{"id":33426,"date":"2016-10-17T09:50:13","date_gmt":"2016-10-17T07:50:13","guid":{"rendered":"http:\/\/www.h-its.org\/event\/lecture-stellar-evolution\/"},"modified":"2019-10-28T13:41:45","modified_gmt":"2019-10-28T12:41:45","slug":"lecture-stellar-evolution","status":"publish","type":"hits-teaching","link":"https:\/\/www.h-its.org\/de\/teachings\/lecture-stellar-evolution\/","title":{"rendered":"Lecture: Stellar structures, evolution, and explosions"},"content":{"rendered":"\r\n<h2 class=\"wp-block-heading\">Winter semester 2016\/2017<\/h2>\r\n\r\n\r\n\r\n<p>Prof. Dr. F. R\u00f6pke, L. Horst, Dr. P. Edelmann, Dr. S. Jones, Dr. S. Ohlmann<\/p>\r\n\r\n\r\n\r\n<p><strong>Lecture:\u00a0 <\/strong>Tuesday, 14 &#8211; 16 h<\/p>\r\n\r\n\r\n\r\n<p><strong>Homework session: <\/strong>Tuesday, 16 &#8211; 18 h<\/p>\r\n\r\n\r\n\r\n<p>The homework problems have to be uploaded. <a href=\"https:\/\/elearning2.uni-heidelberg.de\/mod\/assign\/view.php?id=384208\">Click here<\/a> to find the lecture on the E-learning system.<\/p>\r\n\r\n\r\n\r\n<h2 class=\"wp-block-heading\">Syllabus<\/h2>\r\n\r\n\r\n\r\n<p>Stars are the building blocks of the Universe. This lecture covers their structures, evolution, and explosions from a theoretical point of view.<\/p>\r\n\r\n\r\n\r\n<ul class=\"wp-block-list\">\r\n<li>Brief overview of observational results<\/li>\r\n<li>Theoretical modeling approaches\r\n<ul>\r\n<li>fluid mechanics and mechanical equilibrium of stars<\/li>\r\n<li>simple stellar models<\/li>\r\n<li>energetic equilibrium of stars<\/li>\r\n<\/ul>\r\n<\/li>\r\n<li>Physical properties of stellar matter\r\n<ul>\r\n<li>stellar thermodynamics<\/li>\r\n<li>equation of state<\/li>\r\n<li>opacities<\/li>\r\n<\/ul>\r\n<\/li>\r\n<li>Nuclear processes in stars\r\n<ul>\r\n<li>energy production and reactions<\/li>\r\n<li>thermonuclear reaction rates<\/li>\r\n<li>main nuclear burning cycles<\/li>\r\n<li>neutrino emission<\/li>\r\n<\/ul>\r\n<\/li>\r\n<li>Energy transport in stellar interiors\r\n<ul>\r\n<li>radiation, diffusion, conduction<\/li>\r\n<li>convection<\/li>\r\n<\/ul>\r\n<\/li>\r\n<li>Stellar evolution models\r\n<ul>\r\n<li>basic equations<\/li>\r\n<li>stellar stability<\/li>\r\n<li>homology relations<\/li>\r\n<li>schematic stellar evolution<\/li>\r\n<\/ul>\r\n<\/li>\r\n<li>Early stages of stellar evolution and main sequence phase\r\n<ul>\r\n<li>pre-main sequence<\/li>\r\n<li>zero-age main sequence<\/li>\r\n<li>central hydrogen burning<\/li>\r\n<\/ul>\r\n<\/li>\r\n<li>Post-main sequence evolution\r\n<ul>\r\n<li>Schoenberg-Chandrasekhar limit<\/li>\r\n<li>hydrogen-shell burning<\/li>\r\n<li>helium burning<\/li>\r\n<li>pulsational instability<\/li>\r\n<\/ul>\r\n<\/li>\r\n<li>Late evolution of low- and intermediate mass stars\r\n<ul>\r\n<li>the asymptotic giant branch<\/li>\r\n<li>white dwarfs<\/li>\r\n<\/ul>\r\n<\/li>\r\n<li>Massive stars\r\n<ul>\r\n<li>stellar winds<\/li>\r\n<li>advanced burning stages<\/li>\r\n<li>pre-supernova evolution<\/li>\r\n<\/ul>\r\n<\/li>\r\n<li>Stellar explosions\r\n<ul>\r\n<li>supernovae<\/li>\r\n<li>stellar remnants<\/li>\r\n<\/ul>\r\n<\/li>\r\n<\/ul>\r\n","protected":false},"author":57,"featured_media":29914,"template":"","hits-research-group":[1279],"class_list":["post-33426","hits-teaching","type-hits-teaching","status-publish","has-post-thumbnail","hentry","hits-research-group-pso-de"],"acf":[],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.4 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>Lecture: Stellar structures, evolution, and explosions - HITS gGmbH<\/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:\/\/www.h-its.org\/de\/teachings\/lecture-stellar-evolution\/\" \/>\n<meta property=\"og:locale\" content=\"de_DE\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Lecture: Stellar structures, evolution, and explosions - HITS gGmbH\" \/>\n<meta property=\"og:description\" content=\"Winter semester 2016\/2017 Prof. Dr. F. 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