{"id":739,"date":"2014-12-28T05:20:55","date_gmt":"2014-12-28T05:20:55","guid":{"rendered":"http:\/\/phsites.technion.ac.il\/soker\/?p=739"},"modified":"2014-12-28T05:20:55","modified_gmt":"2014-12-28T05:20:55","slug":"implications-turbulence-jets-core-collapse-supernova-explosions-december-2014","status":"publish","type":"post","link":"https:\/\/phsites.technion.ac.il\/soker\/implications-turbulence-jets-core-collapse-supernova-explosions-december-2014\/","title":{"rendered":"Implications of turbulence for jets in core-collapse supernova explosions (December 2014)"},"content":{"rendered":"<p><strong>Avishai Gilkis<\/strong> and I show that turbulence in core collapse supernovae which has been shown recently to ease shock revival can also lead to the formation of intermittent thick accretion disks, or accretion belts, around the newly born neutron star. This is likely to result in jets that explode the star. We strengthen the <span style=\"background-color: #ffff00\">jittering jets mechanism<\/span> as a prominent explosion mechanism of massive stars.\u00a0<a title=\"Paper\" href=\"http:\/\/arxiv.org\/abs\/1412.4984\">Paper<\/a> was posted on astro-ph.\u00a0<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Avishai Gilkis and I show that turbulence in core collapse supernovae which has been shown recently to ease shock revival can also lead to the formation of intermittent thick accretion disks, or accretion belts, around the newly born neutron star. This is likely to result in jets that explode the star. We strengthen the jittering &hellip;<\/p>\n","protected":false},"author":6,"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":[2],"tags":[],"class_list":{"0":"post-739","1":"post","2":"type-post","3":"status-publish","4":"format-standard","6":"category-news","7":"entry"},"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.5 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>Implications of turbulence for jets in core-collapse supernova explosions (December 2014) Prof. Noam Soker<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/phsites.technion.ac.il\/soker\/implications-turbulence-jets-core-collapse-supernova-explosions-december-2014\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Implications of turbulence for jets in core-collapse supernova explosions (December 2014) Prof. Noam Soker\" \/>\n<meta property=\"og:description\" content=\"Avishai Gilkis and I show that turbulence in core collapse supernovae which has been shown recently to ease shock revival can also lead to the formation of intermittent thick accretion disks, or accretion belts, around the newly born neutron star. This is likely to result in jets that explode the star. We strengthen the jittering &hellip;\" \/>\n<meta property=\"og:url\" content=\"https:\/\/phsites.technion.ac.il\/soker\/implications-turbulence-jets-core-collapse-supernova-explosions-december-2014\/\" \/>\n<meta property=\"og:site_name\" content=\"Prof. Noam Soker\" \/>\n<meta property=\"article:published_time\" content=\"2014-12-28T05:20:55+00:00\" \/>\n<meta name=\"author\" content=\"Noam Soker\" \/>\n<meta name=\"twitter:card\" content=\"summary_large_image\" \/>\n<meta name=\"twitter:label1\" content=\"Written by\" \/>\n\t<meta name=\"twitter:data1\" content=\"Noam Soker\" \/>\n<script type=\"application\/ld+json\" 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