2015年8月6日
Cosmic microwave background radiation temperature in a dissipative universe
Physical Review D - Particles, Fields, Gravitation and Cosmology
- ,
- 巻
- 92
- 号
- 4
- 記述言語
- 英語
- 掲載種別
- 研究論文(学術雑誌)
- DOI
- 10.1103/PhysRevD.92.043507
- 出版者・発行元
- American Physical Society
© 2015 American Physical Society. The relationship between the cosmic microwave background radiation temperature and the redshift, i.e., the T-z relation, is examined in a phenomenological dissipative model. The model contains two constant terms, as if a nonzero cosmological constant Λ and a dissipative process are operative in a homogeneous, isotropic, and spatially flat universe. The T-z relation is derived from a general radiative temperature law, as appropriate for describing nonequilibrium states in a creation of cold dark matter model. Using this relation, the radiation temperature in the late Universe is calculated as a function of a dissipation rate ranging from μ=0, corresponding to a nondissipative lambda cold dark matter model, to μ=1, corresponding to a fully dissipative creation of cold dark matter model. The T-z relation for μ=0 is linear for standard cosmology and is consistent with observations. However, with increasing dissipation rate μ, the radiation temperature gradually deviates from a linear law because the effective equation-of-state parameter varies with time. When the background evolution of the Universe agrees with a fine-tuned pure lambda cold dark matter model, the T-z relation for low μ matches observations, whereas the T-z relation for high μ does not. Previous work also found that a weakly dissipative model accords with measurements of a growth rate for clustering related to structure formations. These results imply that low dissipation is likely for the Universe. The weakly dissipative model should be further constrained by recent observations.
- リンク情報
- ID情報
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- DOI : 10.1103/PhysRevD.92.043507
- ISSN : 1550-7998
- eISSN : 1550-2368
- SCOPUS ID : 84940500722