{"id":2260,"date":"2002-05-01T18:46:14","date_gmt":"2002-05-01T18:46:14","guid":{"rendered":"http:\/\/casgroups.case.edu\/physics-senior-projects\/?p=2260"},"modified":"2016-06-20T13:32:05","modified_gmt":"2016-06-20T13:32:05","slug":"halo-signatures-in-dark-matter-detection","status":"publish","type":"post","link":"https:\/\/casgroups.case.edu\/physics-senior-projects\/halo-signatures-in-dark-matter-detection\/","title":{"rendered":"Halo Signatures in Dark Matter Detection"},"content":{"rendered":"<h3 style=\"text-align: center\">Cameron Keenan with Lawrence Krauss<\/h3>\n<h3 style=\"text-align: center\">Halo Signatures in Dark Matter Detection<\/h3>\n<p>\u00a0Matter plays a crucial role in the nature of the universe.\u00a0 Features such as the expansion rate of the universe and the value of Einstein&#8217;s Cosmological Constant are determined by the amount of matter present in the universe.\u00a0 If dark matter exists it will have a profound affect on physics.\u00a0 Up to this point no accurate measue of the local expansion rate of our galaxy has been recorded.\u00a0 It is our goal to measure this expansion rate and examine the affect that this value plays on the believed distribution of dark matter in the universe.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Cameron Keenan with Lawrence KraussHalo Signatures in Dark Matter Detection<\/p>\n<p>\u00a0Matter plays a crucial role in the nature of the universe.\u00a0 Features such as the expansion rate of the universe and the value of Einstein&#8217;s Cosmological Constant are determined by the amount of matter present in the universe.\u00a0 If dark matter exists it will have a profound affect on physics.\u00a0 Up to this point no accurate measue of the local expansion rate of our galaxy has been recorded.\u00a0 It is our goal to measure this expansion rate and examine the affect that this value plays on the believed distribution of dark matter in the universe.<\/p>\n<p><a href=\"https:\/\/casgroups.case.edu\/physics-senior-projects\/halo-signatures-in-dark-matter-detection\/\" class=\"more-link\">Continue reading&#8230; <span class=\"screen-reader-text\">Halo Signatures in Dark Matter Detection<\/span><\/a><\/p>\n","protected":false},"author":19,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"spay_email":""},"categories":[88,41],"tags":[],"jetpack_featured_media_url":"","_links":{"self":[{"href":"https:\/\/casgroups.case.edu\/physics-senior-projects\/wp-json\/wp\/v2\/posts\/2260"}],"collection":[{"href":"https:\/\/casgroups.case.edu\/physics-senior-projects\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/casgroups.case.edu\/physics-senior-projects\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/casgroups.case.edu\/physics-senior-projects\/wp-json\/wp\/v2\/users\/19"}],"replies":[{"embeddable":true,"href":"https:\/\/casgroups.case.edu\/physics-senior-projects\/wp-json\/wp\/v2\/comments?post=2260"}],"version-history":[{"count":3,"href":"https:\/\/casgroups.case.edu\/physics-senior-projects\/wp-json\/wp\/v2\/posts\/2260\/revisions"}],"predecessor-version":[{"id":2606,"href":"https:\/\/casgroups.case.edu\/physics-senior-projects\/wp-json\/wp\/v2\/posts\/2260\/revisions\/2606"}],"wp:attachment":[{"href":"https:\/\/casgroups.case.edu\/physics-senior-projects\/wp-json\/wp\/v2\/media?parent=2260"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/casgroups.case.edu\/physics-senior-projects\/wp-json\/wp\/v2\/categories?post=2260"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/casgroups.case.edu\/physics-senior-projects\/wp-json\/wp\/v2\/tags?post=2260"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}