Poynting Vector
A first course in general relativity
New Developments and Perspectives in General Relativity and Cosmology Thesis Dennis Smoot University of Illinois Chicago, IL.
Eienstein field equations
D. Vulcanov: Symbolic Computation Methods in Cosmology and General Relativity [3]
COLLISIONS IN A D S AND HOLOGRAPHIC THERMALISATION Towards more realistic models of the QGP thermalisation Wilke van der Schee Supervisors: Gleb Arutyunov,
General Relativity Physics Honours 2008 A/Prof. Geraint F. Lewis Rm 560, A29 [email protected] Lecture Notes 10.
Black hole information via ADM reduction Inyong Park Philander Smith College KIAS, Seoul Dec 2013.
How do we transform between accelerated frames? Consider Newton’s first and second laws: m i is the measure of the inertia of an object – its resistance.
The 2d gravity coupled to a dilaton field with the action This action ( CGHS ) arises in a low-energy asymptotic of string theory models and in certain.
Notes on Black-hole Evatoration - Unruh
THE GRACEFUL EXIT FROM INFLATION AND DARK ENERGY By Tomislav Prokopec Publications: Tomas Janssen and T. Prokopec, arXiv:0707.3919; Tomas Janssen, Shun-Pei.