Observational constraints on quintessence: Thawing, tracker, and scaling models

Takeshi Chiba*, Antonio De Felice, Shinji Tsujikawa

*この研究の対応する著者

研究成果: Article査読

67 被引用数 (Scopus)

抄録

For two types of quintessence models having thawing and tracking properties, there exist analytic solutions for the dark energy equation of state w expressed in terms of several free parameters. We put observational bounds on the parameters in such scenarios by using the recent type Ia supernovae, cosmic microwave background, and baryon acoustic oscillations data. The observational constraints are quite different depending on whether or not the recent baryon acoustic oscillations data from BOSS are taken into account. With the BOSS data the upper bounds of today's values of w (=w0) in thawing models is very close to -1, whereas without this data the values of w0 away from -1 can still be allowed. The tracker equation of state w(0) during the matter era is constrained to be w(0)<-0.949 at 95% C.L. even without the BOSS data, so that the tracker models with w away from -1 are severely disfavored. We also study observational constraints on scaling models in which w starts to evolve from 0 in the deep matter era and show that the transition to the equation of state close to w=-1 needs to occur at an early cosmological epoch. In the three classes of quintessence models studied in this paper, the past evolution of the Hubble parameters in the best-fit models shows only less than a 2.5% difference compared to ΛCDM.

本文言語English
論文番号083505
ジャーナルPhysical Review D - Particles, Fields, Gravitation and Cosmology
87
8
DOI
出版ステータスPublished - 2013 4月 3
外部発表はい

ASJC Scopus subject areas

  • 核物理学および高エネルギー物理学
  • 物理学および天文学(その他)

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