{"created":"2023-06-20T13:23:24.410120+00:00","id":4251,"links":{},"metadata":{"_buckets":{"deposit":"9ad988b7-412b-49fd-b580-11b52f210051"},"_deposit":{"created_by":21,"id":"4251","owners":[21],"pid":{"revision_id":0,"type":"depid","value":"4251"},"status":"published"},"_oai":{"id":"oai:ir.soken.ac.jp:00004251","sets":["1:274"]},"author_link":["734","737","738"],"item_10001_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1984","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"2","bibliographicPageEnd":"232","bibliographicPageStart":"216","bibliographicVolumeNumber":"72","bibliographic_titles":[{"bibliographic_title":"Progress of Theoretical Physics"},{"bibliographic_title":"Progress of Theoretical Physics","bibliographic_titleLang":"en"}]}]},"item_10001_creator_3":{"attribute_name":"著者別名","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"池内, 了"}],"nameIdentifiers":[{"nameIdentifier":"738","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"1000090025461","nameIdentifierScheme":"NRID","nameIdentifierURI":" "},{"nameIdentifier":"90025461","nameIdentifierScheme":"e-Rad","nameIdentifierURI":"https://kaken.nii.ac.jp/ja/search/?qm=90025461"}]}]},"item_10001_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"The growth of density contrasts of collisionless particles and nucleonic matter is pursued from the decoupling era up to the present in the Newtonian mechanics. The negative density perturbation of collisionles particles grows quickly to the void and surrounding ridge. Meanwhile, the shell-crossing occurs. The nucleonic matter, which is set uniformly at the decoupling epoch, is enforced to concentrate into the ridge by the gravitational force at this shell-crossing epoch. At the same time, the temperature of nucleonic matter increases rapidly due to the dissipation of kinetic energy by the pressure force. The dependence of results upon the amplitude of the initial density perturbation is made clear. If the galaxies were formed after the shell-crossing, the initial amplitude of density perturbation of collisionless particles must be higher than 0.03 in the Einstein-de Sitter universe. Through the analysis of gravitational instability of ridges, a possible scenario for the formation of the large-scale structure of the universe within the adiabatic theory is presented. ","subitem_description_type":"Abstract"}]},"item_10001_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"Oxford University Press "}]},"item_10001_relation_14":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"10.1143/PTP.72.216 "}],"subitem_relation_type_id":{"subitem_relation_type_id_text":"https://doi.org/10.1143/PTP.72.216","subitem_relation_type_select":"DOI"}}]},"item_10001_rights_15":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"©  2014  The Physical Society of Japan "}]},"item_10001_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0033-068X","subitem_source_identifier_type":"ISSN"}]},"item_access_right":{"attribute_name":"アクセス権","attribute_value_mlt":[{"subitem_access_right":"metadata only access","subitem_access_right_uri":"http://purl.org/coar/access_right/c_14cb"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"IKEUCHI, Satoru"}],"nameIdentifiers":[{"nameIdentifier":"734","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"UMEMURA, Masayuki"}],"nameIdentifiers":[{"nameIdentifier":"737","nameIdentifierScheme":"WEKO"}]}]},"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":"Nonlinear Growth of Density Contrast and Formation of Galaxies in a Neutrino-Dominated Universe","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Nonlinear Growth of Density Contrast and Formation of Galaxies in a Neutrino-Dominated Universe"},{"subitem_title":"Nonlinear Growth of Density Contrast and Formation of Galaxies in a Neutrino-Dominated Universe","subitem_title_language":"en"}]},"item_type_id":"10001","owner":"21","path":["274"],"pubdate":{"attribute_name":"公開日","attribute_value":"2014-02-18"},"publish_date":"2014-02-18","publish_status":"0","recid":"4251","relation_version_is_last":true,"title":["Nonlinear Growth of Density Contrast and Formation of Galaxies in a Neutrino-Dominated Universe"],"weko_creator_id":"21","weko_shared_id":21},"updated":"2023-06-20T14:26:25.216134+00:00"}