{"id":4609,"date":"2023-07-11T12:58:08","date_gmt":"2023-07-11T07:28:08","guid":{"rendered":"https:\/\/www.isical.ac.in\/~pamu\/?post_type=highlight&#038;p=4609"},"modified":"2024-04-12T15:54:04","modified_gmt":"2024-04-12T10:24:04","slug":"imprints-of-dark-matter-massive-neutrino-interaction-in-upcoming-post-reionization-and-galaxy-surveys","status":"publish","type":"highlight","link":"https:\/\/oldweb.isical.ac.in\/~pamu\/highlight\/imprints-of-dark-matter-massive-neutrino-interaction-in-upcoming-post-reionization-and-galaxy-surveys\/","title":{"rendered":"Imprints of dark matter-massive neutrino interaction in upcoming post-reionization and galaxy surveys"},"content":{"rendered":"<p>We explore possible signatures of the interaction between dark matter and massive neutrinos in\u00a0the upcoming post-reionization and galaxy surveys:\u00a0Square Kilometre Array (SKA1 and SKA2) and Euclid.\u00a0All these missions show promise in constraining the interaction parameter and total neutrino mass by a few orders compared to the existing\u00a0constraints from Planck telescope,\u00a0SKA2 performing the best among them.\u00a0We further perform a brief investigation of the prospects of some of the next generation Cosmic Microwave Background (CMB) missions in combinations with LSS experiments in improving the constraints. Our analysis reveals that both SKA2 and CMB-S4 + Euclid + SKA1 IM2 combination will put the strongest bounds on the model parameters.<\/p>\n<p>Reference:\u00a0<a href=\"https:\/\/arxiv.org\/abs\/2307.00606\" target=\"_blank\" rel=\"noopener noreferrer\">https:\/\/arxiv.org\/abs\/2307.00606<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>We explore possible signatures of the interaction between dark matter and massive neutrinos in\u00a0the upcoming post-reionization and galaxy surveys:\u00a0Square Kilometre Array (SKA1 and SKA2) and Euclid.<\/p>\n","protected":false},"featured_media":4613,"template":"","categories":[111],"tags":[],"acf":[],"_links":{"self":[{"href":"https:\/\/oldweb.isical.ac.in\/~pamu\/wp-json\/wp\/v2\/highlight\/4609"}],"collection":[{"href":"https:\/\/oldweb.isical.ac.in\/~pamu\/wp-json\/wp\/v2\/highlight"}],"about":[{"href":"https:\/\/oldweb.isical.ac.in\/~pamu\/wp-json\/wp\/v2\/types\/highlight"}],"version-history":[{"count":1,"href":"https:\/\/oldweb.isical.ac.in\/~pamu\/wp-json\/wp\/v2\/highlight\/4609\/revisions"}],"predecessor-version":[{"id":4611,"href":"https:\/\/oldweb.isical.ac.in\/~pamu\/wp-json\/wp\/v2\/highlight\/4609\/revisions\/4611"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/oldweb.isical.ac.in\/~pamu\/wp-json\/wp\/v2\/media\/4613"}],"wp:attachment":[{"href":"https:\/\/oldweb.isical.ac.in\/~pamu\/wp-json\/wp\/v2\/media?parent=4609"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/oldweb.isical.ac.in\/~pamu\/wp-json\/wp\/v2\/categories?post=4609"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/oldweb.isical.ac.in\/~pamu\/wp-json\/wp\/v2\/tags?post=4609"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}