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Monte Carlo study on distortion of the space-dimension in COBE monopole data
http://hdl.handle.net/10091/17854
http://hdl.handle.net/10091/1785467b4d381-5e38-4168-a3e0-23b86ae8f1ec
名前 / ファイル | ライセンス | アクション |
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Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2014-09-05 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Monte Carlo study on distortion of the space-dimension in COBE monopole data | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | Cosmic background radiation | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | Cosmological parameters | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | Space-dimension | |||||
資源タイプ | ||||||
資源 | http://purl.org/coar/resource_type/c_6501 | |||||
タイプ | journal article | |||||
著者 |
Biyajima, Minoru
× Biyajima, Minoru× Mizoguchi, Takuya |
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信州大学研究者総覧へのリンク | ||||||
氏名 | Biyajima, Minoru | |||||
URL | http://soar-rd.shinshu-u.ac.jp/profile/ja.ZaDNOeyC.html | |||||
出版者 | ||||||
出版者 | SPRINGER | |||||
引用 | ||||||
内容記述タイプ | Other | |||||
内容記述 | ASTROPHYSICS AND SPACE SCIENCE. 350(1):317-323 (2014) | |||||
書誌情報 |
ASTROPHYSICS AND SPACE SCIENCE 巻 350, 号 1, p. 317-323, 発行日 2014-03 |
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内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | Published online: 5 December 2013 | |||||
抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | A concise explanation of studies on distortion of space-time dimension is briefly introduced. Second we obtain the limits (i.e., bounded values) of the dimensionless chemical potential mu, the Sunyaev-Zeldovich (SZ) effect y and distortion of the space-dimension epsilon by Monte Carlo (MC) analysis of the parameter set (T, d=3+epsilon, mu, and y) in cosmic microwave data assuming that the SZ effect is positive (y > 0). In this analysis, the magnitude of the space-dimension d with distortion of the space-dimension epsilon is defined by d=3+epsilon. The limits of mu and y are determined as |mu|< 9x10(-5) (2 sigma) (mu=(-3.9 +/- 2.6)x10(-5) (sigma)), |y|< 5x10(-6) (2 sigma) (y=(2.0 +/- 1.4)x10(-6) (sigma)), while the distortion of the space-dimension is |epsilon|< 6x10(-5) (2 sigma) (epsilon=(-0.78 +/- 2.50)x10(-5) (sigma)). The magnitudes of these three estimated limits are ordered as . The estimated limit of |y|< 5x10(-6) appears to be related to re-ionization processes occurring at redshift z (ri similar to)10. We also present data analysis assuming a relativistic SZ effect. | |||||
資源タイプ(コンテンツの種類) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Article | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 0004-640X | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA00553333 | |||||
DOI | ||||||
識別子タイプ | DOI | |||||
関連識別子 | https://doi.org/10.1007/s10509-013-1717-6 | |||||
関連名称 | 10.1007/s10509-013-1717-6 | |||||
権利 | ||||||
権利情報 | The final publication is available at link.springer.com | |||||
出版タイプ | ||||||
出版タイプ | AM | |||||
出版タイプResource | http://purl.org/coar/version/c_ab4af688f83e57aa | |||||
WoS | ||||||
表示名 | Web of Science | |||||
URL | http://gateway.isiknowledge.com/gateway/Gateway.cgi?&GWVersion=2&SrcAuth=ShinshuUniv&SrcApp=ShinshuUniv&DestLinkType=FullRecord&DestApp=WOS&KeyUT=000332662800035 |