{"id":532060,"date":"2025-10-27T23:14:09","date_gmt":"2025-10-27T23:14:09","guid":{"rendered":"https:\/\/www.europesays.com\/uk\/532060\/"},"modified":"2025-10-27T23:14:09","modified_gmt":"2025-10-27T23:14:09","slug":"dark-matter-could-color-our-view-of-the-universe","status":"publish","type":"post","link":"https:\/\/www.europesays.com\/uk\/532060\/","title":{"rendered":"Dark matter could color our view of the universe"},"content":{"rendered":"<p>            <img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/www.europesays.com\/uk\/wp-content\/uploads\/2025\/10\/universe-2.jpg\" alt=\"universe\" title=\"Credit: Unsplash\/CC0 Public Domain\" width=\"800\" height=\"530\"\/><\/p>\n<p>                Credit: Unsplash\/CC0 Public Domain<\/p>\n<p>Dark matter has two central properties: it has mass like regular matter, and unlike regular matter, it reacts weakly or not at all with light. Neutrinos satisfy these two criteria, but neutrinos move through space at nearly the speed of light, making them a form of hot dark matter. The observations we have suggest that <a href=\"https:\/\/briankoberlein.com\/blog\/cold-and-dark\/\" target=\"_blank\" rel=\"noopener\">dark matter is cold.<\/a><\/p>\n<p>There also aren&#8217;t enough neutrinos to account for all of dark matter, so we know dark matter isn&#8217;t made of <a href=\"https:\/\/phys.org\/tags\/neutrinos\/\" rel=\"tag noopener\" class=\"textTag\" target=\"_blank\">neutrinos<\/a>. No other known particle meets the criteria, so we have no idea what dark matter might be made of. Cue the <a href=\"https:\/\/phys.org\/tags\/theoretical+physicists\/\" rel=\"tag noopener\" class=\"textTag\" target=\"_blank\">theoretical physicists<\/a>.<\/p>\n<p>One of the more popular theoretical ideas is that dark matter is made of <a href=\"https:\/\/briankoberlein.com\/post\/nerds-seeking-wimps\/\" target=\"_blank\" rel=\"noopener\">weakly interacting massive particles (WIMPs).<\/a> There are various versions of WIMPs, but the basic idea is that they are particles much too massive to be observed in the <a href=\"https:\/\/phys.org\/tags\/particle+accelerators\/\" rel=\"tag noopener\" class=\"textTag\" target=\"_blank\">particle accelerators<\/a> we currently have. One consequence of WIMPs is that they would\u2014either spontaneously or through mutual interactions\u2014decay into the less <a href=\"https:\/\/phys.org\/tags\/massive+particles\/\" rel=\"tag noopener\" class=\"textTag\" target=\"_blank\">massive particles<\/a> we currently observe.<\/p>\n<p>Because of this, there have been several searches for emissions from dark matter, such as <a href=\"https:\/\/phys.org\/tags\/gamma+rays\/\" rel=\"tag noopener\" class=\"textTag\" target=\"_blank\">gamma rays<\/a>. The idea is that when dark matter collides, it could create a cascade of high-energy particles and light. Evidence for this has been <a href=\"https:\/\/briankoberlein.com\/blog\/when-dark-matter-collides\/\" target=\"_blank\" rel=\"noopener\">weak at best<\/a> so far and doesn&#8217;t rise to the level of clear evidence. If dark matter interacts, it doesn&#8217;t interact strongly, and it doesn&#8217;t emit significant light.<\/p>\n<p>But a recent study looks at WIMP decay particles in a different way. The study is <a href=\"https:\/\/linkinghub.elsevier.com\/retrieve\/pii\/S0370269325006781\" target=\"_blank\" rel=\"noopener\">published<\/a> in the journal Physics Letters B.<\/p>\n<p>Rather than detecting high-energy decay particles directly, the authors calculate how background light would interact with these particles. They found that there could be interactions that affect light from distant galaxies in a measurable way.<\/p>\n<p>The team calculated the theoretical scattering cross-sections for two dark matter cases: one where dark matter only interacts gravitationally and one where dark matter particle collisions produce secondary particles. They found that in the first case, low-energy photons tend to scatter more forward, while in the second case, photons tend to backscatter more often.<\/p>\n<p>This means that if dark matter is purely gravitational, then light passing through it would get a tiny bit of extra energy overall, skewing it slightly to the blue. If <a href=\"https:\/\/phys.org\/tags\/dark+matter\/\" rel=\"tag noopener\" class=\"textTag\" target=\"_blank\">dark matter<\/a> is weakly interacting, then light passing through it loses a bit of energy and appears slightly more red.<\/p>\n<p>It should be emphasized that this tinting effect is very tiny. It&#8217;s far too small to allow for alternate cosmology models such as tired light. But the effect might be large enough for us to observe. For example, the authors compared their models with Fermi-LAT observations of the Milky Way&#8217;s <a href=\"https:\/\/phys.org\/tags\/galactic+center\/\" rel=\"tag noopener\" class=\"textTag\" target=\"_blank\">galactic center<\/a>.<\/p>\n<p>They found that either model fits within the uncertainties of the observations we have. Better observations of high-energy gamma rays from the center of our galaxy might prove or disprove the model.<\/p>\n<p>Dark matter remains a deep puzzle of cosmology, so it&#8217;s good to keep looking for new ideas. Perhaps the discovery we&#8217;ve been looking for will prove that we see the universe through rose-tinted glasses.<\/p>\n<p><strong>More information:<\/strong><br \/>\n\t\t\t\t\t\t\t\t\t\t\t\tA. Acar et al, Dark matter: Red or blue?, Physics Letters B (2025). <a data-doi=\"1\" href=\"https:\/\/dx.doi.org\/10.1016\/j.physletb.2025.139920\" target=\"_blank\" rel=\"noopener\">DOI: 10.1016\/j.physletb.2025.139920<\/a><\/p>\n<p>\n\t\t\t\t\t\t\t\t\t\t\t\t\tProvided by<br \/>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<a href=\"https:\/\/phys.org\/partners\/universe-today\/\" target=\"_blank\" rel=\"noopener\">Universe Today<\/a><br \/>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<a class=\"icon_open\" href=\"https:\/\/www.universetoday.com\/\" target=\"_blank\" rel=\"nofollow noopener\"><\/p>\n<p>\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/a>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/p>\n<p>\n\t\t\t\t\t\t\t\t\t\t\t\t<strong>Citation<\/strong>:<br \/>\n\t\t\t\t\t\t\t\t\t\t\t\tDark matter could color our view of the universe (2025, October 26)<br \/>\n\t\t\t\t\t\t\t\t\t\t\t\tretrieved 27 October 2025<br \/>\n\t\t\t\t\t\t\t\t\t\t\t\tfrom https:\/\/phys.org\/news\/2025-10-dark-view-universe.html\n\t\t\t\t\t\t\t\t\t\t\t <\/p>\n<p>\n\t\t\t\t\t\t\t\t\t\t\t This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no<br \/>\n\t\t\t\t\t\t\t\t\t\t\t part may be reproduced without the written permission. The content is provided for information purposes only.\n\t\t\t\t\t\t\t\t\t\t\t <\/p>\n","protected":false},"excerpt":{"rendered":"Credit: Unsplash\/CC0 Public Domain Dark matter has two central properties: it has mass like regular matter, and unlike&hellip;\n","protected":false},"author":2,"featured_media":532061,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[8],"tags":[75,76,74,71,70,72,53,73,16,15],"class_list":{"0":"post-532060","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-science","8":"tag-materials","9":"tag-nanotech","10":"tag-physics","11":"tag-physics-news","12":"tag-science","13":"tag-science-news","14":"tag-technology","15":"tag-technology-news","16":"tag-uk","17":"tag-united-kingdom"},"share_on_mastodon":{"url":"https:\/\/pubeurope.com\/@uk\/115448674746691737","error":""},"_links":{"self":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/posts\/532060","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/comments?post=532060"}],"version-history":[{"count":0,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/posts\/532060\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/media\/532061"}],"wp:attachment":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/media?parent=532060"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/categories?post=532060"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/tags?post=532060"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}