{"id":138458,"date":"2026-01-12T17:35:41","date_gmt":"2026-01-12T17:35:41","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/sin-categoria\/modelos-de-atmosferas-de-supernovas-de-tipo-ia-desde-la-fase-fotosferica-a-la-fase-nebular\/"},"modified":"2026-01-12T17:35:41","modified_gmt":"2026-01-12T17:35:41","slug":"modelos-de-atmosferas-de-supernovas-de-tipo-ia-desde-la-fase-fotosferica-a-la-fase-nebular","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/barcelona\/modelos-de-atmosferas-de-supernovas-de-tipo-ia-desde-la-fase-fotosferica-a-la-fase-nebular\/","title":{"rendered":"Modelos de atmosferas de supernovas de tipo ia desde la fase fotosferica a la fase nebular."},"content":{"rendered":"<h2>Tesis doctoral de <strong>  Ruiz Lapuente M. Pilar Carolina <\/strong><\/h2>\n<p>La presente tesis consiste en el desarrollo y aplicacion de modelos de atmosferas de supernovas que son capaces de predecir los espectros de radiacion observados en distintas fases de su evolucion en luminosidad: en la fase fotosferica un metodo de montecarlo es utilizado para el calculo del transporte de radiacion juntamente con un tratamiento fuera de equilibrio termodinamico local de las ecuaciones de equilibrio estadistico de los niveles energeticos de los distintos iones presentes en la envoltura de sn. En la fase nebular un tratamiento del transporte apropiado para esta fase con el calculo del equilibrio termico ionizacion y excitacion del material eyectado es ajustado a una tecnica de optimizacion de los valores de los parametros del modelo que mejor ajustan las observaciones. Este metodo, aplicado a las supernovas de tipo ia, permite la determinacion de distancias y masas de distintos elementos sintetizados.<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Modelos de atmosferas de supernovas de tipo ia desde la fase fotosferica a la fase nebular.<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Modelos de atmosferas de supernovas de tipo ia desde la fase fotosferica a la fase nebular. <\/li>\n<li><strong>Autor:<\/strong>\u00a0  Ruiz Lapuente M. Pilar Carolina <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 Barcelona<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 01\/01\/1992<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n<h3>Direcci\u00f3n y tribunal<\/h3>\n<ul>\n<li><strong>Director de la tesis<\/strong>\n<ul>\n<li>Ram\u00f3n Canal Masgoret<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal: Francisco Sanchez Martinez <\/li>\n<li>Willem Wamsteker (vocal)<\/li>\n<li>Jordi Isern Vilaboy (vocal)<\/li>\n<li>Artemio Herrero Davo (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Ruiz Lapuente M. Pilar Carolina La presente tesis consiste en el desarrollo y aplicacion de modelos de [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"site-sidebar-layout":"default","site-content-layout":"","ast-site-content-layout":"","site-content-style":"default","site-sidebar-style":"default","ast-global-header-display":"","ast-banner-title-visibility":"","ast-main-header-display":"","ast-hfb-above-header-display":"","ast-hfb-below-header-display":"","ast-hfb-mobile-header-display":"","site-post-title":"","ast-breadcrumbs-content":"","ast-featured-img":"","footer-sml-layout":"","theme-transparent-header-meta":"","adv-header-id-meta":"","stick-header-meta":"","header-above-stick-meta":"","header-main-stick-meta":"","header-below-stick-meta":"","astra-migrate-meta-layouts":"default","ast-page-background-enabled":"default","ast-page-background-meta":{"desktop":{"background-color":"var(--ast-global-color-4)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-gradient":""},"tablet":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-gradient":""},"mobile":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-gradient":""}},"ast-content-background-meta":{"desktop":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-gradient":""},"tablet":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-gradient":""},"mobile":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-gradient":""}},"footnotes":""},"categories":[7616,1050,951,1052,7615,33966],"tags":[26221,7770,33969,10114,252994,15292],"class_list":["post-138458","post","type-post","status-publish","format-standard","hentry","category-astronomia-optica","category-astronomia-y-astrofisica","category-barcelona","category-cosmologia-y-cosmogonia","category-espectroscopia-astrofisica","category-supernovas","tag-artemio-herrero-davo","tag-francisco-sanchez-Martinez","tag-jordi-isern-vilaboy","tag-ramon-canal-masgoret","tag-ruiz-lapuente-m-pilar-carolina","tag-willem-wamsteker"],"_links":{"self":[{"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/posts\/138458","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/comments?post=138458"}],"version-history":[{"count":0,"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/posts\/138458\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/media?parent=138458"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/categories?post=138458"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/tags?post=138458"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}