Super massive Black holes

Содержание

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Black Holes: A Theoretical Definition (A Review)

An area of space-time with a

Black Holes: A Theoretical Definition (A Review) An area of space-time with
gravitational field so intense that its escape velocity is equal to or exceeds the speed of light.
The Important thing is that this area can be of any size.

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The Finite Speed of Light

As you all know (especially Contemporary people), That

The Finite Speed of Light As you all know (especially Contemporary people),
the speed of light is a finite value in a vacuum.
(A black-hole-powered jet of sub-atomic particles traveling at nearly the speed of light out of the M87 galaxy)

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Escape Velocity, Density, and Schwarzschild Radius

In terms of gravitational force, every object

Escape Velocity, Density, and Schwarzschild Radius In terms of gravitational force, every
has an escape velocity as
vesc = Sqrt[(2 G M)/r].
From that Schwarzschild Radius can be easily found.
All comes down to a matter of density.

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Thinking in Terms of General Relativity

Einstein’s Theory of General Relativity basically says

Thinking in Terms of General Relativity Einstein’s Theory of General Relativity basically
that gravity warps space time.
Rubber Sheet analogue
Down, up, and through the funnel. An embedding diagram is generally a good representation of a black hole's warping of nearby space-time. But such 2-dimensional illustrations can also cause conceptual problems.

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This is a simplified model

The black hole no hair theorem shows that

This is a simplified model The black hole no hair theorem shows
mass, charge, and angular momentum are the only properties a black hole can possess

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Types of Black Holes

“Normal Sized” Black Holes
Microscopic (Primordial) Sized
Super-Massive Black Holes (On

Types of Black Holes “Normal Sized” Black Holes Microscopic (Primordial) Sized Super-Massive
the order of millions to billions of Solar Masses)
(Estimated 3 million solar masses for Milky Way Black Hole)

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How Normal Black Holes Come About (A Review)

Most Black Holes are believed

How Normal Black Holes Come About (A Review) Most Black Holes are
to come about from the death of massive stars.

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Stellar Evolution (Brief)

Star (Mass of Hydrogen) is massive enough (M > 0.1

Stellar Evolution (Brief) Star (Mass of Hydrogen) is massive enough (M >
Msun ) to ignite fusion
Star performs stable core fusion (first H->HE)
Cycle repeats if star is big enough until the core is Fe.
Star is in a kind of onion peel structure of elemental layers

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Supernovas!?

After fusion cycles through and star’s core is Fe, if the star

Supernovas!? After fusion cycles through and star’s core is Fe, if the
now is M < 1.4 Msun , the star will supernova as a Type II supernova. Otherwise, it becomes a white dwarf, supported by degenerate electron pressure.
This mass limit for supernovas is the Chandrasekhar limit.

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Black Hole or Neutron Star?

If the star the went supernova was between

Black Hole or Neutron Star? If the star the went supernova was
1.4 and 3 Msun , then the remnant will be a Neutron Star supported by degenerate neutron pressure (Pulsar).
Otherwise,
Mfinal > 3Msun , and the result is a black hole because the is no source of outward pressure strong enough.

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Where Could Super-Massive Black Holes Exist?

The only known places in the Universe

Where Could Super-Massive Black Holes Exist? The only known places in the
where there could be enough mass in one area is in the center of massive galaxies
Not believed to be anywhere else

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Quasars: What are They?

In some places where point sources of radio waves

Quasars: What are They? In some places where point sources of radio
were found, no visible source other than a stellar-looking object was found (it looked like a point of like --- like a star does). These objects were called the "qausi-stellar radio sources", or "quasars" for short.
Later, it was found these sources could not be stars in our galaxy, but must be very far away --- as far as any of the distant galaxies seen. We now think these objects are the very bright centers of some distant galaxies, where some sort of energetic action is occurring.

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Active Galactic Nuclei

In some galaxies, known as "active galactic nuclei" (AGN), the

Active Galactic Nuclei In some galaxies, known as "active galactic nuclei" (AGN),
nucleus (or central core) produces more radiation than the entire rest of the galaxy! Quasars are very distant AGN - the most distant quasars mark an epoch when the universe was less than a billion years old and a sixth of its current size.

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Brief Review of case for Super-Massive Black Holes in these observed AGN

The

Brief Review of case for Super-Massive Black Holes in these observed AGN
Time Variation of AGN
The Eddington Luminosity Argument
The Motion of broad line emission medium around the central core

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How did Super-Massive Black Holes come about?--theories

From “Lumps” in the early universe
The

How did Super-Massive Black Holes come about?--theories From “Lumps” in the early
“Stellar Seed” Model
Collapse of a whole star cluster

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Lumps from the early Universe

In the “Big Bang” the whole universe was

Lumps from the early Universe In the “Big Bang” the whole universe
in a really dense state. So much that perhaps lumps could have formed and of matter dense enough that a black hole was formed.
There was enough surrounding matter that galaxies formed around the lumps
Could explain why pockets of interstellar gas never became galaxies

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The Stellar Seed Model

Provided that the surrounding environment is sufficiently rich in

The Stellar Seed Model Provided that the surrounding environment is sufficiently rich
matter, a giant black hole could result in an initial “stellar seed” of 10 Msun produced during a supernova.

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Collapse of a whole cluster

If the stars of a tight knit cluster

Collapse of a whole cluster If the stars of a tight knit
of the moderately young Universe had all relatively the same size stars (above the Chandrasekhar Limit), there would be quite a few Black Holes forming simultaneously causing smaller stars to be absorbed, and black holes to combine.
NGC 1850 to the right

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Some Characteristic of AGN

Super Bright: AGN 3C273 (an extreme example) is L

Some Characteristic of AGN Super Bright: AGN 3C273 (an extreme example) is
= 4.8*10^12 Lsun .
Cosmic Optical Jets
Tidal forces
Cannibalism—they do eat, the source of energy

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Optical Jets—Why?

The magnetic fields around a black holes that are thought to

Optical Jets—Why? The magnetic fields around a black holes that are thought
produce the spectacular jets of high-energy particles rushing away from black holes come from the disk of hot gas around the black hole, not the black hole itself.
The jets are made by the Magnetic field of the matter before it goes in the Black Hole.
Emit Synchrotron radio signals
Cygnus A

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Tidal forces stretch farther, but are weaker

The tidal force is proportional to

Tidal forces stretch farther, but are weaker The tidal force is proportional
the mass of the black hole. In other words, as the object gets more massive, the force should get bigger too. But the force is also inversely proportional to the cube of the object's radius. As the hole gets more massive, its size increases, but because of the cube factor, the force decreases much faster than any possible mass increase can account for. The result is that big black holes have weak tidal forces, and small ones have strong tidal forces.
Frames from a NASA computer animation depict one possible cause of gamma ray bursts. A star orbiting a black hole spirals in as it is shredded by tidal forces, generating an intense burst of gamma and other radiation as the its matter is compressed and super-heated on its way to oblivion.

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Cannibalism

Apparently, Quasars are only active on order of 100 million years
A dead

Cannibalism Apparently, Quasars are only active on order of 100 million years
quasar could be revived with a new source food—by colliding galaxies
Proof—elliptical galaxies have been found to be active in radio transmissions as well.
Collision Galaxies NGC 2207 & IC 2163

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Observations of Super Massive Black Holes

Radio observations at various radio telescopes
X-ray observations

Observations of Super Massive Black Holes Radio observations at various radio telescopes
from the orbital Chandra Observatory
Optical Observations from Hubble Space Telescope

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Pictures

NGC4261

Pictures NGC4261

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Fate of Universe?

All Black Holes Evaporate over time due to Hawking Radiation
Eventually

Fate of Universe? All Black Holes Evaporate over time due to Hawking
the Universe will have no matter in a cold dark death and all there will be left is radiation.
Evaporation Time:
1 * 10^-7 (M/Msun)^3 Years
On order of 1* 10^20 years