Subhadra Sundar Chakraborty (CSE/2015/043)
S. Tushar (CSE/2015/042)
Amar Kr. Gupta (CSE/2015/053)
Akhil Mishra (CSE/2015/060)
Akshay Mishra (CSE/2015/052)
The Supernova andThe Supernova and
Black HolesBlack Holes
HU481
Technical Report Writing & Language Laboratory
Black Holes: A TheoreticalBlack Holes: A Theoretical
DefinitionDefinition
 An area of space-timeAn area of space-time
with a gravitationalwith a gravitational
field so intense thatfield so intense that
it’s escape velocity isit’s escape velocity is
equal to or exceedsequal to or exceeds
the speed of light.the speed of light.
 The important thing isThe important thing is
that this area can be ofthat this area can be of
any size.any size.
The Finite Speed of LightThe Finite Speed of Light
 The base of physicalThe base of physical
theories assumes thattheories assumes that
speed of light inspeed of light in
vacuum is finite andvacuum is finite and
maximum possible.maximum possible.
(A black-hole-powered jet of(A black-hole-powered jet of
subatomic particles traveling atsubatomic particles traveling at
nearly the speed of light out of thenearly the speed of light out of the
M87 galaxy)M87 galaxy)
Escape Velocity, Density, andEscape Velocity, Density, and
Schwarzschild RadiusSchwarzschild Radius
 Every entity has anEvery entity has an
escape velocity asescape velocity as
 VVESCESC = sqrt(2GM / R)= sqrt(2GM / R)
 From thatFrom that
Schwarzschild RadiusSchwarzschild Radius
can be easily found.can be easily found.
 All comes down to aAll comes down to a
matter of density.matter of density.
√(2∗GM
R )
Thinking in Terms of GeneralThinking in Terms of General
RelativityRelativity
 Einstein’s Theory ofEinstein’s Theory of
General RelativityGeneral Relativity
basically says thatbasically says that
gravity warps spacegravity warps space
time.time.
 It can be depicted byIt can be depicted by
drawing an analogy todrawing an analogy to
bending rubberbending rubber
sheets.sheets.
The Bending of Space and
Time
Types of Black HolesTypes of Black Holes
 ““Normal Sized” BlackNormal Sized” Black
HolesHoles
 Microscopic (Primordial)Microscopic (Primordial)
SizedSized
 Super-Massive BlackSuper-Massive Black
Holes (On the order ofHoles (On the order of
millions to billions ofmillions to billions of
Solar Masses)Solar Masses)
 (Estimated 3 million solar(Estimated 3 million solar
masses for Milky Waymasses for Milky Way
Black Hole)Black Hole)
How Normal Black Holes ComeHow Normal Black Holes Come
AboutAbout
 Most Black Holes areMost Black Holes are
believed to comebelieved to come
about from the deathabout from the death
of massive stars.of massive stars.
 These deaths areThese deaths are
termed as Supernova.termed as Supernova.
Supernovas ExplainedSupernovas Explained
 After many fusion cycles, star’s core reduces to FeAfter many fusion cycles, star’s core reduces to Fe3+3+ (Iron)(Iron)
ion. If the star now is of mass M < 1.4 Mion. If the star now is of mass M < 1.4 Msunsun , the star will, the star will
degenerate as a Type II supernova. Otherwise, itdegenerate as a Type II supernova. Otherwise, it
becomes a white dwarf, supported by degeneratebecomes a white dwarf, supported by degenerate
electron pressure.electron pressure.
 This mass limit for supernovas is the Chandrasekhar limit.This mass limit for supernovas is the Chandrasekhar limit.
Black Hole or Neutron Star?Black Hole or Neutron Star?
 If the star the wentIf the star the went
supernova was betweensupernova was between
1.4 and 3 M1.4 and 3 Msunsun , then the, then the
remnant will be a Neutronremnant will be a Neutron
Star supported byStar supported by
degenerate neutrondegenerate neutron
pressure (Pulsar).pressure (Pulsar).
 Otherwise,Otherwise,
MMfinalfinal > 3M> 3Msunsun , and the result, and the result
is a black hole because theis a black hole because the
is no source of outwardis no source of outward
pressure strong enough.pressure strong enough.
Where Could Super-Massive BlackWhere Could Super-Massive Black
Holes Exist?Holes Exist?
 The only known placesThe only known places
in the Universe wherein the Universe where
there could be enoughthere could be enough
mass in one area is inmass in one area is in
the center of massivethe center of massive
galaxiesgalaxies
 Not believed to beNot believed to be
anywhere elseanywhere else
The Stellar Seed ModelThe Stellar Seed Model
 Provided that theProvided that the
surroundingsurrounding
environment isenvironment is
sufficiently rich insufficiently rich in
matter, a giant blackmatter, a giant black
hole could result in anhole could result in an
initial “stellar seed” ofinitial “stellar seed” of
10 M10 Msunsun producedproduced
during a supernova.during a supernova.
Optical JetsOptical Jets
 The magnetic fieldsThe magnetic fields
around the black holesaround the black holes
come from thecome from the
surrounding hot matters.surrounding hot matters.
 The jets are made by theThe jets are made by the
Magnetic field of theMagnetic field of the
matter before it goes inmatter before it goes in
the Black Hole.the Black Hole.
 They emit synchrotronThey emit synchrotron
radio signalsradio signals
Cygnus A
CannibalismCannibalism
 Apparently, Quasars areApparently, Quasars are
only active on order ofonly active on order of
100 million years100 million years
 A dead quasar could beA dead quasar could be
revived with a new sourcerevived with a new source
food—by collidingfood—by colliding
galaxiesgalaxies
 Proof—elliptical galaxiesProof—elliptical galaxies
have been found to behave been found to be
active in radioactive in radio
transmissions as well.transmissions as well. Collision Galaxies NGC
2207 & IC 2163
The Expanding UniverseThe Expanding Universe
 There exist anThere exist an
observationobservation
stating whereverstating wherever
a person look ata person look at
into theinto the
universe, heuniverse, he
would observewould observe
everythingeverything
moving away.moving away.
 Of course , this isOf course , this is
not possible in anot possible in a
finite geometry.finite geometry.
More on expansion...More on expansion...
The universe
now centered
on the blue and
red dots.
Even more...Even more...
The universe
now centered
somewhere
else.
Observations of Super MassiveObservations of Super Massive
Black HolesBlack Holes
 Radio observations atRadio observations at
various radiovarious radio
telescopestelescopes
 X-Ray observationsX-Ray observations
from the orbitalfrom the orbital
Chandra ObservatoryChandra Observatory
 Optical observationsOptical observations
from Hubble Spacefrom Hubble Space
TelescopeTelescope
Travelling Towards a Black HoleTravelling Towards a Black Hole
It shouldn’t come as a surprise that we would die ifIt shouldn’t come as a surprise that we would die if
we were to travel towards a black hole. But whatwe were to travel towards a black hole. But what
is interesting is what happens before that.is interesting is what happens before that.
How would a Black Hole appear to us?How would a Black Hole appear to us?
1. Light coming from behind is distorted1. Light coming from behind is distorted
2. Hence objects far behind it would appear as2. Hence objects far behind it would appear as
a ring.a ring.
3. This is known as Gravitational Lensing.3. This is known as Gravitational Lensing.
Photon SpherePhoton Sphere
1. The next interesting stop is1. The next interesting stop is
photon sphere.photon sphere.
2. At this point more than half2. At this point more than half
of our vision is in completeof our vision is in complete
darkness.darkness.
3. The light neither gets sucked in nor leaves the Black Hole.3. The light neither gets sucked in nor leaves the Black Hole.
4. In this region, Photon particles orbit the4. In this region, Photon particles orbit the Event Horizon.Event Horizon.
5. Seeing in this region, one can get his or her rear view.5. Seeing in this region, one can get his or her rear view.
The Observer’s ViewThe Observer’s View
1. A falling object would not1. A falling object would not
be sucked in suddenly.be sucked in suddenly.
Fall would gradually slowFall would gradually slow
down.down.
2. It continues till event2. It continues till event
horizon where light cannothorizon where light cannot
escape.escape.
3. Object falls towards3. Object falls towards
singularity until diminishing view of the Universe finallysingularity until diminishing view of the Universe finally
disappears and there’s complete darkness.disappears and there’s complete darkness.
SpaghettificationSpaghettification
1. Now this is where things
would start to hurt.
2. Gravitational pull across
space is greater.
3. So parts facing singularity
will be pulled more
strongly than those facing
away.
4. The difference is so
pronounced that our body
will be stretched. The
effect is so incredible that
the scientists call it
Spaghettification.
Fate of UniverseFate of Universe
 All Black Holes Evaporate over time due to HawkingAll Black Holes Evaporate over time due to Hawking
RadiationRadiation
 Eventually the Universe will have no matter in a cold darkEventually the Universe will have no matter in a cold dark
death and all there will be left is radiation.death and all there will be left is radiation.
 Estimated Evaporation Time:Estimated Evaporation Time:
1010-7-7 (M/M(M/Msunsun))33 YearsYears
On order of 10On order of 102020 yearsyears
PicturesPictures
NGC4261
ConclusionConclusion
Existence of black holes are highly debated. However,Existence of black holes are highly debated. However,
without them the universe doesn’t seem to make anywithout them the universe doesn’t seem to make any
sense.sense.
The facts provide strong evidences that they do exist allThe facts provide strong evidences that they do exist all
over the space.over the space.
BibliographyBibliography
https://en.wikipedia.org/wiki/Supermassive_black_holehttps://en.wikipedia.org/wiki/Supermassive_black_hole

The Metaphysics BlogThe Metaphysics Blog

NASA Think Tank.NASA Think Tank. “NASA Hubble Web Exploratorium”.“NASA Hubble Web Exploratorium”. Annual SpaceAnnual Space
Magazine 2002Magazine 2002

http://www.exploratorium.edu/origins/hubble/tools/center.htmlhttp://www.exploratorium.edu/origins/hubble/tools/center.html

Carroll, Sean M.Carroll, Sean M. Spacetime and Geometry.Spacetime and Geometry. Toronto. Pearson.Toronto. Pearson.
20072007
Thank You

The Supernova and Black Holes

  • 1.
    Subhadra Sundar Chakraborty(CSE/2015/043) S. Tushar (CSE/2015/042) Amar Kr. Gupta (CSE/2015/053) Akhil Mishra (CSE/2015/060) Akshay Mishra (CSE/2015/052) The Supernova andThe Supernova and Black HolesBlack Holes HU481 Technical Report Writing & Language Laboratory
  • 2.
    Black Holes: ATheoreticalBlack Holes: A Theoretical DefinitionDefinition  An area of space-timeAn area of space-time with a gravitationalwith a gravitational field so intense thatfield so intense that it’s escape velocity isit’s escape velocity is equal to or exceedsequal to or exceeds the speed of light.the speed of light.  The important thing isThe important thing is that this area can be ofthat this area can be of any size.any size.
  • 3.
    The Finite Speedof LightThe Finite Speed of Light  The base of physicalThe base of physical theories assumes thattheories assumes that speed of light inspeed of light in vacuum is finite andvacuum is finite and maximum possible.maximum possible. (A black-hole-powered jet of(A black-hole-powered jet of subatomic particles traveling atsubatomic particles traveling at nearly the speed of light out of thenearly the speed of light out of the M87 galaxy)M87 galaxy)
  • 4.
    Escape Velocity, Density,andEscape Velocity, Density, and Schwarzschild RadiusSchwarzschild Radius  Every entity has anEvery entity has an escape velocity asescape velocity as  VVESCESC = sqrt(2GM / R)= sqrt(2GM / R)  From thatFrom that Schwarzschild RadiusSchwarzschild Radius can be easily found.can be easily found.  All comes down to aAll comes down to a matter of density.matter of density. √(2∗GM R )
  • 5.
    Thinking in Termsof GeneralThinking in Terms of General RelativityRelativity  Einstein’s Theory ofEinstein’s Theory of General RelativityGeneral Relativity basically says thatbasically says that gravity warps spacegravity warps space time.time.  It can be depicted byIt can be depicted by drawing an analogy todrawing an analogy to bending rubberbending rubber sheets.sheets. The Bending of Space and Time
  • 6.
    Types of BlackHolesTypes of Black Holes  ““Normal Sized” BlackNormal Sized” Black HolesHoles  Microscopic (Primordial)Microscopic (Primordial) SizedSized  Super-Massive BlackSuper-Massive Black Holes (On the order ofHoles (On the order of millions to billions ofmillions to billions of Solar Masses)Solar Masses)  (Estimated 3 million solar(Estimated 3 million solar masses for Milky Waymasses for Milky Way Black Hole)Black Hole)
  • 7.
    How Normal BlackHoles ComeHow Normal Black Holes Come AboutAbout  Most Black Holes areMost Black Holes are believed to comebelieved to come about from the deathabout from the death of massive stars.of massive stars.  These deaths areThese deaths are termed as Supernova.termed as Supernova.
  • 8.
    Supernovas ExplainedSupernovas Explained After many fusion cycles, star’s core reduces to FeAfter many fusion cycles, star’s core reduces to Fe3+3+ (Iron)(Iron) ion. If the star now is of mass M < 1.4 Mion. If the star now is of mass M < 1.4 Msunsun , the star will, the star will degenerate as a Type II supernova. Otherwise, itdegenerate as a Type II supernova. Otherwise, it becomes a white dwarf, supported by degeneratebecomes a white dwarf, supported by degenerate electron pressure.electron pressure.  This mass limit for supernovas is the Chandrasekhar limit.This mass limit for supernovas is the Chandrasekhar limit.
  • 9.
    Black Hole orNeutron Star?Black Hole or Neutron Star?  If the star the wentIf the star the went supernova was betweensupernova was between 1.4 and 3 M1.4 and 3 Msunsun , then the, then the remnant will be a Neutronremnant will be a Neutron Star supported byStar supported by degenerate neutrondegenerate neutron pressure (Pulsar).pressure (Pulsar).  Otherwise,Otherwise, MMfinalfinal > 3M> 3Msunsun , and the result, and the result is a black hole because theis a black hole because the is no source of outwardis no source of outward pressure strong enough.pressure strong enough.
  • 10.
    Where Could Super-MassiveBlackWhere Could Super-Massive Black Holes Exist?Holes Exist?  The only known placesThe only known places in the Universe wherein the Universe where there could be enoughthere could be enough mass in one area is inmass in one area is in the center of massivethe center of massive galaxiesgalaxies  Not believed to beNot believed to be anywhere elseanywhere else
  • 11.
    The Stellar SeedModelThe Stellar Seed Model  Provided that theProvided that the surroundingsurrounding environment isenvironment is sufficiently rich insufficiently rich in matter, a giant blackmatter, a giant black hole could result in anhole could result in an initial “stellar seed” ofinitial “stellar seed” of 10 M10 Msunsun producedproduced during a supernova.during a supernova.
  • 12.
    Optical JetsOptical Jets The magnetic fieldsThe magnetic fields around the black holesaround the black holes come from thecome from the surrounding hot matters.surrounding hot matters.  The jets are made by theThe jets are made by the Magnetic field of theMagnetic field of the matter before it goes inmatter before it goes in the Black Hole.the Black Hole.  They emit synchrotronThey emit synchrotron radio signalsradio signals Cygnus A
  • 13.
    CannibalismCannibalism  Apparently, QuasarsareApparently, Quasars are only active on order ofonly active on order of 100 million years100 million years  A dead quasar could beA dead quasar could be revived with a new sourcerevived with a new source food—by collidingfood—by colliding galaxiesgalaxies  Proof—elliptical galaxiesProof—elliptical galaxies have been found to behave been found to be active in radioactive in radio transmissions as well.transmissions as well. Collision Galaxies NGC 2207 & IC 2163
  • 14.
    The Expanding UniverseTheExpanding Universe  There exist anThere exist an observationobservation stating whereverstating wherever a person look ata person look at into theinto the universe, heuniverse, he would observewould observe everythingeverything moving away.moving away.  Of course , this isOf course , this is not possible in anot possible in a finite geometry.finite geometry.
  • 15.
    More on expansion...Moreon expansion... The universe now centered on the blue and red dots.
  • 16.
    Even more...Even more... Theuniverse now centered somewhere else.
  • 17.
    Observations of SuperMassiveObservations of Super Massive Black HolesBlack Holes  Radio observations atRadio observations at various radiovarious radio telescopestelescopes  X-Ray observationsX-Ray observations from the orbitalfrom the orbital Chandra ObservatoryChandra Observatory  Optical observationsOptical observations from Hubble Spacefrom Hubble Space TelescopeTelescope
  • 18.
    Travelling Towards aBlack HoleTravelling Towards a Black Hole It shouldn’t come as a surprise that we would die ifIt shouldn’t come as a surprise that we would die if we were to travel towards a black hole. But whatwe were to travel towards a black hole. But what is interesting is what happens before that.is interesting is what happens before that. How would a Black Hole appear to us?How would a Black Hole appear to us? 1. Light coming from behind is distorted1. Light coming from behind is distorted 2. Hence objects far behind it would appear as2. Hence objects far behind it would appear as a ring.a ring. 3. This is known as Gravitational Lensing.3. This is known as Gravitational Lensing.
  • 19.
    Photon SpherePhoton Sphere 1.The next interesting stop is1. The next interesting stop is photon sphere.photon sphere. 2. At this point more than half2. At this point more than half of our vision is in completeof our vision is in complete darkness.darkness. 3. The light neither gets sucked in nor leaves the Black Hole.3. The light neither gets sucked in nor leaves the Black Hole. 4. In this region, Photon particles orbit the4. In this region, Photon particles orbit the Event Horizon.Event Horizon. 5. Seeing in this region, one can get his or her rear view.5. Seeing in this region, one can get his or her rear view.
  • 20.
    The Observer’s ViewTheObserver’s View 1. A falling object would not1. A falling object would not be sucked in suddenly.be sucked in suddenly. Fall would gradually slowFall would gradually slow down.down. 2. It continues till event2. It continues till event horizon where light cannothorizon where light cannot escape.escape. 3. Object falls towards3. Object falls towards singularity until diminishing view of the Universe finallysingularity until diminishing view of the Universe finally disappears and there’s complete darkness.disappears and there’s complete darkness.
  • 21.
    SpaghettificationSpaghettification 1. Now thisis where things would start to hurt. 2. Gravitational pull across space is greater. 3. So parts facing singularity will be pulled more strongly than those facing away. 4. The difference is so pronounced that our body will be stretched. The effect is so incredible that the scientists call it Spaghettification.
  • 22.
    Fate of UniverseFateof Universe  All Black Holes Evaporate over time due to HawkingAll Black Holes Evaporate over time due to Hawking RadiationRadiation  Eventually the Universe will have no matter in a cold darkEventually the Universe will have no matter in a cold dark death and all there will be left is radiation.death and all there will be left is radiation.  Estimated Evaporation Time:Estimated Evaporation Time: 1010-7-7 (M/M(M/Msunsun))33 YearsYears On order of 10On order of 102020 yearsyears
  • 23.
  • 24.
    ConclusionConclusion Existence of blackholes are highly debated. However,Existence of black holes are highly debated. However, without them the universe doesn’t seem to make anywithout them the universe doesn’t seem to make any sense.sense. The facts provide strong evidences that they do exist allThe facts provide strong evidences that they do exist all over the space.over the space.
  • 25.
    BibliographyBibliography https://en.wikipedia.org/wiki/Supermassive_black_holehttps://en.wikipedia.org/wiki/Supermassive_black_hole  The Metaphysics BlogTheMetaphysics Blog  NASA Think Tank.NASA Think Tank. “NASA Hubble Web Exploratorium”.“NASA Hubble Web Exploratorium”. Annual SpaceAnnual Space Magazine 2002Magazine 2002  http://www.exploratorium.edu/origins/hubble/tools/center.htmlhttp://www.exploratorium.edu/origins/hubble/tools/center.html  Carroll, Sean M.Carroll, Sean M. Spacetime and Geometry.Spacetime and Geometry. Toronto. Pearson.Toronto. Pearson. 20072007
  • 26.