{"id":1775,"date":"2022-05-26T15:00:11","date_gmt":"2022-05-26T12:00:11","guid":{"rendered":"https:\/\/phsites.technion.ac.il\/soker\/?p=1775"},"modified":"2022-08-23T20:23:36","modified_gmt":"2022-08-23T17:23:36","slug":"three-dimensional-simulations-of-the-jet-feedback-mechanism-in-common-envelope-jets-supernovae-three-dimensional-simulations-of-the-jet-feedback-mechanism-in-common-envelope-jets-supernovae-june","status":"publish","type":"post","link":"https:\/\/phsites.technion.ac.il\/soker\/three-dimensional-simulations-of-the-jet-feedback-mechanism-in-common-envelope-jets-supernovae-three-dimensional-simulations-of-the-jet-feedback-mechanism-in-common-envelope-jets-supernovae-june\/","title":{"rendered":"Three-dimensional simulations of the jet feedback mechanism in common envelope jets supernovae (June 2022)"},"content":{"rendered":"\n<p>We (<strong>Shlomi Hillel<\/strong>, <strong>Ron Schreier<\/strong>, <strong>Noam Soker<\/strong>) conducted three-dimensional hydrodynamical simulations of common envelope jets supernova (CEJSN) events where we assume that a neutron star (NS) launches jets as it orbits inside the outer zones of a red supergiant (RSG) envelope, and find the negative jet feedback coefficient to be \u2243 0.1 &#8211; 0.2. See paper <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2022MNRAS.tmp.1286H\/abstract\" target=\"_blank\" rel=\"noopener\">here<\/a>.&nbsp;<\/p>\n<p><a href=\"https:\/\/phsites.technion.ac.il\/soker\/wp-content\/uploads\/sites\/4\/2022\/05\/HillelSchreierSoker2022.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\"alignnone  wp-image-1777\" src=\"https:\/\/phsites.technion.ac.il\/soker\/wp-content\/uploads\/sites\/4\/2022\/05\/HillelSchreierSoker2022.jpg\" alt=\"\" width=\"589\" height=\"406\" srcset=\"https:\/\/phsites.technion.ac.il\/soker\/wp-content\/uploads\/sites\/4\/2022\/05\/HillelSchreierSoker2022.jpg 1084w, https:\/\/phsites.technion.ac.il\/soker\/wp-content\/uploads\/sites\/4\/2022\/05\/HillelSchreierSoker2022-300x207.jpg 300w, https:\/\/phsites.technion.ac.il\/soker\/wp-content\/uploads\/sites\/4\/2022\/05\/HillelSchreierSoker2022-1024x706.jpg 1024w, https:\/\/phsites.technion.ac.il\/soker\/wp-content\/uploads\/sites\/4\/2022\/05\/HillelSchreierSoker2022-768x529.jpg 768w\" sizes=\"auto, (max-width: 589px) 100vw, 589px\" \/><\/a><\/p>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>We (Shlomi Hillel, Ron Schreier, Noam Soker) conducted three-dimensional hydrodynamical simulations of common envelope jets supernova (CEJSN) events where we assume that a neutron star (NS) launches jets as it orbits inside the outer zones of a red supergiant (RSG) envelope, and find the negative jet feedback coefficient to be \u2243 0.1 &#8211; 0.2. See &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":[7],"class_list":{"0":"post-1775","1":"post","2":"type-post","3":"status-publish","4":"format-standard","6":"category-news","7":"tag-jets-in-common-envelope","8":"entry"},"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.4 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>Three-dimensional simulations of the jet feedback mechanism in common envelope jets supernovae (June 2022) 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\/three-dimensional-simulations-of-the-jet-feedback-mechanism-in-common-envelope-jets-supernovae-three-dimensional-simulations-of-the-jet-feedback-mechanism-in-common-envelope-jets-supernovae-june\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Three-dimensional simulations of the jet feedback mechanism in common envelope jets supernovae (June 2022) Prof. Noam Soker\" \/>\n<meta property=\"og:description\" content=\"We (Shlomi Hillel, Ron Schreier, Noam Soker) conducted three-dimensional hydrodynamical simulations of common envelope jets supernova (CEJSN) events where we assume that a neutron star (NS) launches jets as it orbits inside the outer zones of a red supergiant (RSG) envelope, and find the negative jet feedback coefficient to be \u2243 0.1 &#8211; 0.2. See &hellip;\" \/>\n<meta property=\"og:url\" content=\"https:\/\/phsites.technion.ac.il\/soker\/three-dimensional-simulations-of-the-jet-feedback-mechanism-in-common-envelope-jets-supernovae-three-dimensional-simulations-of-the-jet-feedback-mechanism-in-common-envelope-jets-supernovae-june\/\" \/>\n<meta property=\"og:site_name\" content=\"Prof. Noam Soker\" \/>\n<meta property=\"article:published_time\" content=\"2022-05-26T12:00:11+00:00\" \/>\n<meta property=\"article:modified_time\" content=\"2022-08-23T17:23:36+00:00\" \/>\n<meta property=\"og:image\" content=\"https:\/\/phsites.technion.ac.il\/soker\/wp-content\/uploads\/sites\/4\/2022\/05\/HillelSchreierSoker2022.jpg\" \/>\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\t<meta name=\"twitter:label2\" content=\"Est. reading time\" \/>\n\t<meta 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