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Bianchi type II brane-world cosmologies(U>~0)

2002/12/23 by R. J. van den Hoogen, J. Ibáñez, J. Ibanez · 1 citation
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Brane #Cosmology and Gravitation Theories #Ecology #Geometry #Isotropy #Mathematical physics #Mathematics #Noncommutative and Quantum Gravity Theories #Perfect fluid #Physics #Quantum mechanics #Scalar (mathematics) #Scalar field #Singularity #Theoretical physics #Type (biology) #gr-qc

paper · pdf · doi:10.1103/physrevd.67.083510

published as Phys.Rev. D67 (2003) 083510 · 30 pages, 28 eps figures, Revtex

arxiv created 2002/12/23 · openalex publication_date 2003/04/24 · arxiv updated 2009/11/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

The asymptotic properties of the Bianchi type II cosmological model in the brane-world scenario are investigated. The matter content is assumed to be a combination of a perfect fluid and a minimally coupled scalar field that is restricted to the brane. The isotropic brane-world solution is determined to represent the initial singularity in all brane-world cosmologies. Additionally, it is shown that it is the kinetic energy of the scalar field which dominates the initial dynamics in these brane-world cosmologies. It is important to note that the dynamics of these brane-world cosmologies is not necessarily asymptotic to general relativistic cosmologies to the future in the case of a zero four-dimensional cosmological constant.

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