{"id":87718,"date":"2000-04-12T00:00:00","date_gmt":"2000-04-12T00:00:00","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/sin-categoria\/perturbaciones-post-newtonianas-en-mecanica-celeste-relativista\/"},"modified":"2000-04-12T00:00:00","modified_gmt":"2000-04-12T00:00:00","slug":"perturbaciones-post-newtonianas-en-mecanica-celeste-relativista","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/fisica\/perturbaciones-post-newtonianas-en-mecanica-celeste-relativista\/","title":{"rendered":"Perturbaciones post-newtonianas en mecanica celeste relativista"},"content":{"rendered":"<h2>Tesis doctoral de <strong> Pedro Zamorano Belio <\/strong><\/h2>\n<p>A partir de las ecuaciones de campo de einstein aplicadas al campo gravitatorio solar, se obtienen por un lado las ecuaciones de movimiento en aproximaci\u00f3n post-newtoniana correspondiente a part\u00edculas test, y por otro, se demuestra que no es necesario introducir t\u00e9rminos no lineales endichas ecuaciones cuando se utilizan las coordenas gausianas polares o sus coordenadas fermi asociadas.  es analog\u00eda con la hidrodinamica relativista, se ha obtenido la aproximaci\u00f3n post-newtoniana tanto del tensor velocidad de deformaci\u00f3n como del tensor de spin, lo que ha permitido definir y caracterizar los movimientos r\u00edgido e irrotacional, as\u00ed como obtener la distribuci\u00f3n de velocidades asociada a dichos movimientos.  a continuaci\u00f3n, se construyen y caracterizan sistemas de referencia en rotaci\u00f3n r\u00edgida en el sentido post-newtoniano de born para un sistema constituido para n cuerpos extensos y se demuestra la imposibilidad de que el movimiento sea simult\u00e1neamente r\u00edgido e irrotacional. Finalmente, se propone distintos sistemas de referencia r\u00edgidos aplicables a cuerpos del sistema soler que incluyen los efectos de marea.<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Perturbaciones post-newtonianas en mecanica celeste relativista<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Perturbaciones post-newtonianas en mecanica celeste relativista <\/li>\n<li><strong>Autor:<\/strong>\u00a0 Pedro Zamorano Belio <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 Complutense de Madrid<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 04\/12\/2000<\/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>Jose Gambi Fernandez<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal:  Diaz diaz Jes\u00fas ildefonso <\/li>\n<li>Alberto Ibort latre (vocal)<\/li>\n<li> Lopez bonilla Luis Francisco (vocal)<\/li>\n<li>Juan Getino fernandez (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Pedro Zamorano Belio A partir de las ecuaciones de campo de einstein aplicadas al campo gravitatorio solar, [&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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