Braneworld effects on cosmological dynamics
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Braneworld effects on cosmological dynamics

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Published by University of Portsmouth, Institute of Cosmology and Gravitation in Portsmouth .
Written in English


Book details:

Edition Notes

Thesis (Ph.D.) - University of Portsmouth, 2003.

StatementBurin Gumjudpai.
ID Numbers
Open LibraryOL20418996M

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  In the next step we focus briefly o n the cosmological dynamics of a bulk scalar field in the RS II braneworld scenario (see Refs. [48, 49, 66] for details) to see the relation b etween bulk. If the address matches an existing account you will receive an email with instructions to reset your password. Title: Dynamics of Brane-World Cosmological Models. Authors: A. Coley (Submitted on 4 Oct , last revised 25 Apr (this version, v2)) Abstract: We show that generically the initial singularity is isotropic in spatially homogeneous cosmological models in the brane-world scenario. We then argue that it is plausible that the initial Cited by: @article{osti_, title = {Cosmological tachyon condensation}, author = {Bilic, Neven and Tupper, Gary B and Viollier, Raoul D and Centre of Theoretical Physics and Astrophysics, University of Cape Town, Rondebosch }, abstractNote = {We consider the prospects for dark matter/energy unification in k-essence type cosmologies.. General mappings are established between the k-essence.

@article{osti_, title = {Simple coupling with cosmological implications. The initial singularity and the inflationary universe}, author = {Saez, D}, abstractNote = {In this work the metric is coupled with a scalar field phi in a simple way. Although this coupling becomes problematic because the energy density of phi appears to be unbounded from below, it is displayed as a very simple. The explicit forms of the warp factor and the scalar field are given by () f (σ) = − a 1 k e − k | σ |, () T (σ) = 2 k a 1 e k 2 | σ |, for the entire domain of the extra dimension, − ∞ Cited by:   The framework Keeton and Petters developed predicts certain cosmological effects that, if observed, should help scientists validate the braneworld theory. is . Observational Parameters in a Braneworld Inlationary Scenario 1. OBSERVATIONAL PARAMETERS IN A BRANEWORLD INFLATIONARY SCENARIO MILAN MILOŠEVIĆ Department of Physics Faculty of Sciences and Mathematics University of Niš, Serbia Ruđer Bošković Institute, Zagreb, Croatia, 2 November In collaboration with N. Bilić (Zagreb), G. Djordjević (Niš), D. Dimitrijević (Niš) and M.

  The Dynamics of Truth will guide you into understanding of how to operate in the truth of God's Word, for a more abundant life and way of living. The Dynamics of Truth will transform your life like you could never have imagined. You develop God-given principles that will reward you with a life full of health, wealth and : Bertram Wallace. String theory is a broad and varied subject that attempts to address a number of deep questions of fundamental physics. String theory has been applied to a variety of problems in black hole physics, early universe cosmology, nuclear physics, and condensed matter physics, and it has stimulated a number of major developments in pure mathematics.   We review recent developments and results in testing general relativity (GR) at cosmological scales. The subject has witnessed rapid growth during the last two decades with the aim of addressing the question of cosmic acceleration and the dark energy associated with it. However, with the advent of precision cosmology, it has also become a well-motivated endeavor by itself to test Cited by: We review some general aspects of braneworld cosmologies in which an inflationary period driven by a scalar field confined on the brane is described by a nonstandard effective Friedmann equation. The perturbation spectra, consistency equations and observational consequences of Author: Gianluca Calcagni.