Published November 23, 2008 | Version v1
Journal article Metadata-only

Gravitational wave background as a probe of reheating temperature of the Universe

Creators

  • 1. Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582 (Japan)
  • 2. Department of Physics, Graduate School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033 (Japan)
  • 3. Institute for the Physics and Mathematics of the Universe (IPMU), University of Tokyo, Kashiwa, Chiba 277-8568 (Japan)
  • 4. Research Center for the Early Universe (RESCEU), Graduate School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033 (Japan)

Description

It is shown that the reheating temperature of the Universe can be determined observationally by future space-based laser interferometer experiments such as DECIGO and/or BBO if it is around 106-9 GeV, depending on the tensor-to-scalar ratio r. As an application, it may provide an evidence of the gravitino dark matter scenario, if it is the LSP.

Additional details

Identifiers

DOI
10.1063/1.3052013;

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1078
Journal Issue
1
Journal Page Range
p. 515-517
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
16. international conference on supersymmetry and the unification of fundamental interactions
Acronym
SUSY08
Dates
16-21 Jun 2008
Place
Seoul (Korea, Republic of)

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
41005697
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
COSMOLOGY; EEV RANGE; GRAVITATIONAL WAVES; INTERFEROMETERS; LASERS; NONLUMINOUS MATTER; PEV RANGE; STANDARD MODEL; TENSORS; UNIVERSE
Descriptors DEC
ENERGY RANGE; FIELD THEORIES; GRAND UNIFIED THEORY; MATHEMATICAL MODELS; MATTER; MEASURING INSTRUMENTS; PARTICLE MODELS; QUANTUM FIELD THEORY; UNIFIED GAUGE MODELS

Optional Information

Notes
(c) 2008 American Institute of Physics