{"created":"2023-07-27T06:26:38.643216+00:00","id":10447,"links":{},"metadata":{"_buckets":{"deposit":"6daf43ea-eca0-461c-b1b1-715c854ab238"},"_deposit":{"created_by":3,"id":"10447","owners":[3],"pid":{"revision_id":0,"type":"depid","value":"10447"},"status":"published"},"_oai":{"id":"oai:kanazawa-u.repo.nii.ac.jp:00010447","sets":["934:935:937"]},"author_link":["15839","15840","15841"],"item_4_biblio_info_8":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2011-01-01","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"7","bibliographicPageStart":"026","bibliographicVolumeNumber":"2011","bibliographic_titles":[{"bibliographic_title":"Journal of High Energy Physics"}]}]},"item_4_description_21":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"We show that the lightest right-handed sneutrino in TeV scale supersymmetric B - L model with inverse seesaw mechanism is a viable candidate for cold dark matter. We find that it accounts for the observed dark matter relic abundance in a wide range of parameter space. The spin-independent cross section of B - L right-handed sneutrino is consistent with the recent results CDMS II and XENON experiments and it is detectable in future direct detection experiments. Although the B-L right-handed sneutrinos annihilate into leptons, the PAMELA results can not be explained in this model unless a huge boost factor is considered. Also the muon flux generated by B -L right-handed sneutrino in the galactic center is smaller than Super-Kamiokande's upper bound. © SISSA 2011.","subitem_description_type":"Abstract"}]},"item_4_publisher_17":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"Springer Verlag / SISSA"}]},"item_4_relation_12":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_type":"isVersionOf","subitem_relation_type_id":{"subitem_relation_type_id_text":"10.1007/JHEP07(2011)026","subitem_relation_type_select":"DOI"}}]},"item_4_relation_28":{"attribute_name":"関連URI","attribute_value_mlt":[{"subitem_relation_type_id":{"subitem_relation_type_id_text":"http://iopscience.iop.org/1126-6708","subitem_relation_type_select":"URI"}},{"subitem_relation_type_id":{"subitem_relation_type_id_text":"http://www.springerlink.com/content/nr238wj318r37496/","subitem_relation_type_select":"URI"}}]},"item_4_source_id_11":{"attribute_name":"NCID","attribute_value_mlt":[{"subitem_source_identifier":"AA11380940","subitem_source_identifier_type":"NCID"}]},"item_4_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"1126-6708","subitem_source_identifier_type":"ISSN"}]},"item_4_version_type_25":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_version_resource":"http://purl.org/coar/version/c_ab4af688f83e57aa","subitem_version_type":"AM"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Khalil, Shaaban"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Okada, Hiroshi"}],"nameIdentifiers":[{},{}]},{"creatorNames":[{"creatorName":"Toma, Takashi"}],"nameIdentifiers":[{}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2017-10-03"}],"displaytype":"detail","filename":"SC-PR-TOMA-T-026.pdf","filesize":[{"value":"1.3 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"SC-PR-TOMA-T-026.pdf","url":"https://kanazawa-u.repo.nii.ac.jp/record/10447/files/SC-PR-TOMA-T-026.pdf"},"version_id":"8321924a-eb9c-4241-ac87-7cea16dd9050"}]},"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":"Right-handed sneutrino dark matter in supersymmetric B - L model","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Right-handed sneutrino dark matter in supersymmetric B - L model"}]},"item_type_id":"4","owner":"3","path":["937"],"pubdate":{"attribute_name":"公開日","attribute_value":"2017-10-03"},"publish_date":"2017-10-03","publish_status":"0","recid":"10447","relation_version_is_last":true,"title":["Right-handed sneutrino dark matter in supersymmetric B - L model"],"weko_creator_id":"3","weko_shared_id":-1},"updated":"2023-07-28T01:40:37.352154+00:00"}