black holes eternal? or just long lived? by patrick murphy
TRANSCRIPT
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Black Holes
Eternal? Or just long lived?
by Patrick Murphy
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A Brief History Of Black Holes.
• First proposed in thought experiment by John Mitchell in 1783
• 1916: Karl Schwarzschild solves Einstein’s field equation for spacetime around a spherical body.
• A little more on Einstein….
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General Relativity
• Published in 1915• Describes the
relationship between mass and spacetime.
• Spacetime tells mass how to move and mass tells spacetime how to curve.
• Confirmed in 1919 by Arthur Eddington
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Spacetime:
• Apparent vs. real trajectory of a light beam
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Karl Schwarzschild
• Solved metric for spacetime surrounding a spherical mass.
• Schwarzschild metric :
• Schwarzschild radius :
2 2 2 2 2ds = 1/(1-2M/r)dr + r d - 1/(1-2M/r)dt
2R = 2GM/c
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Classic Black Holes
• 1939 : Oppenheimer shows massive stars collapse to a singular point.
• Multiple solutions involving small perturbations confirm results.
• Singularity surrounded by event horizon, point of no return.
• Three parameters : Mass, Charge and Spin
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Roger Penrose• 1969: Proved all
full gravitational collapses result in a singularity
• Postulated Cosmic Censorship Law
Classic Black Holes
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2 main types
Schwarzschild• Static, no rotation• Point-like singularity• Event Horizon
Kerr• Rotates• Ring shaped
singularity• Inner Horizon• Outer Horizon• Ergosphere
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2 main types
Schwarzschild Kerr
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So nothing can escape the gravitational attraction of the black hole once past the event horizon?
Classically, yes
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Problems with classical theory
• Assumed TBH = 0 K, despite mathematical evidence to the contrary .
• No thermal spectrum• Singularity too small for Relativity
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Can Black Holes Radiate?
Maybe so…• 1970 : Jacob Berkenstein suggests area
of event horizon is a measurement of black holes entropy.
• 1970 : Stephen Hawking shows that area of event horizon always increases.
• 1971 : Borisovitch Zel’dovitch claims rotating black holes radiate until they stop spinning .
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1974: Hawking Radiation
• Hawking repeats Zel’dovitch’s calculatons.
• Agrees except….• Finds they continue to
radiate!• There’s more…• His solution predicted the
emission spectrum to be exactly that of a hot body.
• That means temperature and entropy
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How can it radiate?
• Various mechanisms are possible, depending on your frame of reference.
• They all acknowledge quantum vacuum fluctuations as source.
• Quantum vacuum fluctuations are unavoidable due to Heisenberg’s Uncertainty Principle
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And…?
• Say you’re safely at rest, watching vacuum fluctuations.
• You see a virtual pair of photons created just outside the event horizon.
• Tidal gravity pulls them apart, they become real.
• One gets sucked in, the other escapes forever.
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So What’s Left?
• Resolution of the “Information paradox”
• Development of an adequate quantum theory of gravity, Relativity is no longer a valid approximation on scales smaller than the Planck length, lp = (hG/2πc3)1/2 .
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Information loss?
• In technical jargon, the black hole has performed a non-unitary transformation on the state of the system. As you may recall, non-unitary evolution is not allowed to occur naturally in a quantum theory because it fails to preserve probability.
• Hawking suggests that black hole radiation contains information about what went in, albeit in a mangled form.
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Branes?
• P brane: length in p dimensions
• P = 1 : String
• P = 2 : Membrane
• Etc…
• Information stored
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Quantum Gravity?
• Singularities are tiny• Quantum foam• No time, how space
manifests itself is probabilistic
• Many candidates, include : M-theory, Supergravity, AdS/CFT , holography …
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So Why study Black holes?
• Black holes push the limits of physical theories
• Among the most extreme phenomena in the universe
• I think they’re cool.• That’s it• Thanks for listening• The End• (applause…. please?)
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References :• Kip Thorne, Black Holes And Timewarps (Norton, 1994)
• Eric Poisson, A Relativist's Toolkit, The mathematics of black hole mechanics (Cambridge University Press, 2004).
• Alessandro Fabbri and Jos\'{e} Navarro-Salas,Modeling Black Hole Evaporation (Imperial College Press, 2005)
• John A. Wheeler, E.F. Taylor, Exploring Black Holes, Introduction to General Relativity (Addison Wesley, 2000)
• Stephen Hawking, The Universe In A Nutshell (Bantam, 2001)
Images :• http://chandra.harvard.edu/resources• http://www.belmontnc.4dw.net/DWFNEU5.gif• www.tqnyc.org/NYC040808/ neutron_star.jpg• http://en.wikipedia.org• www.scienceweek.at