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  1. 010 学術雑誌論文
  2. 池内, 了 / IKEUCHI, Satoru

Quasar absorption lines with a nonzero cosmological constant

https://ir.soken.ac.jp/records/3502
https://ir.soken.ac.jp/records/3502
efe9083b-7710-4d90-8461-d990e72e0ed6
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Item type 学術雑誌論文 / Journal Article(1)
公開日 2013-04-23
タイトル
タイトル Quasar absorption lines with a nonzero cosmological constant
タイトル
タイトル Quasar absorption lines with a nonzero cosmological constant
言語 en
言語
言語 eng
資源タイプ
資源タイプ識別子 http://purl.org/coar/resource_type/c_6501
資源タイプ journal article
著者 TURNER, Edwin L

× TURNER, Edwin L

TURNER, Edwin L

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IKEUCHI, Satoru

× IKEUCHI, Satoru

IKEUCHI, Satoru

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著者別名 池内 , 了

× 池内 , 了

池内 , 了

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抄録
内容記述タイプ Abstract
内容記述 Flat but nonzero cosmological constant model universes contain substantially larger comoving volumes and path lengths within a given redshift than more conventional zero Λ ones. They also change the nature of their expansion at a characteristic critical redshift z c = (λ 0/Ω 0) 1/3, whereas zero Λ flat models show a smooth power-law expansion at all epochs. Both of these physical differences can affect intergalactic absorption and scattering processes. The former simply implies more absorption for a given fixed population of absorbers or, conversely, requires fewer absorbers to explain a given observed amount of absorption. The latter manifests itself as a break in the number of absorbers per unit redshift at about z c and gives rise to a quite different redshift dependence of the number of absorbers at z < z c. Thus, there is an interesting interaction between Λ effects and cosmic absorption phenomena which are explored in this paper. For example, the absolute frequency of metal and high column density H I absorption at high redshift is significantly closer to that expected from the properties of low-redshift galaxies in Λ-dominated cosmologies than in conventional ones. The equations describing IGM absorption statistics are developed for nonzero Λ cosmologies, both for unevolving absorber populations and including the effects of the expected absorber evolution in some of the more popular physical models for the IGM and intergalactic clouds. These results are compared to observations for the cases of Lyman-α forest lines, damped Lyman-α lines, Lyman limit systems, C IV 1549 Å lines, Mg II 2800 Å lines, diffuse H I absorption (Gunn-Peterson effect), and the Compton y-parameter. Cosmological models with (Ω 0, λ 0) of (1, 0) and (0.1, 0.9) are contrasted. In general, the available data are consistent with both models, but the (0.1, 0.9) model extrapolates to much less absorption at low redshift and requires less evolution with redshift than the (1, 0) model. Hubble Space Telescope and ASTRO space UV spectroscopy of low-redshift absorption lines should allow a fairly direct test of Λ. The Mg II absorption line data currently extend to fairly low redshifts and allow the best Λ discrimination available with present data; the (0.1, 0.9) model gives a beter fit to the Mg II observations, but the size of the statistical errors is such that the (1, 0) model is not excluded with great significance. It is also found that the available Gunn-Peterson effect and Compton y-parameter limits are somewhat more difficult to satisfy in the (0.1, 0.9) model than in the (1, 0) one.
書誌情報 Astrophysics and Space Science
en : Astrophysics and Space Science

巻 389, 号 2, p. 478-490, 発行日 1992-04
出版者
出版者 The American Astronomical Society
ISSN
収録物識別子タイプ ISSN
収録物識別子 20418205
DOI
関連タイプ isIdenticalTo
識別子タイプ DOI
関連識別子 http://doi.org/10.1086/171224
関連名称 10.1086/171224
権利
権利情報 © 1992. The American Astronomical Society
関連サイト
識別子タイプ URI
関連識別子 http://aas.org/publications/aas-copyright-policy
関連名称 Copyright
フォーマット
内容記述タイプ Other
内容記述 application/pdf
著者版フラグ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
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