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OmniScriptum Dynamique des Galaxies: Gravité newtonienne et Gravité modifiée: Tester la loi de la gravitation par des simulations numériques (Omn.Univ.Europ.)

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Description

La dynamique des systèmes gravitationnels s'appuie traditionnellement sur la physique de Newton. Appliquée à l'échelle des galaxies, la gravitation newtonienne impose l'existence d'une certaine matière, actuellement invisible: la matière noire. Si ce modèle (LCDM) rencontre des succès à grande échelle, des difficultés apparaissent à l'échelle des galaxies. Dans ma thèse, j'explore par des simulations numériques une alternative de la gravitation newtonienne: MOND (Modified Newtonian Dynamics), où la loi newtonienne de la gravité est modifiée selon une échelle d'accélération, sans l'intervention de la matière noire. Cette expression de la gravitation est non-linéaire et impose une méthode différente de celle utilisée dans les systèmes avec matière noire. Ce travail ouvre des horizons vers des simulations cosmologiques qui pourraient valoriser un modèle en analysant la formation hiérarchique des structures à partir des fluctuations de densité primordiales.

Product Specifications

Format
paperback
Domain
Amazon UK
Release Date
05 November 2010
Listed Since
08 November 2010

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