{"id":1633,"date":"2022-04-06T07:06:46","date_gmt":"2022-04-06T11:06:46","guid":{"rendered":"https:\/\/web.uri.edu\/gravity\/?p=1633"},"modified":"2023-01-03T11:16:02","modified_gmt":"2023-01-03T16:16:02","slug":"tousifs-paper-on-our-much-improved-surrogate","status":"publish","type":"post","link":"https:\/\/web.uri.edu\/gravity\/tousifs-paper-on-our-much-improved-surrogate\/","title":{"rendered":"Tousif&#8217;s paper on our much improved surrogate"},"content":{"rendered":"\n<p>Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity<\/p>\n\n\n\n<p><a href=\"https:\/\/arxiv.org\/search\/gr-qc?searchtype=author&amp;query=Islam%2C+T\">Tousif Islam<\/a>,&nbsp;<a href=\"https:\/\/arxiv.org\/search\/gr-qc?searchtype=author&amp;query=Field%2C+S+E\">Scott E. Field<\/a>,&nbsp;<a href=\"https:\/\/arxiv.org\/search\/gr-qc?searchtype=author&amp;query=Hughes%2C+S+A\">Scott A. Hughes<\/a>,&nbsp;<a href=\"https:\/\/arxiv.org\/search\/gr-qc?searchtype=author&amp;query=Khanna%2C+G\">Gaurav Khanna<\/a>,&nbsp;<a href=\"https:\/\/arxiv.org\/search\/gr-qc?searchtype=author&amp;query=Varma%2C+V\">Vijay Varma<\/a>,&nbsp;<a href=\"https:\/\/arxiv.org\/search\/gr-qc?searchtype=author&amp;query=Giesler%2C+M\">Matthew Giesler<\/a>,&nbsp;<a href=\"https:\/\/arxiv.org\/search\/gr-qc?searchtype=author&amp;query=Scheel%2C+M+A\">Mark A. Scheel<\/a>,&nbsp;<a href=\"https:\/\/arxiv.org\/search\/gr-qc?searchtype=author&amp;query=Kidder%2C+L+E\">Lawrence E. Kidder<\/a>,&nbsp;<a href=\"https:\/\/arxiv.org\/search\/gr-qc?searchtype=author&amp;query=Pfeiffer%2C+H+P\">Harald P. Pfeiffer<\/a><\/p>\n\n\n\n<p><a href=\"https:\/\/arxiv.org\/abs\/2204.01972\">Phys. Rev. D 106, 104025 (2022)<\/a> [Editor&#8217;s Suggestion]<\/p>\n\n\n\n<p><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity Tousif Islam,&nbsp;Scott E. Field,&nbsp;Scott A. Hughes,&nbsp;Gaurav Khanna,&nbsp;Vijay Varma,&nbsp;Matthew Giesler,&nbsp;Mark A. Scheel,&nbsp;Lawrence E. Kidder,&nbsp;Harald P. Pfeiffer Phys. Rev. D 106, 104025 (2022) [Editor&#8217;s Suggestion]<\/p>\n","protected":false},"author":4052,"featured_media":514,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"footnotes":"","_links_to":"","_links_to_target":""},"categories":[5],"tags":[],"class_list":["post-1633","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-publications"],"acf":[],"_links":{"self":[{"href":"https:\/\/web.uri.edu\/gravity\/wp-json\/wp\/v2\/posts\/1633","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/web.uri.edu\/gravity\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/web.uri.edu\/gravity\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/web.uri.edu\/gravity\/wp-json\/wp\/v2\/users\/4052"}],"replies":[{"embeddable":true,"href":"https:\/\/web.uri.edu\/gravity\/wp-json\/wp\/v2\/comments?post=1633"}],"version-history":[{"count":4,"href":"https:\/\/web.uri.edu\/gravity\/wp-json\/wp\/v2\/posts\/1633\/revisions"}],"predecessor-version":[{"id":1817,"href":"https:\/\/web.uri.edu\/gravity\/wp-json\/wp\/v2\/posts\/1633\/revisions\/1817"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/web.uri.edu\/gravity\/wp-json\/wp\/v2\/media\/514"}],"wp:attachment":[{"href":"https:\/\/web.uri.edu\/gravity\/wp-json\/wp\/v2\/media?parent=1633"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/web.uri.edu\/gravity\/wp-json\/wp\/v2\/categories?post=1633"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/web.uri.edu\/gravity\/wp-json\/wp\/v2\/tags?post=1633"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}