{"id":1044,"date":"2025-05-23T08:43:35","date_gmt":"2025-05-23T08:43:35","guid":{"rendered":"https:\/\/pages.lip.pt\/pheno\/?p=1044"},"modified":"2025-05-23T16:08:17","modified_gmt":"2025-05-23T16:08:17","slug":"the-dawn-of-gravitational-wave-cosmology-workshop","status":"publish","type":"post","link":"https:\/\/pages.lip.pt\/pheno\/uncategorized\/the-dawn-of-gravitational-wave-cosmology-workshop\/","title":{"rendered":"The Dawn of Gravitational Wave Cosmology (workshop)"},"content":{"rendered":"\n<p style=\"font-size:15px\">The upcoming era of gravitational wave (GW) cosmology, enabled by a broad range of next-generation detectors, demands a coordinated theoretical effort and a robust theory-to-data pipeline to fully exploit its discovery potential. The workshop <strong>&#8220;The Dawn of Gravitational Wave Cosmology&#8221;<\/strong>, held at <strong>Benasque<\/strong> (Spain) <strong>from April 27th to May 17th<\/strong>, brought together experts across diverse GW probes to develop a multi-messenger strategy, with a key focus on cross-correlations to disentangle primordial signals from astrophysical backgrounds.<\/p>\n\n\n\n<p class=\"has-background\" style=\"background-color:#8dd2fc4d;font-size:15px\">The workshop featured a contribution of the LIP-Phenomenology member Marco Finetti. He presented PT2GWFinder, a Mathematica-based tool developed to streamline the analysis of first-order cosmological phase transitions and their associated gravitational wave signals within Beyond the Standard Model (BSM) scenarios.<\/p>\n\n\n\n<p>PT2GWFinder simplifies the computation of key phase transition parameters\u2014such as nucleation and percolation temperatures\u2014by automating tasks like phase tracing, bounce action fitting, and gravitational wave spectrum derivation, using the polygonal bounce method via FindBounce. It also emphasizes user-friendliness and full automation while maintaining compatibility with dimensional reduction frameworks like DRalgo.<\/p>\n\n\n<div class=\"wp-block-image\">\n<figure class=\"aligncenter size-full\"><img fetchpriority=\"high\" decoding=\"async\" width=\"1008\" height=\"498\" src=\"https:\/\/pages.lip.pt\/pheno\/wp-content\/uploads\/sites\/29\/2025\/05\/well.001.jpeg\" alt=\"\" class=\"wp-image-1046\" srcset=\"https:\/\/pages.lip.pt\/pheno\/wp-content\/uploads\/sites\/29\/2025\/05\/well.001.jpeg 1008w, https:\/\/pages.lip.pt\/pheno\/wp-content\/uploads\/sites\/29\/2025\/05\/well.001-300x148.jpeg 300w, https:\/\/pages.lip.pt\/pheno\/wp-content\/uploads\/sites\/29\/2025\/05\/well.001-768x379.jpeg 768w\" sizes=\"(max-width: 767px) 89vw, (max-width: 1000px) 54vw, (max-width: 1071px) 543px, 580px\" \/><\/figure>\n<\/div>\n\n\n<p>For more information, see <a href=\"https:\/\/benasque.org\/2025gwc\/\">https:\/\/benasque.org\/2025gwc\/<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>The upcoming era of gravitational wave (GW) cosmology, enabled by a broad range of next-generation detectors, demands a coordinated theoretical effort and a robust theory-to-data pipeline to fully exploit its discovery potential. The workshop &#8220;The Dawn of Gravitational Wave Cosmology&#8221;, held at Benasque (Spain) from April 27th to May 17th, brought together experts across diverse &hellip; <\/p>\n<p class=\"link-more\"><a href=\"https:\/\/pages.lip.pt\/pheno\/uncategorized\/the-dawn-of-gravitational-wave-cosmology-workshop\/\" class=\"more-link\">Continue reading<span class=\"screen-reader-text\"> &#8220;The Dawn of Gravitational Wave Cosmology (workshop)&#8221;<\/span><\/a><\/p>\n","protected":false},"author":33,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[1],"tags":[],"class_list":["post-1044","post","type-post","status-publish","format-standard","hentry","category-uncategorized"],"_links":{"self":[{"href":"https:\/\/pages.lip.pt\/pheno\/wp-json\/wp\/v2\/posts\/1044","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/pages.lip.pt\/pheno\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/pages.lip.pt\/pheno\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/pages.lip.pt\/pheno\/wp-json\/wp\/v2\/users\/33"}],"replies":[{"embeddable":true,"href":"https:\/\/pages.lip.pt\/pheno\/wp-json\/wp\/v2\/comments?post=1044"}],"version-history":[{"count":4,"href":"https:\/\/pages.lip.pt\/pheno\/wp-json\/wp\/v2\/posts\/1044\/revisions"}],"predecessor-version":[{"id":1063,"href":"https:\/\/pages.lip.pt\/pheno\/wp-json\/wp\/v2\/posts\/1044\/revisions\/1063"}],"wp:attachment":[{"href":"https:\/\/pages.lip.pt\/pheno\/wp-json\/wp\/v2\/media?parent=1044"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/pages.lip.pt\/pheno\/wp-json\/wp\/v2\/categories?post=1044"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/pages.lip.pt\/pheno\/wp-json\/wp\/v2\/tags?post=1044"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}