Cosmic microwave background constraints on a decaying cosmological term related to the thermal evolution

Riou Nakamura, Masa Aki Hashimoto, Kiyotomo Ichiki

研究成果: ジャーナルへの寄稿記事

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We constrain the thermal evolution of the universe with a decaying cosmological term by using the method of the analysis for the Wilkinson Microwave Anisotropy Probe (WMAP) observation data. The cosmological term is assumed to be a function of the scale factor that increases toward the early universe, and the radiation energy density is lower compared to that in the model with the standard cosmological constant (ΛCDM). The decrease in the radiation density affects the thermal history of the universe; e.g. the photon decoupling occurs at higher-z compared to the case of the standard ΛCDM model. As a consequence, a decaying cosmological term affects the cosmic microwave background (CMB) anisotropy. Thanks to the Markov-Chain Monte Carlo method, we compare the angular power spectrum in the decaying ΛCDM model with the CMB data, and we get severe constraints on parameters of the model.

元の言語英語
記事番号123511
ジャーナルPhysical Review D - Particles, Fields, Gravitation and Cosmology
77
発行部数12
DOI
出版物ステータス出版済み - 6 10 2008

    フィンガープリント

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)

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