp.22-29, 36-38, 81, 97-99
C. Cohen-Tannoudji, B. Diu, F. Laloe, “Quantum Mechanics”, John Wiley & Sons, 1977, Ch. 6, General Properties of Angular Momentum in Quantum Mechanics”, pp. 641-772
A. Lasenby, C. Doran, “A Lecture Course in Geometric Algebra”, http://www.mrao.cam.ac.uk/~clifford/ptlllcourse/
http://en.wikipedia.org/wiki/Paul_Dirac
http://en.wikipedia.org/wiki/Dirac_equation
T. Frankel, “The Geometry of Physics, An Introduction”, Cambridge University Press, 1997, Chapter 19, “The Dirac Equation”, pp.491-521
R.P. Feynman, “Quantum Electrodynamics”, W.A. Benjamin, Inc., New York, 1961
P.R. Wallace, “Mathematical Analysis of Physical Problems”, Dover Publications, 1972, 1984, ch. 5, Sec. 20 “Spin of Scalar Vector Field”, pp. 288 – 291
A.O. Barut, “Electrodynamics and Classical Theory of Fields and Particles”, Dover, 1964, 1980, pp.22-29, 36-38, 81, 97-99
C. Cohen-Tannoudji, B. Diu, F. Laloe, “Quantum Mechanics”, John Wiley & Sons, 1977, Ch. 6, General Properties of Angular Momentum in Quantum Mechanics”, pp. 641-772
A. Lasenby, C. Doran, “A Lecture Course in Geometric Algebra”, http://www.mrao.cam.ac.uk/~clifford/ptlllcourse/
R.P. Feynman, R.B. Leighton, M. Sands, “Feinmam Lectures on Physics”, Vol III, Addison-Wesley, 1965, § 11-4
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
R.P. Feynman, R.B. Leighton, M. Sands, “Feinmam Lectures on Physics”, Vol III, Addison-Wesley, 1965, § 11-4
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
R.P. Feynman, R.B. Leighton, M. Sands, “Feinmam Lectures on Physics”, Vol III, Addison-Wesley, 1965, § 11-4
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
R.P. Feynman, R.B. Leighton, M. Sands, “Feinmam Lectures on Physics”, Vol III, Addison-Wesley, 1965, § 11-4
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
J. Baggott, “The Meaning of Quantum Theory”, Oxford Science Presentations, 1992, pp. 64-67
J. Baggott, “The Meaning of Quantum Theory”, Oxford Science Presentations, 1992, pp. 64-65
R.P. Feynman, R.B. Leighton, M. Sands, “Feinmam Lectures on Physics”, Vol III, Addison-Wesley, 1965, § 11-4
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
Nick Herbert, “Quantum Reality – Beyond the New Physics”, Anchor Press /Doubleday, 1985
R.P. Feynman, R.B. Leighton, M. Sands, “Feinmam Lectures on Physics”, Vol III, Addison-Wesley, 1965, § 11-4
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
Nick Herbert, “Quantum Reality – Beyond the New Physics”, Anchor Press /Doubleday, 1985
R.P. Feynman, R.B. Leighton, M. Sands, “Feinmam Lectures on Physics”, Vol III, Addison-Wesley, 1965, § 11-4
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
Nick Herbert, “Quantum Reality – Beyond the New Physics”, Anchor Press /Doubleday, 1985
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992. pp. 73-74
R.P. Feynman, R.B. Leighton, M. Sands, “Feinmam Lectures on Physics”, Vol III, Addison-Wesley, 1965, § 11-4
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
http://en.wikipedia.org/wiki/Measurement_in_quantum_mechanics#Wavefunction_collapse
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
http://www.csicop.org/si/show/quantum_quackery/
http://en.wikipedia.org/wiki/Measurement_in_quantum_mechanics#Wavefunction_collapse
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992, pg. 105
John Gribbin, “Schrödinger’s Kittens and the Search for Reality”
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992, pp. 84-86
V.J. Stenger, “The Unconscious Quantum – Metaphysics in Modern Physics and Cosmology”, Prometheus Books, 1995, pp.58-60
http://timeline.web.cern.ch/timelines/From-the-archive
http://timeline.web.cern.ch/the-como-congress-1927
http://en.wikipedia.org/wiki/Bohr%E2%80%93Einstein_debates
Niels Bohr, &quot;Discussions with Einstein on Epistemological Problems in Atomic Physics&quot; in, P. A. Schilpp, ed., Albert Einstein-Philosopher Scientist. 2nd ed. New York: Tudor Publishing, 1951.
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
http://en.wikipedia.org/wiki/Bohr%E2%80%93Einstein_debates
Niels Bohr, &quot;Discussions with Einstein on Epistemological Problems in Atomic Physics&quot; in, P. A. Schilpp, ed., Albert Einstein-Philosopher Scientist. 2nd ed. New York: Tudor Publishing, 1951.
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
http://en.wikipedia.org/wiki/Bohr%E2%80%93Einstein_debates
Niels Bohr, &quot;Discussions with Einstein on Epistemological Problems in Atomic Physics&quot; in, P. A. Schilpp, ed., Albert Einstein-Philosopher Scientist. 2nd ed. New York: Tudor Publishing, 1951.
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
http://en.wikipedia.org/wiki/Bohr%E2%80%93Einstein_debates
Niels Bohr, &quot;Discussions with Einstein on Epistemological Problems in Atomic Physics&quot; in, P. A. Schilpp, ed., Albert Einstein-Philosopher Scientist. 2nd ed. New York: Tudor Publishing, 1951.
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
http://en.wikipedia.org/wiki/Bohr%E2%80%93Einstein_debates
Niels Bohr, &quot;Discussions with Einstein on Epistemological Problems in Atomic Physics&quot; in, P. A. Schilpp, ed., Albert Einstein-Philosopher Scientist. 2nd ed. New York: Tudor Publishing, 1951.
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
http://en.wikipedia.org/wiki/Bohr%E2%80%93Einstein_debates
Niels Bohr, &quot;Discussions with Einstein on Epistemological Problems in Atomic Physics&quot; in, P. A. Schilpp, ed., Albert Einstein-Philosopher Scientist. 2nd ed. New York: Tudor Publishing, 1951.
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
http://en.wikipedia.org/wiki/Bohr%E2%80%93Einstein_debates
Niels Bohr, &quot;Discussions with Einstein on Epistemological Problems in Atomic Physics&quot; in, P. A. Schilpp, ed., Albert Einstein-Philosopher Scientist. 2nd ed. New York: Tudor Publishing, 1951.
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
http://en.wikipedia.org/wiki/Bohr%E2%80%93Einstein_debates
Niels Bohr, &quot;Discussions with Einstein on Epistemological Problems in Atomic Physics&quot; in, P. A. Schilpp, ed., Albert Einstein-Philosopher Scientist. 2nd ed. New York: Tudor Publishing, 1951.
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
V.J. Stenger, “The Unconscious Quantum – Metaphysics in Modern Physics and Cosmology”, Prometheus Books, 1995, pp.66-99
http://en.wikipedia.org/wiki/Bohr%E2%80%93Einstein_debates
Niels Bohr, &quot;Discussions with Einstein on Epistemological Problems in Atomic Physics&quot; in, P. A. Schilpp, ed., Albert Einstein-Philosopher Scientist. 2nd ed. New York: Tudor Publishing, 1951.
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
http://en.wikipedia.org/wiki/Path_integral_formulation
http://en.wikipedia.org/wiki/Relation_between_Schr%C3%B6dinger%27s_equation_and_the_path_integral_formulation_of_quantum_mechanics
R. P. Feynman, A.R. Hibbs, “Quantum Mechanics and Path Integration”, McGraw-Hill, 1965
H. Kleinert, “Path Integrals in Quantum Mechanics Statistics and Polymer Physics”, World Scientific, 1999
http://en.wikipedia.org/wiki/Path_integral_formulation
http://en.wikipedia.org/wiki/Relation_between_Schr%C3%B6dinger%27s_equation_and_the_path_integral_formulation_of_quantum_mechanics
R. P. Feynman, A.R. Hibbs, “Quantum Mechanics and Path Integration”, McGraw-Hill, 1965
H. Kleinert, “Path Integrals in Quantum Mechanics Statistics and Polymer Physics”, World Scientific, 1999
http://en.wikipedia.org/wiki/Path_integral_formulation
http://en.wikipedia.org/wiki/Relation_between_Schr%C3%B6dinger%27s_equation_and_the_path_integral_formulation_of_quantum_mechanics
R. P. Feynman, A.R. Hibbs, “Quantum Mechanics and Path Integration”, McGraw-Hill, 1965
A. Zee, “Quantum Field Theory in a Nutshell”, Princeton University Press, 2003, pp. 10-13
H. Kleinert, “Path Integrals in Quantum Mechanics Statistics and Polymer Physics”, World Scientific, 1999, Ch.2
http://en.wikipedia.org/wiki/Path_integral_formulation
http://en.wikipedia.org/wiki/Relation_between_Schr%C3%B6dinger%27s_equation_and_the_path_integral_formulation_of_quantum_mechanics
R. P. Feynman, A.R. Hibbs, “Quantum Mechanics and Path Integration”, McGraw-Hill, 1965
A. Zee, “Quantum Field Theory in a Nutshell”, Princeton University Press, 2003, pp. 10-13
H. Kleinert, “Path Integrals in Quantum Mechanics Statistics and Polymer Physics”, World Scientific, 1999, Ch.2
http://en.wikipedia.org/wiki/Path_integral_formulation
http://en.wikipedia.org/wiki/Relation_between_Schr%C3%B6dinger%27s_equation_and_the_path_integral_formulation_of_quantum_mechanics
R. P. Feynman, A.R. Hibbs, “Quantum Mechanics and Path Integration”, McGraw-Hill, 1965
A. Zee, “Quantum Field Theory in a Nutshell”, Princeton University Press, 2003, pp. 10-13
H. Kleinert, “Path Integrals in Quantum Mechanics Statistics and Polymer Physics”, World Scientific, 1999, Ch. 2
http://physics.stackexchange.com/questions/68940/virtual-photons-what-makes-them-virtualR. P. Feynman, A.R. Hibbs, “Quantum Mechanics and Path Integration”, McGraw-Hill, 1965
A. Zee, “Quantum Field Theory in a Nutshell”, Princeton University Press, 2003, pp. 10-13
H. Kleinert, “Path Integrals in Quantum Mechanics Statistics and Polymer Physics”, World Scientific, 1999, Ch. 2
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
http://en.wikipedia.org/wiki/Hidden_variable_theory
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992
http://en.wikipedia.org/wiki/Hidden_variable_theory
http://en.wikipedia.org/wiki/De_Broglie%E2%80%93Bohm_theory
V.J. Stenger, “The Unconscious Quantum – Metaphysics in Modern Physics and Cosmology”, Prometheus Books, 1995, pp.105-106
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992, pg.113
http://en.wikipedia.org/wiki/De_Broglie%E2%80%93Bohm_theory
V.J. Stenger, “The Unconscious Quantum – Metaphysics in Modern Physics and Cosmology”, Prometheus Books, 1995, pp.105-106
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press,1992, pg.113
http://en.wikipedia.org/wiki/Bell_inequality
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press, 1992, Ch. 4, “Putting it to the test”, pp. 117-158
http://en.wikipedia.org/wiki/Bell_inequality
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press, 1992, Ch. 4, “Putting it to the test”, pp. 117-158
http://en.wikipedia.org/wiki/Bell_inequality
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press, 1992, Ch. 4, “Putting it to the test”, pp. 117-158
http://en.wikipedia.org/wiki/Bell_inequality
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press, 1992, Ch. 4, “Putting it to the test”, pp. 117-158
http://en.wikipedia.org/wiki/Bell_inequality
http://en.wikipedia.org/wiki/CHSH_inequality
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press, 1992, Ch. 4, “Putting it to the test”, pp. 117-158
http://www.uwo.ca/sci/featured_faculty/r_holt.html
http://www.stonehill.edu/directory/michael-horne/
http://en.wikipedia.org/wiki/CHSH_inequality
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press, 1992, Ch. 4, “Putting it to the test”, pp. 117-158
http://www.uwo.ca/sci/featured_faculty/r_holt.html
http://www.stonehill.edu/directory/michael-horne/
http://en.wikipedia.org/wiki/CHSH_inequality
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press, 1992, Ch. 4, “Putting it to the test”, pp. 117-158
http://www.uwo.ca/sci/featured_faculty/r_holt.html
http://www.stonehill.edu/directory/michael-horne/
http://en.wikipedia.org/wiki/CHSH_inequality
J. Baggott, “The Meaning of Quantum Theory”, Oxford University Press, 1992, Ch. 4, “Putting it to the test”, pp. 117-158
http://www.uwo.ca/sci/featured_faculty/r_holt.html
http://www.stonehill.edu/directory/michael-horne/
V.J. Stenger, “The Unconscious Quantum – Metaphysics in Modern Physics and Cosmology”, Prometheus Books, 1995
http://en.wikipedia.org/wiki/Alain_Aspect
http://en.wikipedia.org/wiki/Bell_test_experiments
http://commons.wikimedia.org/wiki/File:Alain_Aspect_experiment_1981_diagram.svg
http://freespace.virgin.net/ch.thompson1/Against/vigier.htm
http://en.wikipedia.org/wiki/Schrödinger equation - Wikipedia, the free encyclopedia.mht
http://en.wikipedia.org/wiki/Valentine_Telegdi
http://public.ihes.fr/LouisMichel/FILES/PHOTO_LMsite.pdf
http://en.wikipedia.org/wiki/Valentine_Bargmann
http://www.nasonline.org/publications/biographical-memoirs/memoir-pdfs/bargmann-valentine.pdf
A.O.Barut, “Electrodynamics and Classical Theory of Fields and Particles”, Dover, 1964, 1980, pp. 75-76
J.D.Jackson, “Classical Electrodynamics”, John Wiley & Sons, Ed. 3, 1999, pg. 563, Eq. (11.164)