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KAMALA NEHRU INSTITUTE OF PHYSICAL & SOCIAL SCIENCE SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

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Page 1: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

KAMALA NEHRU INSTITUTE OF PHYSICAL

& SOCIAL SCIENCE

SESSION: 2011-12

Black hole

SUBMITTED BY: SUBMITTED TO:

Dr.A.K.SRIVASTAVA

UNDER SUPERVISION OF:SHRI SUSHEEL SINGH

M.Sc FINAL

Amaresh Singh

Page 2: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

Some Definitions of BLACK HOLES

black hole is just another thing a star can turns in to when it runs out of fuel.or it is x star

Black holes are the cold remnants of former star ,so dense that no matter not even light is able to escape their powerful gravitational pull.

Page 3: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

KINDS OF BLACK HOLES

Stellar black holes. Super massive black hole An Intermediate mass black hole Mini black hole Worm holes

Page 4: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

Stellar Mass – must be at least 3 solar masses (~1034 g)Intermediate Mass – a few thousand to a few tens of thousands of solar masses; possibly the agglomeration of stellar mass holesSuper massive – millions to billions of solar masses; located in the centers of galaxies

Page 5: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

Some technical terms

Schwarz schild radius. SingularityEvent horizon, Escape velocity.

Page 6: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

Schwarzschild Radius and Event Horizon

Page 7: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh
Page 8: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

Escape Velocity

Imagine feebly tossing a rocketship up in the air. It falls back to Earth because its kinetic energy was less than its gravitational potential energy.

However, toss it with a larger and larger velocity and it will go higher and higher before falling back to Earth.

There is a velocity above which it will not return to Earth -- this is the escape velocity.

Page 9: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

Escape Velocity

To determine the escape velocity from Earth you set the gravitational potential energy equal to kinetic energy and solve for velocity

Vescape 2 GM

R

Radius from which you want to escape

Mass of theobject from which you want to escape

Page 10: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

Note that the escape velocity doesn’t depend on the mass of the escaping body.For the Earth, put in the mass and radius of the Earth (for escape from the surface of the Earth) and you get: Vesc= 11 km/sec = 25,000 miles/hr

Page 11: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

Now suppose you shrink the Earth to 1/100 of its current radius (at constant mass). What

happens to Vesc?

As R goes up, Vesc goes down

As R goes down, Vesc goes up

Don’t forget the square root

For this case, Vesc increases by 10x

Vesc 2GM

R

Vesc 1

R

Page 12: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

Reduce the radius of the Earth to 1cm and Vesc=c (speed of light)

In this new theory of Gravity, where photons are affected by gravity, if the escape velocity equals or exceeds the speed of light, that object can no longer be observed. This is a Black Hole

Page 13: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

Properties & Structures

Three parameters completely describe the structure of a black

hole

MassAs measured by the black hole’s effect on orbiting bodies, such as another starTotal electric chargeAs measured by the strength of the electric forceSpin = angular momentumHow fast the black hole is spinning

Page 14: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

Formation of black hole $ growth of black hole

Page 15: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

Detection of BLACK HOLE

Page 16: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

What would be happens when we get close to a black hole?

Time would slow (as seen by outside observers.) Falling person notices nothing, even crossing event horizon.

Light from falling person (to outside observers) becomes more and more redshifted. The person falling slowly disappears from view (to outside observers.

Gravitational “tidal forces” would stretch matter out into longer and longer, thinner and thinner strands.

Eventually all things that characterize matter would be gone. atoms molecules, protons, neutrons, electrons…

Everything is compressed into an infinitely small point of infinite density (the singularity).

All that remains is mass (energy) and angular momentum…

Page 17: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh
Page 18: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

An astronaut descending down towards the event horizon of the

black hole will be stretched vertically (tidal effects) and

squeezed laterally unless the black hole is very large like thousands

of solar masses, so the multi-million solar mass black hole in the center of the galaxy is safe.

Page 19: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

The only known places in the Universe where there could be enough mass in one area is in the center of massive galaxiesNot believed to be anywhere else

Where Could Super-Massive Black Holes Exist?

Page 20: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

Which is the closest black hole to the earth?

Page 21: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

Which is The biggest black hole?

Page 22: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

WHAT HAPPENS IF A BLACK HOLE HIT THE EARTH

Page 23: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

EVIDENCE OF BLACK HOLE

Page 24: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

MYTHS & FACTS OF BLACK HOLES

Black holes are completely black.

Page 25: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

Matter which falls into a black holes reappears somewhere else in universe.

Page 28: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

A black hole in space would devour everything in our galaxy.

Page 30: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

AcknowledgementI am grateful to all respected teachers & specially shri Susheel singh & Satyendra pandey sir for his pleasant cooperation in collection & collation of information & material required for the preparation of this innovative representation.Last but not least I would like to thanks my parents & my friends specially those who work together as in terns at KNIPSS for the wise ideas throughout the project.

Page 31: SESSION: 2011-12 Black hole SUBMITTED BY: SUBMITTED TO: Dr.A.K.SRIVASTAVA UNDER SUPERVISION OF: SHRI SUSHEEL SINGH M.Sc FINAL Amaresh Singh

thanks