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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 \u003e 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|\u003c 9x10(-5) (2 sigma) (mu=(-3.9 +/- 2.6)x10(-5) (sigma)), |y|\u003c 5x10(-6) (2 sigma) (y=(2.0 +/- 1.4)x10(-6) (sigma)), while the distortion of the space-dimension is |epsilon|\u003c 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|\u003c 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": "\u8cc7\u6e90\u30bf\u30a4\u30d7\uff08\u30b3\u30f3\u30c6\u30f3\u30c4\u306e\u7a2e\u985e\uff09", "attribute_value_mlt": [{"subitem_description": "Article", "subitem_description_type": "Other"}]}, "item_6_description_5": {"attribute_name": "\u5f15\u7528", "attribute_value_mlt": [{"subitem_description": "ASTROPHYSICS AND SPACE SCIENCE. 350(1):317-323 (2014)", "subitem_description_type": "Other"}]}, "item_6_link_3": {"attribute_name": "\u4fe1\u5dde\u5927\u5b66\u7814\u7a76\u8005\u7dcf\u89a7\u3078\u306e\u30ea\u30f3\u30af", "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_text": "Web of Science", "subitem_link_url": "http://gateway.isiknowledge.com/gateway/Gateway.cgi?\u0026GWVersion=2\u0026SrcAuth=ShinshuUniv\u0026SrcApp=ShinshuUniv\u0026DestLinkType=FullRecord\u0026DestApp=WOS\u0026KeyUT=000332662800035"}]}, "item_6_publisher_4": {"attribute_name": "\u51fa\u7248\u8005", "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": "\u6a29\u5229", "attribute_value_mlt": [{"subitem_rights": "The final publication is available at link.springer.com"}]}, "item_6_select_64": {"attribute_name": "\u8457\u8005\u7248\u30d5\u30e9\u30b0", "attribute_value_mlt": [{"subitem_select_item": "author"}]}, "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_39": {"attribute_name": "NII ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "0004-640X", "subitem_source_identifier_type": "ISSN"}]}, "item_6_source_id_40": {"attribute_name": "\u66f8\u8a8c\u30ec\u30b3\u30fc\u30c9ID", "attribute_value_mlt": [{"subitem_source_identifier": "AA00553333", "subitem_source_identifier_type": "NCID"}]}, "item_6_text_69": {"attribute_name": "wosonly authkey", "attribute_value_mlt": [{"subitem_text_value": "Cosmic background radiation; Cosmological parameters; Space-dimension"}]}, "item_6_text_70": {"attribute_name": "wosonly keywords", "attribute_value_mlt": [{"subitem_text_value": "MICROWAVE BACKGROUND SPECTRUM; RELATIVISTIC CORRECTIONS; HOT-MODEL; RADIATION; TIME; RENORMALIZATION; REGULARIZATION; INSTRUMENT; UNIVERSE; MATTER"}]}, "item_6_textarea_68": {"attribute_name": "wosonly abstract", "attribute_value_mlt": [{"subitem_textarea_value": "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 \u003e 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|\u003c 9x10(-5) (2 sigma) (mu=(-3.9 +/- 2.6)x10(-5) (sigma)), |y|\u003c 5x10(-6) (2 sigma) (y=(2.0 +/- 1.4)x10(-6) (sigma)), while the distortion of the space-dimension is |epsilon|\u003c 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|\u003c 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."}]}, "item_creator": {"attribute_name": "\u8457\u8005", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "Biyajima,  Minoru"}], "nameIdentifiers": [{"nameIdentifier": "35935", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Mizoguchi,  Takuya"}], "nameIdentifiers": [{"nameIdentifier": "35936", "nameIdentifierScheme": "WEKO"}]}]}, "item_files": {"attribute_name": "\u30d5\u30a1\u30a4\u30eb\u60c5\u5831", "attribute_type": "file", "attribute_value_mlt": [{"accessrole": "open_date", "date": [{"dateType": "Available", "dateValue": "2015-09-28"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "Monte_Carlo_study_distortion.pdf", "filesize": [{"value": "338.6 kB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_note", "mimetype": "application/pdf", "size": 338600.0, "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": "\u30ad\u30fc\u30ef\u30fc\u30c9", "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": "\u8a00\u8a9e", "attribute_value_mlt": [{"subitem_language": "eng"}]}, "item_resource_type": {"attribute_name": "\u8cc7\u6e90\u30bf\u30a4\u30d7", "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": "\u30bf\u30a4\u30c8\u30eb", "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": ["1169/1170"], "permalink_uri": "http://hdl.handle.net/10091/17854", "pubdate": {"attribute_name": "PubDate", "attribute_value": "2014-09-05"}, "publish_date": "2014-09-05", "publish_status": "0", "recid": "11726", "relation": {}, "relation_version_is_last": true, "title": ["Monte Carlo study on distortion of the space-dimension in COBE monopole data"], "weko_shared_id": -1}