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MAHAVIR SWAMI COLLEGE OF
ENGINEERING AND TECHNOLOGY
IMAGES OF BLACK HOLES
•A black hole is a region of        •   Around a black hole there is a
spacetime from which gravity            mathematically defined
                                        surface called an
prevents anything, including light,     event horizon that marks the
from escaping.                          point of no return.

                                     • It is called "black" because it
                                       absorbs all the light that hits
                                       the horizon, reflecting
                                       nothing, just like a perfect
                                       blackbody in
                                       thermodynamics.
•This temperature is inversely
proportional to the mass of the      • Quantum field theory in curved spa
black hole, making it difficult to     predicts that event horizons
observe this radiation for             emit radiation like a black
black holes of stellar mass or         body with a finite temperature.
greater.
PROJECT GOAL
TO KNOW ABOUT:-

THE TERM “BLACK HOLE”.

CONTRIBUTOR’S IN THE FIELD OF BLACK HOLE.

DISCOVERY & RESEARCH ABOUT BLACK HOLE.
INTRODUCTION TO CONTRIBUTOR’S

•   SOME GREAT CONTRIBUTORS IN THE FIELD OF BLACK HOLE
    ARE AS FOLLOWS :-

•   JOHN MICHELL
•   ALBERT EINSTEIN
•   STEPHEN HAWKING
•   HENDRIC LORENTZ
•   DAVID HILBERT
•   JULES HENRI POINCARE
•   KARL SCHWARZSCHILD

•   & MANY OTHERS.
SELECTED CONTRIBUTOR’S IN THE FIELD
          OF BLACK HOLE

     • 1.GEOLOGIST JOHN MICHELL
        (25 December 1724 – 29 April 1793)


    • 2.PHYSICIST ALBERT EINSTEIN
         (14 March 1879 – 18 April 1955)


  • 3.COSMOLOGIST STEPHEN HAWKING
               (born 8 January 1942)
1.Geologist john michell
John Michell was an
English natural
philosopher and
geologist whose work
spanned a wide range
of subjects from
astronomy to geology,
optics, and gravitation.
                           Born : December 25, 1724
He was both a              Died : April 29, 1793
theorist and an            Education : University of
                              Cambridge, Queens'
experimenter.
                             College, Cambridge
JOHN MICHELL CONTRIBUTION
• The idea of a body so massive that even light
  could not escape was first put forward by
  geologist John Michell in a letter written to
  Henry Cavendish in 1783 of the Royal Society:

• If the semi-diameter of a sphere of the same
  density as the Sun were to exceed that of the Sun
  in the proportion of 500 to 1, a body falling from
  an infinite height towards it would have acquired
  at its surface greater velocity than that of light,
  and consequently supposing light to be attracted
  by the same force in proportion to its vis inertiae,
  with other bodies, all light emitted from such a
  body would be made to return towards it by its
  own proper gravity.
  —John Michell
CONT…
• In 1796, mathematician
  Pierre-Simon Laplace
   promoted the same idea in
  the first and second editions
  of his book Exposition du
  système du Monde (it was
  removed from later
  editions).

• Such "dark stars” were
  largely ignored in the
  nineteenth century, since it
  was not understood how a
  massless wave such as light
  could be influenced by
  gravity.
2. PHYSICIST ALBERT EINSTEIN
Albert Einstein was a German-born theoretical physicist who developed
the general theory of relativity, one of the two pillars of modern physics.
 Born : March 14, 1879, Ulm

 Died : April 18, 1955, Princeton

 Children : Hans Albert Einstein, Eduard
      Einstein, Lieserl Einstein,Margot
      Einstein, Ilse Einstein

 Education : University of Zurich (1905), ETH
     Zurich (1901), Aargau Cantonal School
     (1895 – 1896), Luitpold Gymnasium

 Spouse : Elsa Einstein (m. 1919–
     1936), Mileva Marić (m. 1903–1919)

 Awards : Nobel Prize in Physics, Copley
     Medal, Franklin Medal
ALBERT EINSTEIN CONTRIBUTION

•Albert Einstein’s general theory of relativity helped much in
believing the existence of black holes.

•Now experts say they have shown that the theoretical
phenomenon, whose gravitational pull is thought to hold galaxies
together, exist "beyond any reasonable doubt".

•The team of scientists spent 16 years studying the existence of
a super massive black hole thought to be at the centre of our
galaxy, the Milky Way.

•While the black hole itself is invisible to the eye, the team proved
its existence by tracking the motions of 28 stars circling around it.
CONT...
•“The stellar orbits in the galactic centre show that the
central mass concentration of four million solar masses
must be a black hole, beyond any reasonable doubt”.

•The astronomers were also able to measure with great
accuracy how far the Earth is from the centre of the galaxy
- a distance of 27,000 light years.

•While the idea of a black hole dates back as far as 1783, it
was only after Einstein published his general relativity
theory in 1916 that the modern concept was introduced by
the German physicist Karl Scharzchild. The actual phrase
black hole was not, however, coined until 1968.
3.COSMOLOGIST STEPHAN HAWKING
•Stephen William Hawking, CH,
CBE, FRS, FRSA is a British
theoretical physicist, cosmologist
and author.
•Born : January 8, 1942 (age 71), Oxford
•Spouse : Elaine Hawking (m. 1995–
2006), Jane Hawking (m. 1965–1991)
•Children : Lucy Hawking, Timothy
Hawking, Robert Hawking
•Movies and TV shows : Stephen
Hawking's Universe, More
•Awards : Presidential Medal of
Freedom, Copley Medal, More
STEPHAN HAWKING’S CONTRIBUTION
In 1974, Hawking showed that black holes are not entirely
black but emit small amounts of thermal radiation;an effect
that has become known as Hawking radiation.
By applying quantum field theory to a static black hole
background, he determined that a black hole should emit
particles in a perfect black body spectrum.
If Hawking's theory of black hole radiation is correct, then
black holes are expected to shrink and evaporate over time
because they lose mass by the emission of photons and
other particles.
The temperature of this thermal spectrum (Hawking
temperature) is proportional to the surface gravity of the black
hole, which, for a Schwarzschild black hole, is inversely
proportional to the mass.
CONT...
•A stellar black hole of one solar mass has a Hawking
temperature of about 100 nanokelvins.
•This is far less than the 2.7 K temperature of the cosmic
microwave background radiation.
•To have a Hawking temperature larger than 2.7 K (and be
able to evaporate), a black hole needs to have less mass
than the Moon.
•Such a black hole would have a diameter of less than a
tenth of a millimeter.
•If a black hole is very small the radiation effects are
expected to become very strong. Even a black hole that is
heavy compared to a human would evaporate in an instant.

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Black hole

  • 1. MAHAVIR SWAMI COLLEGE OF ENGINEERING AND TECHNOLOGY
  • 2.
  • 4. •A black hole is a region of • Around a black hole there is a spacetime from which gravity mathematically defined surface called an prevents anything, including light, event horizon that marks the from escaping. point of no return. • It is called "black" because it absorbs all the light that hits the horizon, reflecting nothing, just like a perfect blackbody in thermodynamics. •This temperature is inversely proportional to the mass of the • Quantum field theory in curved spa black hole, making it difficult to predicts that event horizons observe this radiation for emit radiation like a black black holes of stellar mass or body with a finite temperature. greater.
  • 5. PROJECT GOAL TO KNOW ABOUT:- THE TERM “BLACK HOLE”. CONTRIBUTOR’S IN THE FIELD OF BLACK HOLE. DISCOVERY & RESEARCH ABOUT BLACK HOLE.
  • 6. INTRODUCTION TO CONTRIBUTOR’S • SOME GREAT CONTRIBUTORS IN THE FIELD OF BLACK HOLE ARE AS FOLLOWS :- • JOHN MICHELL • ALBERT EINSTEIN • STEPHEN HAWKING • HENDRIC LORENTZ • DAVID HILBERT • JULES HENRI POINCARE • KARL SCHWARZSCHILD • & MANY OTHERS.
  • 7. SELECTED CONTRIBUTOR’S IN THE FIELD OF BLACK HOLE • 1.GEOLOGIST JOHN MICHELL (25 December 1724 – 29 April 1793) • 2.PHYSICIST ALBERT EINSTEIN (14 March 1879 – 18 April 1955) • 3.COSMOLOGIST STEPHEN HAWKING (born 8 January 1942)
  • 8. 1.Geologist john michell John Michell was an English natural philosopher and geologist whose work spanned a wide range of subjects from astronomy to geology, optics, and gravitation. Born : December 25, 1724 He was both a Died : April 29, 1793 theorist and an Education : University of Cambridge, Queens' experimenter. College, Cambridge
  • 9. JOHN MICHELL CONTRIBUTION • The idea of a body so massive that even light could not escape was first put forward by geologist John Michell in a letter written to Henry Cavendish in 1783 of the Royal Society: • If the semi-diameter of a sphere of the same density as the Sun were to exceed that of the Sun in the proportion of 500 to 1, a body falling from an infinite height towards it would have acquired at its surface greater velocity than that of light, and consequently supposing light to be attracted by the same force in proportion to its vis inertiae, with other bodies, all light emitted from such a body would be made to return towards it by its own proper gravity. —John Michell
  • 10. CONT… • In 1796, mathematician Pierre-Simon Laplace promoted the same idea in the first and second editions of his book Exposition du système du Monde (it was removed from later editions). • Such "dark stars” were largely ignored in the nineteenth century, since it was not understood how a massless wave such as light could be influenced by gravity.
  • 11. 2. PHYSICIST ALBERT EINSTEIN Albert Einstein was a German-born theoretical physicist who developed the general theory of relativity, one of the two pillars of modern physics. Born : March 14, 1879, Ulm Died : April 18, 1955, Princeton Children : Hans Albert Einstein, Eduard Einstein, Lieserl Einstein,Margot Einstein, Ilse Einstein Education : University of Zurich (1905), ETH Zurich (1901), Aargau Cantonal School (1895 – 1896), Luitpold Gymnasium Spouse : Elsa Einstein (m. 1919– 1936), Mileva Marić (m. 1903–1919) Awards : Nobel Prize in Physics, Copley Medal, Franklin Medal
  • 12. ALBERT EINSTEIN CONTRIBUTION •Albert Einstein’s general theory of relativity helped much in believing the existence of black holes. •Now experts say they have shown that the theoretical phenomenon, whose gravitational pull is thought to hold galaxies together, exist "beyond any reasonable doubt". •The team of scientists spent 16 years studying the existence of a super massive black hole thought to be at the centre of our galaxy, the Milky Way. •While the black hole itself is invisible to the eye, the team proved its existence by tracking the motions of 28 stars circling around it.
  • 13. CONT... •“The stellar orbits in the galactic centre show that the central mass concentration of four million solar masses must be a black hole, beyond any reasonable doubt”. •The astronomers were also able to measure with great accuracy how far the Earth is from the centre of the galaxy - a distance of 27,000 light years. •While the idea of a black hole dates back as far as 1783, it was only after Einstein published his general relativity theory in 1916 that the modern concept was introduced by the German physicist Karl Scharzchild. The actual phrase black hole was not, however, coined until 1968.
  • 14. 3.COSMOLOGIST STEPHAN HAWKING •Stephen William Hawking, CH, CBE, FRS, FRSA is a British theoretical physicist, cosmologist and author. •Born : January 8, 1942 (age 71), Oxford •Spouse : Elaine Hawking (m. 1995– 2006), Jane Hawking (m. 1965–1991) •Children : Lucy Hawking, Timothy Hawking, Robert Hawking •Movies and TV shows : Stephen Hawking's Universe, More •Awards : Presidential Medal of Freedom, Copley Medal, More
  • 15. STEPHAN HAWKING’S CONTRIBUTION In 1974, Hawking showed that black holes are not entirely black but emit small amounts of thermal radiation;an effect that has become known as Hawking radiation. By applying quantum field theory to a static black hole background, he determined that a black hole should emit particles in a perfect black body spectrum. If Hawking's theory of black hole radiation is correct, then black holes are expected to shrink and evaporate over time because they lose mass by the emission of photons and other particles. The temperature of this thermal spectrum (Hawking temperature) is proportional to the surface gravity of the black hole, which, for a Schwarzschild black hole, is inversely proportional to the mass.
  • 16. CONT... •A stellar black hole of one solar mass has a Hawking temperature of about 100 nanokelvins. •This is far less than the 2.7 K temperature of the cosmic microwave background radiation. •To have a Hawking temperature larger than 2.7 K (and be able to evaporate), a black hole needs to have less mass than the Moon. •Such a black hole would have a diameter of less than a tenth of a millimeter. •If a black hole is very small the radiation effects are expected to become very strong. Even a black hole that is heavy compared to a human would evaporate in an instant.