{"id":7657,"date":"1995-01-01T00:00:00","date_gmt":"1995-01-01T00:00:00","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/1995\/01\/01\/analisis-estadistico-topologico-y-ondicular-de-la-macroestructura-cosmica\/"},"modified":"1995-01-01T00:00:00","modified_gmt":"1995-01-01T00:00:00","slug":"analisis-estadistico-topologico-y-ondicular-de-la-macroestructura-cosmica","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/astronomia-y-astrofisica\/analisis-estadistico-topologico-y-ondicular-de-la-macroestructura-cosmica\/","title":{"rendered":"Analisis estadistico, topologico y ondicular de la macroestructura cosmica"},"content":{"rendered":"<h2>Tesis doctoral de <strong> Silvestre Paredes Hernandez <\/strong><\/h2>\n<p>Esta tesis trata principalmente dos aspectos relacionados con el analisis de datos cosmologicos: 1) revision del uso de estadisticos clasicos para el analisis de la distribucion de galaxias y cumulos. 2) presentacion de nuevas tecnicas de analisis con sus correspondientes aplicaciones. Se ha estudiado la longitud de correlacion, vo, y un comportamiento con la profundidad de la muestra, la existencia de inhomogeneidades locales, y la absorcion galactica. El analisis se ha realizado sobre el catalogo cfa. Se ha estudiado tambien la funcion de correlacion en cumulos y se ha aportado una interpretacion original de la diferencia entre los valores de vo encontrados para galaxias y cumulos. Se ha justificado la dependencia de las correlaciones espaciales en funcion del umbral de densidad. Por ultimo, se ha utilizado la transformada ondicular, warelet transform, tanto para estudiar el caracter multifractal de la distribucion de galaxias, como para la reconstruccion del campo de densidad de materia en el universo.<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Analisis estadistico, topologico y ondicular de la macroestructura cosmica<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Analisis estadistico, topologico y ondicular de la macroestructura cosmica <\/li>\n<li><strong>Autor:<\/strong>\u00a0 Silvestre Paredes Hernandez <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 Universitat de val\u00e9ncia (estudi general)<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 01\/01\/1995<\/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>Vicente Mart\u00ednez Garc\u00eda<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal: Eduard Salvador Sol\u00e9 <\/li>\n<li>Bernard Jones (vocal)<\/li>\n<li>Rosa Dom\u00ednguez Tenreiro (vocal)<\/li>\n<li>Diego Saez Milan (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Silvestre Paredes Hernandez Esta tesis trata principalmente dos aspectos relacionados con el analisis de datos cosmologicos: 1) [&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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