{"id":112740,"date":"2015-08-11T17:00:00","date_gmt":"2015-08-11T14:00:00","guid":{"rendered":"http:\/\/www.fyysika.ee\/?guid=a7c8d2509175f296979dfa41fa76c940"},"modified":"2015-08-11T17:00:00","modified_gmt":"2015-08-11T14:00:00","slug":"testing-the-dark-matter-scenario-for-pev-neutrinos-observed-in-icecube","status":"publish","type":"post","link":"https:\/\/www.fyysika.ee\/?p=112740","title":{"rendered":"Testing the Dark Matter Scenario for PeV Neutrinos Observed in IceCube"},"content":{"rendered":"<p>Author(s): Kohta Murase, Ranjan Laha, Shin\u2019ichiro Ando, and Markus Ahlers<\/p>\n<p>A class of very-heavy dark matter models could account for the ultra high energy neutrinos observed by IceCube and will be tested by future <math xmlns=\"http:\/\/www.w3.org\/1998\/Math\/MathML\" display=\"inline\"><mi>\u03b3<\/mi><\/math>-ray detectors and neutrino telescopes.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" src=\"http:\/\/d22izw7byeupn1.cloudfront.net\/journals\/PRL\/key_images\/10.1103\/PhysRevLett.115.071301.png\" width=\"200\" height=\"100\"><\/p>\n<p>[Phys. Rev. Lett. 115, 071301] Published Tue Aug 11, 2015<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Author(s): Kohta Murase, Ranjan Laha, Shin&rsquo;ichiro Ando, and Markus Ahlers<\/p>\n<p>A class of very-heavy dark matter models could account for the ultra high energy neutrinos observed by IceCube and will be tested by future &gamma;-ray detectors and neutrino telescopes.<\/p>\n<p><img decoding=\"async\" src=\"http:\/\/d22izw7byeupn1.cloudfront.net\/journals\/PRL\/key_images\/10.1103\/PhysRevLett.115.071301.png\" width=\"200\" height='\"100\"'><br \/>[Phys. Rev. Lett. 115, 071301] Published Tue Aug 11, 2015<\/p>\n","protected":false},"author":0,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_genesis_hide_title":false,"_genesis_hide_breadcrumbs":false,"_genesis_hide_singular_image":false,"_genesis_hide_footer_widgets":false,"_genesis_custom_body_class":"","_genesis_custom_post_class":"","_genesis_layout":"","footnotes":""},"categories":[182],"tags":[],"class_list":{"0":"post-112740","1":"post","2":"type-post","3":"status-publish","4":"format-standard","6":"category-rss-teadus","7":"entry"},"_links":{"self":[{"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/posts\/112740","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/types\/post"}],"replies":[{"embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=112740"}],"version-history":[{"count":0,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/posts\/112740\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=112740"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=112740"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=112740"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}