{"id":2157,"date":"2025-06-06T09:46:29","date_gmt":"2025-06-06T09:46:29","guid":{"rendered":"https:\/\/darkwave.astrocent.pl\/?p=2157"},"modified":"2025-06-12T09:48:21","modified_gmt":"2025-06-12T09:48:21","slug":"astrocent-at-the-darkside-20k-summer-collaboration-meeting","status":"publish","type":"post","link":"https:\/\/darkwave.astrocent.pl\/index.php\/2025\/06\/06\/astrocent-at-the-darkside-20k-summer-collaboration-meeting\/","title":{"rendered":"Astrocent at the DarkSide-20k Summer Collaboration Meeting"},"content":{"rendered":"<p>Views: 9<\/p>\n<p>From 2\u20136 June 2025, the Astrocent team participated in the DarkSide-20k summer collaboration meeting, held in Geremeas, Sardinia. This annual gathering brought together researchers and engineers from institutions around the world to discuss progress, challenges, and plans for the DarkSide-20k experiment \u2014 one of the most advanced dark matter search projects currently underway.<\/p>\n\n\n\n<p>Astrocent is a contributor to the DarkSide-20k collaboration, with many of our team members actively involved in the design and development of the experiment\u2019s cutting-edge technologies. These include low-background electronics, ultra-sensitive photodetectors, data acquisition systems, and other components essential for identifying extremely rare signals from potential dark matter interactions.<\/p>\n\n\n\n<figure class=\"wp-block-image size-large\"><img fetchpriority=\"high\" decoding=\"async\" width=\"1024\" height=\"784\" src=\"https:\/\/darkwave.astrocent.pl\/wp-content\/uploads\/2025\/06\/20250603_140647-1024x784.jpg\" alt=\"\" class=\"wp-image-2158\" srcset=\"https:\/\/darkwave.astrocent.pl\/wp-content\/uploads\/2025\/06\/20250603_140647-1024x784.jpg 1024w, https:\/\/darkwave.astrocent.pl\/wp-content\/uploads\/2025\/06\/20250603_140647-300x230.jpg 300w, https:\/\/darkwave.astrocent.pl\/wp-content\/uploads\/2025\/06\/20250603_140647-768x588.jpg 768w, https:\/\/darkwave.astrocent.pl\/wp-content\/uploads\/2025\/06\/20250603_140647-1536x1176.jpg 1536w, https:\/\/darkwave.astrocent.pl\/wp-content\/uploads\/2025\/06\/20250603_140647-2048x1568.jpg 2048w\" sizes=\"(max-width: 1024px) 100vw, 1024px\" \/><\/figure>\n\n\n\n<h3 class=\"wp-block-heading\">What is DarkSide-20k?<\/h3>\n\n\n\n<p>DarkSide-20k is a next-generation dark matter detector being developed at the INFN Gran Sasso National Laboratory in Italy. It is designed to detect Weakly Interacting Massive Particles (WIMPs) \u2014 one of the most promising candidates for dark matter \u2014 using a dual-phase argon time projection chamber (TPC) filled with 20 tonnes of ultra-pure liquid argon.<\/p>\n\n\n\n<p>One of the experiment\u2019s key innovations is the use of argon sourced from underground reservoirs, which contains dramatically less radioactive isotope ^39Ar compared to atmospheric argon. This significantly reduces background noise, enhancing the sensitivity of the detector to rare events.<\/p>\n\n\n\n<p>DarkSide-20k builds on the success of earlier phases, including DarkSide-50, and aims to push the search for dark matter to unprecedented levels of sensitivity. If WIMPs exist within the range currently allowed by theory, DarkSide-20k could be the experiment that finds them.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Views: 9 From 2\u20136 June 2025, the Astrocent team participated in the DarkSide-20k summer collaboration meeting, held in<\/p>\n","protected":false},"author":3,"featured_media":2158,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[1],"tags":[],"class_list":["post-2157","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-news-news"],"_links":{"self":[{"href":"https:\/\/darkwave.astrocent.pl\/index.php\/wp-json\/wp\/v2\/posts\/2157","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/darkwave.astrocent.pl\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/darkwave.astrocent.pl\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/darkwave.astrocent.pl\/index.php\/wp-json\/wp\/v2\/users\/3"}],"replies":[{"embeddable":true,"href":"https:\/\/darkwave.astrocent.pl\/index.php\/wp-json\/wp\/v2\/comments?post=2157"}],"version-history":[{"count":1,"href":"https:\/\/darkwave.astrocent.pl\/index.php\/wp-json\/wp\/v2\/posts\/2157\/revisions"}],"predecessor-version":[{"id":2159,"href":"https:\/\/darkwave.astrocent.pl\/index.php\/wp-json\/wp\/v2\/posts\/2157\/revisions\/2159"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/darkwave.astrocent.pl\/index.php\/wp-json\/wp\/v2\/media\/2158"}],"wp:attachment":[{"href":"https:\/\/darkwave.astrocent.pl\/index.php\/wp-json\/wp\/v2\/media?parent=2157"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/darkwave.astrocent.pl\/index.php\/wp-json\/wp\/v2\/categories?post=2157"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/darkwave.astrocent.pl\/index.php\/wp-json\/wp\/v2\/tags?post=2157"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}