• Keine Ergebnisse gefunden

BLACK HOLES II (136.029)

N/A
N/A
Protected

Academic year: 2022

Aktie "BLACK HOLES II (136.029)"

Copied!
1
0
0

Wird geladen.... (Jetzt Volltext ansehen)

Volltext

(1)

Daniel Grumiller

Institute for Theoretical Physics

BLACK HOLES II (136.029)

Summer semester 12 Location: Thomas Schopper HS

Time: 13:30-15:45 each Monday (starting March 5) Summary:

Black holes have advanced to the forefront of current research in various disciplines: besides the obvious ones, general relativity, mathematical physics and astrophysics, also string theory, quantum chromodynamics, cosmology, computational physics, quantum gravity and even part of condensed matter physics devote a significant fraction of their resources to the study of black holes. It is thus both a fascinating and timely subject to investigate.

The main purpose of this lecture is a treatment of advanced topics and current research topics in black hole physics.

Contents:

Global structure of black holes: horizons and singularities Critical collapse, quasi-normal modes and numerical relativity Dimensionally reduced black holes I: 2D gravity

Charged black holes and BPS solutions The four laws of black hole mechanics

Gedankenexperiments and black hole thermodynamics

Hawking effect, black hole evaporation and information paradox Black holes in AdS space & Hawking-Page transition

Holographic renormalization & Brown-York stress tensor Dimensionally reduced black holes II: 3D gravity

Black holes in string theory and AdS/CFT

Shear viscosity in relativistic heavy ion collisions

… and possibly further selected recent research topics like higher spin gravity

webpage:

http://quark.itp.tuwien.ac.at/~grumil/teaching.shtml

Referenzen

ÄHNLICHE DOKUMENTE

Compare the p = 1 case with the (computer-) experimental results for the Schwarzschild black hole by Nollert (Phys... Which solution do you obtain for the special case M = −1/8, J

Finally, for the dimensionless rate of period decrease you can equate the rate at which the total energy of a binary system changes, dE tot / dt ∝ d/ dt(−M 2 /R) to (minus)

It can be shown that for suitable choices of the func- tions U, V and for p = 1 the model above is classically equivalent to the s-wave part of General Relativity minimally coupled to

Consider a piece of coal at zero temperature and a laser beam (a pure quantum state with some finite energy and entropy) in vacuum as initial state.. Provided the laser beam is

Finally, check which constraints have (weakly) vanishing Poisson brackets among themselves and with the Hamiltonian — these are then first class constraints, while all other

Note: I am not sure what is the most efficient way of doing this calcula- tion; I started with the variation δ(g µν ∇ µ n ν ) and proceeded from there, but there might be a

Use this ar- gument to find a representation of the full quantum gravity partition function that is as simple as possible.. These exercises are due on June 14

But conceptually this exercise may be non- trivial, so remember what is a thermal state in AdS 3 , look up the Brown–Henneaux result for the central charges and recall that the sum