LIGO-G1000559-v1 Black holes, Einstein, and gravitational waves Peter R. Saulson Syracuse University.
COLLISIONS IN A D S AND HOLOGRAPHIC THERMALISATION Towards more realistic models of the QGP thermalisation Wilke van der Schee Supervisors: Gleb Arutyunov,
G. Esposito G. Esposito. 1 - Historical background 2 - GR singularities in the sixties 3 - Feynman quantization of GR 4 - Quantum cosmology 5 - Singularity.
Black Holes in Extra Dimensions COSMO 2003, Ambleside Toby Wiseman Cambridge (UK) / Harvard Work with B. Kol (Hebrew University) H. Kudoh (Kyoto)
Far-from-equilibrium isotropisation , quasi-normal modes and radial flow
STRONG COUPLING ISOTROPIZATION SIMPLIFIED Why linearized Einstein’s equations may be enough Wilke van der Schee Universitat de Barcelona, March 22, 2012.
On Recent Developments in N=8 Supergravity Renata Kallosh Renata Kallosh EU RTN Varna, September 15, 2008 Stanford university.
Section 5.4 Gravity Waves. Gravity Waves Gravity acts as the restoring force on parcels displaced from hydrostatic equilibrium. Pure gravity exists when.
On Recent Developments in N =8 Supergravity
Collisions in A d S and holographic thermalisation
Strong coupling isotropization simplified
