{"id":534,"date":"2024-07-19T17:08:00","date_gmt":"2024-07-19T17:08:00","guid":{"rendered":"https:\/\/neutrinos.ific.uv.es\/?p=534"},"modified":"2025-02-20T17:11:33","modified_gmt":"2025-02-20T17:11:33","slug":"next-100-assembly-completed","status":"publish","type":"post","link":"https:\/\/neutrinos.ific.uv.es\/index.php\/2024\/07\/19\/next-100-assembly-completed\/","title":{"rendered":"NEXT-100 assembly completed"},"content":{"rendered":"\n<p>The assembly of the NEXT-100 detector is complete!<\/p>\n\n\n\n<p>Presently, the detector is working at low pressure to test and calibrate the instrumentation. NEXT-100 employs 60 photomultipliers in the energy plane, compared to the 12 PMTs used in its predecessor,&nbsp;<a href=\"https:\/\/next-experiment.org\/next-white\/\">NEXT-White<\/a>. The tracking plane is made up of 3584 SiPMs (1792 in NEXT-White) meant to provide the topological signature of the events.<\/p>\n\n\n\n<p>NEXT-100 is expected to be able to provide a background rate below 10<sup>-3<\/sup>&nbsp;counts \/ keV \/ kg \/ year&nbsp;and to reach a sensitivity to the neutrinoless double beta decay half-life of&nbsp;6 x 10<sup>25<\/sup>&nbsp;years&nbsp;at the 90% CL for 3 years of data taking.<\/p>\n\n\n\n<p>This detector will also set the grounds for the construction of a ton-scale detector,&nbsp;<a href=\"https:\/\/next-experiment.org\/next-hd-and-next-bold\/\">NEXT-HD<\/a>, boosting the sensitivity above 10<sup>27<\/sup>&nbsp;yr.&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>The assembly of the NEXT-100 detector is complete! Presently, the detector is working at low pressure to test and calibrate the instrumentation. NEXT-100 employs 60 photomultipliers in the energy plane, compared to the 12 PMTs used in its predecessor,&nbsp;NEXT-White. The tracking plane is made up of 3584 SiPMs (1792 in NEXT-White) meant to provide the [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":535,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[11,12],"tags":[],"class_list":["post-534","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-group-highlights","category-science-highlights"],"_links":{"self":[{"href":"https:\/\/neutrinos.ific.uv.es\/index.php\/wp-json\/wp\/v2\/posts\/534","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/neutrinos.ific.uv.es\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/neutrinos.ific.uv.es\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/neutrinos.ific.uv.es\/index.php\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/neutrinos.ific.uv.es\/index.php\/wp-json\/wp\/v2\/comments?post=534"}],"version-history":[{"count":1,"href":"https:\/\/neutrinos.ific.uv.es\/index.php\/wp-json\/wp\/v2\/posts\/534\/revisions"}],"predecessor-version":[{"id":536,"href":"https:\/\/neutrinos.ific.uv.es\/index.php\/wp-json\/wp\/v2\/posts\/534\/revisions\/536"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/neutrinos.ific.uv.es\/index.php\/wp-json\/wp\/v2\/media\/535"}],"wp:attachment":[{"href":"https:\/\/neutrinos.ific.uv.es\/index.php\/wp-json\/wp\/v2\/media?parent=534"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/neutrinos.ific.uv.es\/index.php\/wp-json\/wp\/v2\/categories?post=534"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/neutrinos.ific.uv.es\/index.php\/wp-json\/wp\/v2\/tags?post=534"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}