Constraints on a vacuum energy from both SNIa and CMB temperature observations

Riou Nakamura, E. P.Berni Ann Thushari, Mikio Ikeda, Masa Aki Hashimoto

研究成果: Contribution to journalArticle査読

抄録

We investigate the cosmic thermal evolution with a vacuum energy which decays into photon at the low redshift. We assume that the vacuum energy is a function of the scale factor that increases toward the early universe. We put on the constraints using recent observations of both type Ia supernovae (SNIa) by Union-2 compilation and the cosmic microwave background (CMB) temperature at the range of the redshift 0.01 < z < 3. From SNIa, we find that the effects of a decaying vacuum energy on the cosmic expansion rate should be very small but could be possible for z < 1.5. On the other hand, we obtain the severe constraints for parameters from the CMB temperature observations. Although the temperature can be still lower than the case of the standard cosmological model, it should only affect the thermal evolution at the early epoch.

本文言語英語
論文番号528243
ジャーナルAdvances in Astronomy
2012
DOI
出版ステータス出版済み - 2012

All Science Journal Classification (ASJC) codes

  • 天文学と天体物理学
  • 宇宙惑星科学

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