{"id":3192,"date":"2026-03-13T19:37:00","date_gmt":"2026-03-13T18:37:00","guid":{"rendered":"https:\/\/projects.ift.uam-csic.es\/severo\/?p=3192"},"modified":"2026-03-13T19:37:00","modified_gmt":"2026-03-13T18:37:00","slug":"the-mystery-of-cosmic-acceleration","status":"publish","type":"post","link":"https:\/\/projects.ift.uam-csic.es\/severo\/index.php\/2026\/03\/13\/the-mystery-of-cosmic-acceleration\/","title":{"rendered":"The Mystery of Cosmic Acceleration."},"content":{"rendered":"\n<h2 class=\"wp-block-heading\">DIFT Colloquium.<\/h2>\n\n\n\n<div id=\"wp-block-themeisle-blocks-advanced-columns-e31fb33f\" class=\"wp-block-themeisle-blocks-advanced-columns has-1-columns has-desktop-equal-layout has-tablet-equal-layout has-mobile-equal-layout has-vertical-unset\"><div class=\"wp-block-themeisle-blocks-advanced-columns-overlay\"><\/div><div class=\"wp-block-themeisle-blocks-advanced-columns-separators top\"><svg id=\"slant\" fill=\"var(--nv-primary-accent)\" viewBox=\"0 0 100 100\" width=\"100%\" height=\"100\" preserveAspectRatio=\"none\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\" class=\"\"><path d=\"M0 0 L100 100 L100 0 Z\"><\/path><\/svg><\/div><div class=\"innerblocks-wrap\">\n<div id=\"wp-block-themeisle-blocks-advanced-column-9394befc\" class=\"wp-block-themeisle-blocks-advanced-column\">\n<div style=\"height:100px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n<\/div>\n<\/div><\/div>\n\n\n\n<h3 class=\"wp-block-heading\"><strong>David Weinberg (The Ohio State University, USA<\/strong>).<\/h3>\n\n\n\n<h4 class=\"wp-block-heading\"><strong>Abstrac<\/strong>t:&nbsp;<\/h4>\n\n\n\n<p>Cosmic acceleration is one of the most surprising cosmological discoveries<br>of the past century. Even the \u201csimplest\u201d explanations require new,<br>cosmologically dominant energy components with exotic physical properties.<br>Current and near-future experiments are seeking clues to the origin of<br>cosmic acceleration by measuring the history of expansion and structure<br>growth with sub-percent precision over a wide span of redshift. I will<br>review the observational methods that underpin these measurements<br>and assess the current state of play, with particular attention to recent<br>measurements from the Dark Energy Spectroscopic Instrument (DESI) which<br>suggest that the properties of dark energy are evolving at a startling rate.<br>I will discuss the prospects and challenges for the new generation of<br>experiments \u2014 DESI, the Euclid mission, the Vera Rubin Observatory,<br>and the Nancy Grace Roman Space Telescope \u2014 which aim to sharpen cosmological<br>measurements by a factor of ten.<\/p>\n\n\n\n<p><strong>When<\/strong>: Wednesday, March 18th, 2026 \u2013 15:00h (CEST)<br><strong>Location&amp;Place<\/strong>:&nbsp;CFTMAT&nbsp;Auditorium<\/p>\n\n\n\n<p>After the talk, we will have a&nbsp;<strong>coffee gathering<\/strong>, providing an opportunity to continue the discussion and interact with the speaker in an informal setting.<\/p>\n\n\n\n<div style=\"height:50px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<figure class=\"wp-block-image size-large\"><img loading=\"lazy\" decoding=\"async\" width=\"724\" height=\"1024\" src=\"https:\/\/projects.ift.uam-csic.es\/severo\/wp-content\/uploads\/2026\/03\/Coloquios-DIFT-weimberg-1-724x1024.jpg\" alt=\"\" class=\"wp-image-3193\" srcset=\"https:\/\/projects.ift.uam-csic.es\/severo\/wp-content\/uploads\/2026\/03\/Coloquios-DIFT-weimberg-1-724x1024.jpg 724w, https:\/\/projects.ift.uam-csic.es\/severo\/wp-content\/uploads\/2026\/03\/Coloquios-DIFT-weimberg-1-212x300.jpg 212w, https:\/\/projects.ift.uam-csic.es\/severo\/wp-content\/uploads\/2026\/03\/Coloquios-DIFT-weimberg-1-768x1086.jpg 768w, https:\/\/projects.ift.uam-csic.es\/severo\/wp-content\/uploads\/2026\/03\/Coloquios-DIFT-weimberg-1-1086x1536.jpg 1086w, https:\/\/projects.ift.uam-csic.es\/severo\/wp-content\/uploads\/2026\/03\/Coloquios-DIFT-weimberg-1-1448x2048.jpg 1448w, https:\/\/projects.ift.uam-csic.es\/severo\/wp-content\/uploads\/2026\/03\/Coloquios-DIFT-weimberg-1.jpg 1587w\" sizes=\"auto, (max-width: 724px) 100vw, 724px\" \/><\/figure>\n\n\n\n<div style=\"height:49px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-9d6595d7 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\" style=\"flex-basis:20%\"><div style=\"padding-top:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30)\" class=\"taxonomy-category has-text-align-center has-link-color wp-elements-1f1b0f0e735d262df90dfd01bcdce4b8 wp-block-post-terms has-text-color has-nv-text-dark-bg-color has-background has-neve-link-color-background-color\"><a href=\"https:\/\/projects.ift.uam-csic.es\/severo\/index.php\/category\/colloquium\/\" rel=\"tag\">Colloquium<\/a><\/div><\/div>\n<\/div>\n","protected":false},"excerpt":{"rendered":"<p>DIFT Colloquium. David Weinberg (The Ohio State University, USA). Abstract:&nbsp; Cosmic acceleration is one of the most surprising cosmological discoveriesof the past century. Even the \u201csimplest\u201d explanations require new,cosmologically dominant energy components with exotic physical properties.Current and near-future experiments are seeking clues to the origin ofcosmic acceleration by measuring the history of expansion and structuregrowth&hellip;&nbsp;<a href=\"https:\/\/projects.ift.uam-csic.es\/severo\/index.php\/2026\/03\/13\/the-mystery-of-cosmic-acceleration\/\" class=\"\" rel=\"bookmark\">Read More &raquo;<span class=\"screen-reader-text\">The Mystery of Cosmic Acceleration.<\/span><\/a><\/p>\n","protected":false},"author":1,"featured_media":3193,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"neve_meta_sidebar":"","neve_meta_container":"","neve_meta_enable_content_width":"","neve_meta_content_width":0,"neve_meta_title_alignment":"","neve_meta_author_avatar":"","neve_post_elements_order":"","neve_meta_disable_header":"","neve_meta_disable_footer":"","neve_meta_disable_title":"","_themeisle_gutenberg_block_has_review":false,"footnotes":""},"categories":[14],"tags":[],"class_list":["post-3192","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-colloquium"],"_links":{"self":[{"href":"https:\/\/projects.ift.uam-csic.es\/severo\/index.php\/wp-json\/wp\/v2\/posts\/3192","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/projects.ift.uam-csic.es\/severo\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/projects.ift.uam-csic.es\/severo\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/projects.ift.uam-csic.es\/severo\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/projects.ift.uam-csic.es\/severo\/index.php\/wp-json\/wp\/v2\/comments?post=3192"}],"version-history":[{"count":2,"href":"https:\/\/projects.ift.uam-csic.es\/severo\/index.php\/wp-json\/wp\/v2\/posts\/3192\/revisions"}],"predecessor-version":[{"id":3195,"href":"https:\/\/projects.ift.uam-csic.es\/severo\/index.php\/wp-json\/wp\/v2\/posts\/3192\/revisions\/3195"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/projects.ift.uam-csic.es\/severo\/index.php\/wp-json\/wp\/v2\/media\/3193"}],"wp:attachment":[{"href":"https:\/\/projects.ift.uam-csic.es\/severo\/index.php\/wp-json\/wp\/v2\/media?parent=3192"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/projects.ift.uam-csic.es\/severo\/index.php\/wp-json\/wp\/v2\/categories?post=3192"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/projects.ift.uam-csic.es\/severo\/index.php\/wp-json\/wp\/v2\/tags?post=3192"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}