{"created":"2021-03-01T06:14:37.450046+00:00","id":11726,"links":{},"metadata":{"_buckets":{"deposit":"ba97b6fe-41ba-44af-a738-ad3ec7969555"},"_deposit":{"id":"11726","owners":[],"pid":{"revision_id":0,"type":"depid","value":"11726"},"status":"published"},"_oai":{"id":"oai:soar-ir.repo.nii.ac.jp:00011726","sets":["1169:1170"]},"author_link":["35935","35936"],"item_1628147817048":{"attribute_name":"出版タイプ","attribute_value_mlt":[{"subitem_version_resource":"http://purl.org/coar/version/c_ab4af688f83e57aa","subitem_version_type":"AM"}]},"item_6_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2014-03","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"1","bibliographicPageEnd":"323","bibliographicPageStart":"317","bibliographicVolumeNumber":"350","bibliographic_titles":[{"bibliographic_title":"ASTROPHYSICS AND SPACE SCIENCE"}]}]},"item_6_description_19":{"attribute_name":"内容記述","attribute_value_mlt":[{"subitem_description":"Published online: 5 December 2013","subitem_description_type":"Other"}]},"item_6_description_20":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"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.","subitem_description_type":"Abstract"}]},"item_6_description_30":{"attribute_name":"資源タイプ（コンテンツの種類）","attribute_value_mlt":[{"subitem_description":"Article","subitem_description_type":"Other"}]},"item_6_description_5":{"attribute_name":"引用","attribute_value_mlt":[{"subitem_description":"ASTROPHYSICS AND SPACE SCIENCE. 350(1):317-323 (2014)","subitem_description_type":"Other"}]},"item_6_link_3":{"attribute_name":"信州大学研究者総覧へのリンク","attribute_value_mlt":[{"subitem_link_text":"Biyajima, Minoru","subitem_link_url":"http://soar-rd.shinshu-u.ac.jp/profile/ja.ZaDNOeyC.html"}]},"item_6_link_67":{"attribute_name":"WoS","attribute_value_mlt":[{"subitem_link_url":"http://gateway.isiknowledge.com/gateway/Gateway.cgi?&GWVersion=2&SrcAuth=ShinshuUniv&SrcApp=ShinshuUniv&DestLinkType=FullRecord&DestApp=WOS&KeyUT=000332662800035"}]},"item_6_publisher_4":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"SPRINGER"}]},"item_6_relation_48":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"10.1007/s10509-013-1717-6"}],"subitem_relation_type_id":{"subitem_relation_type_id_text":"https://doi.org/10.1007/s10509-013-1717-6","subitem_relation_type_select":"DOI"}}]},"item_6_rights_62":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"The final publication is available at link.springer.com"}]},"item_6_source_id_35":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0004-640X","subitem_source_identifier_type":"ISSN"}]},"item_6_source_id_40":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA00553333","subitem_source_identifier_type":"NCID"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Biyajima,  Minoru"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Mizoguchi,  Takuya"}],"nameIdentifiers":[{}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2015-09-28"}],"displaytype":"detail","filename":"Monte_Carlo_study_distortion.pdf","filesize":[{"value":"338.6 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"Monte_Carlo_study_distortion.pdf","url":"https://soar-ir.repo.nii.ac.jp/record/11726/files/Monte_Carlo_study_distortion.pdf"},"version_id":"c1e23bb4-0590-437d-84b6-5f5b6e77dd02"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"Cosmic background radiation","subitem_subject_scheme":"Other"},{"subitem_subject":"Cosmological parameters","subitem_subject_scheme":"Other"},{"subitem_subject":"Space-dimension","subitem_subject_scheme":"Other"}]},"item_language":{"attribute_name":"言語","attribute_value_mlt":[{"subitem_language":"eng"}]},"item_resource_type":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"resourcetype":"journal article","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Monte Carlo study on distortion of the space-dimension in COBE monopole data","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Monte Carlo study on distortion of the space-dimension in COBE monopole data","subitem_title_language":"en"}]},"item_type_id":"6","owner":"1","path":["1170"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2014-09-05"},"publish_date":"2014-09-05","publish_status":"0","recid":"11726","relation_version_is_last":true,"title":["Monte Carlo study on distortion of the space-dimension in COBE monopole data"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2022-12-14T04:38:51.835032+00:00"}