{"id":2422,"date":"2011-10-25T10:06:13","date_gmt":"2011-10-25T17:06:13","guid":{"rendered":"http:\/\/cosmologyscience.com\/cosblog\/?p=2422"},"modified":"2016-02-13T20:42:40","modified_gmt":"2016-02-14T04:42:40","slug":"opera-concern-detecting-only-1-neutrino-hour","status":"publish","type":"post","link":"https:\/\/cosmologyscience.com\/cosblog\/opera-concern-detecting-only-1-neutrino-hour\/","title":{"rendered":"Faster than Light Concern &#8211; Detecting Only 1 Neutrino per Hour"},"content":{"rendered":"<p><strong>Regarding the potentially <a href=\"http:\/\/cosmologyscience.com\/cosblog\/neutrinos-break-light-speed-barrier\/\">Faster than light Neutrinos<\/a>, it is vital to realize that only about one (1) Neutrino is detected by Italy&#8217;s OPERA every hour; that&#8217;s <span style=\"text-decoration: underline;\">one Neutrino per hour<\/span>.<\/strong><\/p>\n<p><strong>Compare that to how <a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0412440\">every square centimeter on Earth (facing the Sun) encounters some 65 billion solar neutrinos per second<\/a>.<\/strong><\/p>\n<p><a href=\"http:\/\/operaweb.lngs.infn.it\/spip.php?rubrique41\"><img loading=\"lazy\" decoding=\"async\" title=\"Neutrino Beam Path\" src=\"http:\/\/operaweb.lngs.infn.it\/local\/cache-vignettes\/L420xH233\/beamtrajectory-en-71dd9-8be65.png\" alt=\"Neutrino Beam Path\" width=\"210\" height=\"116\" \/><\/a><\/p>\n<p><strong>When that single neutrino hits in Italy, its timed arrival is associated (extrapolated back) to a recorded proton pulse at CERN by using the time it would take for a photon to travel the same distance.<\/strong><\/p>\n<p><strong><!--more--><\/strong><br \/>\n<strong> The <a href=\"http:\/\/en.wikipedia.org\/wiki\/Super_Proton_Synchrotron\">Super Proton Synchrotron (SPS) sends pulses of protons<\/a> so that they can be distinguished from a steady beam, but only one (1) neutrino is measured at the Italian detector, for every quadrillion protons fired from CERN\u2019s SPS (16,111 neutrino hits for 10^20th protons fired over 3 years).<\/strong><\/p>\n<p><strong>While OPERA researchers believe they know which pulse is sending the Neutrino detected, I am not at all confident that they know which proton (converted into pion, converted into muon-Neutrino, converted into) &#8211; neutrino they are measuring. It is not at all clear because there is just too little data at the detector.<\/strong><\/p>\n<p><strong>Paraphrasing <a href=\"http:\/\/cosmologyscience.com\/cosblog\/neutrinos-break-light-speed-barrier\/\">Mitchell Porter<\/a>:<\/strong><\/p>\n<blockquote><p><strong>This is a statistical analysis. They are not matching up an individual detection at the emitter in Switzerland with an individual detection at the detector in Italy; they are taking averages and measuring statistical distributions. The interpretation of the starting time depends on which model of meson decay is employed.<\/strong><\/p><\/blockquote>\n<p><strong>To improve the experiment I would like to see <a href=\"http:\/\/cosmologyscience.com\/cosblog\/neutrinos-break-light-speed-barrier\/\">clear pulses of detections (as opposed to one hit per hour). To do so they might consider increasing the proton beam density by at least 3, and probably 4 or 5 magnitudes until they get neutrino hits on the order of 1,000 to 10,000 per hour.<\/a><\/strong><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Regarding the potentially Faster than light Neutrinos, it is vital to realize that only about one (1) Neutrino is detected by Italy&#8217;s OPERA every hour; that&#8217;s one Neutrino per hour. Compare that to how every square centimeter on Earth (facing &hellip; <a href=\"https:\/\/cosmologyscience.com\/cosblog\/opera-concern-detecting-only-1-neutrino-hour\/\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"iawp_total_views":0,"footnotes":"","_links_to":"","_links_to_target":""},"categories":[13,20],"tags":[116,269,208,209,272,267,268],"class_list":["post-2422","post","type-post","status-publish","format-standard","hentry","category-basic-science","category-particles","tag-cern","tag-faster-than-light","tag-italy","tag-neutrinos","tag-o","tag-sps","tag-super-proton-synchrotron"],"_links":{"self":[{"href":"https:\/\/cosmologyscience.com\/cosblog\/wp-json\/wp\/v2\/posts\/2422","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/cosmologyscience.com\/cosblog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/cosmologyscience.com\/cosblog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/cosmologyscience.com\/cosblog\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/cosmologyscience.com\/cosblog\/wp-json\/wp\/v2\/comments?post=2422"}],"version-history":[{"count":0,"href":"https:\/\/cosmologyscience.com\/cosblog\/wp-json\/wp\/v2\/posts\/2422\/revisions"}],"wp:attachment":[{"href":"https:\/\/cosmologyscience.com\/cosblog\/wp-json\/wp\/v2\/media?parent=2422"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/cosmologyscience.com\/cosblog\/wp-json\/wp\/v2\/categories?post=2422"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/cosmologyscience.com\/cosblog\/wp-json\/wp\/v2\/tags?post=2422"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}