Published March 2015 | Version v1
Journal article

Dynamics of Robertson–Walker spacetimes with diffusion

  • 1. Centro de Análise Matemática, Geometria e Sistemas Dinâmicos, Instituto Superior Técnico, Lisboa (Portugal)
  • 2. Department of Mathematical Sciences, Chalmers University of Technology, University of Gothenburg, Gothenburg (Sweden)
  • 3. Departamento de Matemática e Aplicações, Universidade do Minho, Guimarães (Portugal)
  • 4. Centro de Matemática, Universidade do Minho, Braga (Portugal)

Description

We study the dynamics of spatially homogeneous and isotropic spacetimes containing a fluid undergoing microscopic velocity diffusion in a cosmological scalar field. After deriving a few exact solutions of the equations, we continue by analyzing the qualitative behavior of general solutions. To this purpose we recast the equations in the form of a two dimensional dynamical system and perform a global analysis of the flow. Among the admissible behaviors, we find solutions that are asymptotically de-Sitter both in the past and future time directions and which undergo accelerated expansion at all times

Availability note (English)

Available from http://dx.doi.org/10.1016/j.aop.2015.01.010

Additional details

Identifiers

DOI
10.1016/j.aop.2015.01.010;
arXiv
arXiv:1409.4400v2;
PII
S0003-4916(15)00013-5;

Publishing Information

Journal Title
Annals of Physics (New York)
Journal Volume
354
Journal Page Range
p. 475-488
ISSN
0003-4916
CODEN
APNYA6

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
47017156
Subject category
S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
COSMOLOGY; DE SITTER GROUP; DIFFUSION; EXACT SOLUTIONS; SCALAR FIELDS; SPACE-TIME; TWO-DIMENSIONAL CALCULATIONS
Descriptors DEC
LIE GROUPS; MATHEMATICAL SOLUTIONS; SYMMETRY GROUPS

Optional Information

Copyright
Copyright (c) 2015 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.