{"id":96532,"date":"2018-03-11T10:16:48","date_gmt":"2018-03-11T10:16:48","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/sin-categoria\/busqueda-de-evidencias-de-aceleracion-de-hadrones-en-remanentes-de-supernova\/"},"modified":"2018-03-11T10:16:48","modified_gmt":"2018-03-11T10:16:48","slug":"busqueda-de-evidencias-de-aceleracion-de-hadrones-en-remanentes-de-supernova","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/astronomia-y-astrofisica\/busqueda-de-evidencias-de-aceleracion-de-hadrones-en-remanentes-de-supernova\/","title":{"rendered":"Busqueda de evidencias de aceleracion de hadrones en remanentes de supernova"},"content":{"rendered":"<h2>Tesis doctoral de <strong> Mar\u00eda  Teresa Costado Dios <\/strong><\/h2>\n<p>Desde el espacio exterior llegan constantemente a la tierra gran cantidad de particulas cargadas,  la mayoria protones, aunque algunas veces tambien llegan nucleos atomicos que pueden ser tan masivos como el hierro. El espectro de estas particulas abarca un rango muy amplio de energia y sigue una ley de potencias. Este espectro plantea  el problema de averiguar cuales son los mecanismos fisicos que lo pueden generar. Una de las primeras cuestiones es determinar el lugar de origen y la correlacion con algun objeto astrofisico con el objetivo de elaborar un modelo que explique a que se deben esas altas energias. Es de esperar que en los posibles escenarios astrofisicos en los que estas particulas adquieren su energia se libere radiacion electromagnetica. La direccion de estos fotones no sufre los efectos de los campos magneticos interestelares, por tanto el estudio y deteccion de los mismos proporciona la posibilidad de encontrar informacion acerca del origen de los rayos cosmicos.  nuestro proposito sera el estudio del origen de los rayos cosmicos galacticos. Se llevara a  cabo un analisis de un conjunto de candidatos a fuentes de rayos cosmicos observadas con el  telescopio magic-i (major atmospheric gamma-ray imaging cherenkov) para obtener  el espectro de la se\u00f1al de la emision asociada o, en caso de no encontrarse,  determinar un limite superior al flujo de rayos gamma para compararlo con observaciones  de otros telescopios o para en un futuro hacer mas observaciones con los telescopios magic. basicamente se observaran remanentes de supernova, pues son los mejores candidatos a regiones  donde se aceleren los hadrones existentes en los rayos cosmicos de tan altas energias.<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Busqueda de evidencias de aceleracion de hadrones en remanentes de supernova<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Busqueda de evidencias de aceleracion de hadrones en remanentes de supernova <\/li>\n<li><strong>Autor:<\/strong>\u00a0 Mar\u00eda  Teresa Costado Dios <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 La laguna<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 14\/10\/2009<\/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 Jes\u00fas Garc\u00eda L\u00f3pez<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal: artemio Herrero dav\u00f3 <\/li>\n<li>abelardo Moralejo olaizola (vocal)<\/li>\n<li>joan Font serra (vocal)<\/li>\n<li>victoria Fonseca gonz\u00e1lez (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Mar\u00eda Teresa Costado Dios Desde el espacio exterior llegan constantemente a la tierra gran cantidad de particulas [&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 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