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PowerPoint Presentation Chapter 22 Opener Neutron Stars and Black Holes: Strange States of Matter

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Title: PowerPoint Presentation Chapter 22 Opener Neutron Stars and Black Holes: Strange States of Matter


1
Chapter 22--Second Half Blackholes
Black Holes Einsteins Theories of
Relativity Special Relativity Space Travel Near
Black Holes
2
What is Gravity?
Newtonian Picture
Einstein's Picture
Isaac Newton (1642-1726)
the gravitational field.
3
Foundations of General relativity Principle of
Equivalence It is impossible to tell, from within
a closed system, whether one is in a
gravitational field, or accelerating
4
General Relativity and Gravity
  • In Einsteins General Theory of Relativity,
    gravity arises from the curvature of spacetime
    continuum.
  • The curvature of the spacetime continuum is
    produced by the presence of mass.
  • Massive object distorts spacetime continuum more.
  • Spacetime Continuum
  • We are used to thinking that we have three
    physical dimensions (space), and one time
    dimension. Space and time are separate.

Spacetime is stretched near objects with large
mass, like our Earth.
5
The general theory of relativity
  • Published by Einstein in 1915, this is a theory
    of gravity
  • A massive object causes space to curve and time
    to slow down
  • These effects manifest themselves as a
    gravitational force
  • These distortions of space and time are most
    noticeable in the vicinity of large masses or
    compact objects

6
Orbits of Planets
Verification of General Relativity
43 arcsec/100years
The extra amount of precession of planet
Mercurys orbit is explained by GTR.
7
Verification of General Relativity
Einstein 1918 - should see shift of 1.75 arc
sec. 1919 Solar Eclipse Within 20 of
Prediction! Modern Test - Radio Waves Within 1
of Prediction!
8
Harvard 1959 Atomic clock in basement -
slower! Einstein 2.46x10-15 Observed
2.50x10-15
fast
slow
9
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10
  • If a stellar corpse has a mass greater than about
    2 to 3 M?, gravitational compression will
    overwhelm any and all forms of internal pressure
  • The stellar corpse will collapse to such a high
    density that its escape speed exceeds the speed
    of light

11
Black Hole
Rs radius of event horizon is the size of
black hole. Depends upon mass and the speed of
light.
2GM
Rs
The size of a black hole!
c2
1. Photon Sphere 1.5Rs distance where light can
go into circular orbit! 2. Event Horizon
Rs distance where escape speed equals speed of
light! 3. Singularity Mathematical point at
center we dont know what it is, but it is where
the point of the funnel comes to a head if it
does?
1
2
12
Black Holes
  • Light emitted close to the critical surface is
    severely red-shifted (the frequency is lower) and
    at the critical surface, the redshift is
    infinite. Inside the critical surface, spacetime
    is so warped that objects cannot move outward at
    all, not even light.
  • Events inside the critical surface can never
    affect the region outside the critical surface,
    since no information about them can escape
    gravity.
  • We call this surface the event horizon because
    it shields the outside completely from any events
    on the inside.

13
Black Hole Singularity
  • Singularity central point containing all of
    the mass. Known laws of physics break down.

14
Tidal Forces Near a Black Hole
Matter encountering a black hole will experience
enormous tidal forces that will both heat it
enough to radiate, and tear it apart
15
Gravitational Red Shift Light emitted from
compact object( strong gravity) is red shifted
The photon is giving up energy as it escapes
from the pull of the gravitational field Time
Dilation Clocks in stronger gravity fields
appear to slow down to an external observer.
Time Slows
time slowed
16
Blackhole Evaporation
17
The center of the Blackhole
  • Could a black hole somehow be connected to
    another part of spacetime, or even some other
    universe?
  • General relativity predicts that such
    connections, called wormholes, might exist for
    black holes

18
Travel through a black hole and wormhole to Vega!
19
Gravitational Radiation
LISA A space-based gravity wave observatory
Laser Interferometric Gravitational Observatory
(LIGO)
20
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