69 research outputs found

    Blackhole Evaporation - Stress Tensor Approach

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    On Rumer’s Invariant Theory of Gravitational Waves

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    Propagation of gravitational potential and gravitational field-strength has been considered here on the basis of Rumer’s Invariant Theory of Gravitational Waves. Finally some special cases of weak field have been discusse

    On V-Symmetry in Su (3)

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    Raychaudhuri Equation, Big Bang and Accelerating Universe

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    Quasinormal modes for the charged Vaidya metric

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    The scalar wave equation is considered in the background of a charged Vaidya metric in double null coordinates (u,v)(u,v) describing a non-stationary charged black hole with varying mass m(v)m(v) and charge q(v)q(v). The resulting time-dependent quasinormal modes are presented and analyzed. We show, in particular, that it is possible to identify some signatures in the quasinormal frequencies from the creation of a naked singularity.Comment: 4 pages. Prepared for the proceedings of the Spanish Relativity meeting (ERE2010), Granada, Spain, September 6-10, 201

    The Birkhoff Theorem in Multidimensional Gravity

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    The validity conditions for the extended Birkhoff theorem in multidimensional gravity with nn internal spaces are formulated, with no restriction on space-time dimensionality and signature. Examples of matter sources and geometries for which the theorem is valid are given. Further generalization of the theorem is discussed.Comment: 8 page

    A Class of Renormalization Group Invariant Scalar Field Cosmologies

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    We present a class of scalar field cosmologies with a dynamically evolving Newton parameter GG and cosmological term Λ\Lambda. In particular, we discuss a class of solutions which are consistent with a renormalization group scaling for GG and Λ\Lambda near a fixed point. Moreover, we propose a modified action for gravity which includes the effective running of GG and Λ\Lambda near the fixed point. A proper understanding of the associated variational problem is obtained upon considering the four-dimensional gradient of the Newton parameter.Comment: 10 pages, RevTex4, no figures, to appear on GR
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