Published February 15, 2008 | Version v1
Journal article

New interactions in the dark sector mediated by dark energy

  • 1. Astroparticle Theory and Cosmology Group, Department of Physics and Astronomy, University of Sheffield, Hounsfield Road, Sheffield S3 7RH (United Kingdom)
  • 2. Astroparticle Theory and Cosmology Group, Department of Applied Mathematics, University of Sheffield, Hounsfield Road, Sheffield S3 7RH (United Kingdom)

Description

Cosmological observations have revealed the existence of a dark matter sector, which is commonly assumed to be made up of one particle species only. However, this sector might be more complicated than we currently believe: there might be more than one dark matter species (for example, two components of cold dark matter or a mixture of hot and cold dark matter) and there may be new interactions between these particles. In this paper we study the possibility of multiple dark matter species and interactions mediated by a dark energy field. We study both the background and the perturbation evolution in these scenarios. We find that the background evolution of a system of multiple dark matter particles (with constant couplings) mimics a single fluid with a time-varying coupling parameter. However, this is no longer true on the perturbative level. We study the case of attractive and repulsive forces as well as a mixture of cold and hot dark matter particles

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
77
Journal Issue
4
Journal Page Range
p. 043006-043006.10
ISSN
0556-2821
CODEN
PRVDAQ

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
39059085
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Descriptors DEI
COSMOLOGICAL MODELS; COSMOLOGY; COUPLING; DISTURBANCES; FLUIDS; NONLUMINOUS MATTER; PARTICLE INTERACTIONS; PERTURBATION THEORY
Descriptors DEC
INTERACTIONS; MATHEMATICAL MODELS; MATTER

Optional Information

Notes
(c) 2008 The American Physical Society