ar X iv : g r - qc / 0 61 21 14 v 1 19 D ec 2 00 6 Fluctuations of CMBR in accelerating universe

ar X iv : g r - qc / 0 21 00 04 v 1 2 O ct 2 00 2 TIME DEPENDENCE OF BRANS - DICKE PARAMETER ω FOR AN EXPANDING UNIVERSE

We have studied the time dependence of ω for an expanding universe in the generalised B-D theory and have obtained its explicit dependence on the nature of matter contained in the universe in different era.Lastly, we discuss how the observed accelerated expansion of the present universe can be accomodated in the formalism.

ar X iv : g r - qc / 0 21 00 45 v 1 1 5 O ct 2 00 2 Cosmological Parameters are Dressed

Thomas Buchert ∗ and Mauro Carfora † Theoretische Physik, Ludwig–Maximilians–Universität, Theresienstr. 37, D–80333 München, Germany and Department of Physics and Research Center for the Early Universe (RESCEU), School of Science, The University of Tokyo, Tokyo 113–0033, Japan Dipartimento di Fisica Nucleare e Teorica, Università degli Studi di Pavia and Istituto Nazionale di Fisica Nucleare, S...

ar X iv : g r - qc / 0 41 21 17 v 1 2 3 D ec 2 00 4 A quantum mass - spectrum of Kerr black hole : superstrings

Using thermal quantization of geodesics confined under horizons and reasonable conjecture on massless modes, we evaluate quantum spectrum of Kerr black hole masses compatible with superstring symmetries.

ar X iv : g r - qc / 0 11 20 12 v 1 7 D ec 2 00 1 RELATIVISTIC GRAVITY WITH A DYNAMICAL PREFERRED FRAME

ar X iv : g r - qc / 0 61 21 85 v 1 2 9 D ec 2 00 6 Bianchi Type V Universes with Bulk Viscosity in General Relativity

Bianchi type V bulk viscous fluid cosmological models are investigated. Using a generation technique (Camci et al., 2001), it is shown that the Einstein’s field equations are solvable for any arbitrary cosmic scale function. The viscosity coefficient of bulk viscous fluid is assumed to be a power function of mass density. Solutions for particular forms of cosmic scale functions are also obtaine...