On the Lagrangian Theory of Structure Formation in Relativistic Cosmology : Intrinsic Perturbation Approach and Gravitoelectromagnetism Fosca Al Roumi

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On the Lagrangian Theory of Structure Formation in Relativistic Cosmology : Intrinsic Perturbation Approach and Gravitoelectromagnetism Fosca Al Roumi On the Lagrangian Theory of Structure Formation in Relativistic Cosmology : intrinsic Perturbation Approach and Gravitoelectromagnetism Fosca Al Roumi To cite this version: Fosca Al Roumi. On the Lagrangian Theory of Structure Formation in Relativistic Cosmology : intrinsic Perturbation Approach and Gravitoelectromagnetism. Cosmology and Extra-Galactic As- trophysics [astro-ph.CO]. Université Claude Bernard - Lyon I, 2015. English. NNT : 2015LYO10136. tel-01367703 HAL Id: tel-01367703 https://tel.archives-ouvertes.fr/tel-01367703 Submitted on 16 Sep 2016 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Thèse présentée devant l’Université Claude Bernard Lyon - I École Doctorale de Physique et d’Astrophysique pour l’obtention du DIPLÔME de DOCTORAT Spécialité : Physique Théorique / Cosmologie (arrêté du 7 août 2006) par Fosca Al Roumi Théorie Lagrangienne Relativiste de la Formation des Grandes Structures : Description Intrinsèque des Perturbations et Gravitoélectromagnétisme A soutenir publiquement le 18 Septembre 2015 devant la Commission d’Examen : Prof. P. Salati Président du jury - LAPTH, Annecy le Vieux Prof. B. Roukema Rapporteur et examinateur - Torún Centre for Astronomy, Torún Prof. R. Sussman Rapporteur et examinateur - Instituto de Ciencias Nucleares, México, D. F. Prof. R. Triay Examinateur - CPT, Marseille Prof. R. Walder Examinateur - CRAL, Lyon Prof. T. Buchert Directeur de thèse - CRAL, Lyon PHD THESIS of the UNIVERSITY of LYON Delivered by the UNIVERSITY CLAUDE BERNARD LYON 1 Subject: THEORETICAL PHYSICS / COSMOLOGY submitted by Ms FOSCA AL ROUMI for the degree of DOCTOR OF THEORETICAL PHYSICS On the Lagrangian Theory of Structure Formation in Relativistic Cosmology: Intrinsic Perturbation Approach and Gravitoelectromagnetism To be defended 18 September 2015 in front of the following Examining Committee: Prof. P. Salati President - LAPTH, Annecy le Vieux Prof. B. Roukema Reviewer and examiner - Torún Centre for Astronomy, Torún Prof. R. Sussman Reviewer and examiner - Instituto de Ciencias Nucleares, Mexico City Prof. R. Triay Examiner - CPT, Marseille Prof. R. Walder Examiner - CRAL, Lyon Prof. T. Buchert Supervisor - CRAL, Lyon Acknowlegments / Remerciements First of all I would like to thank my mentor, Thomas Buchert. It will take me many years to realize how lucky I’ve been to work under your direction. Thank you for all your scientific skills, your patience and your rigor. But most of all, thank you for your sense of humor, your creativity and for being so open-minded. I hope I took some of your qualities during these three years. I wish to thank Gilles Chabrier for his fruitful remarks during seminars and for hosting us at CRAL-ENS. My thanks to Herbert Wagner and Martin Kerscher, with whom I worked in Munich on gravitoelectromagnetism. Your help, remarks and advices have been very important for my work on this topic. This student exchange was supported by the French–Bavarian Cooperation Center, BFHZ Munich http://www.bayern-france.org/. Special thanks to Xavier Roy, who helped me a lot throughout the PhD. Thank you for the detailed answers to my questions, for all the explanations on foliation of space-time and differential geometry and for all the useful advices you gave me on the manuscript. Thank you also for all the non-scientific discussions we had. They have been crucial to me. My thanks to Alexander Wiegand for the fruitful discussions, the nice work we did together, for you time and advices. Thanks to Léo Brunswic for all the work we achieved on topology and Hodge decom- position. Your mathematical skills have been really precious for this work. I wish also to thank Alexandre Alles for the help and the useful discussions on the blackboard. My thanks to Boud Roukema for the useful discussions on topology and for his very interesting work on inhomogeneous cosmology. Thank you for your time and help! Thanks to Frank Steiner for sharing his great knowledge on cosmic topology. Martin France, thank you for all the nice discussions we had on the CMB. Thanks to Rolf Walder for the nice remarks and discussions we had during the semi- nars. I would also like to thank Roberto Sussman and Boud Roukema for having accepted to be reviewer of my thesis and spending some of your precious time on reading my thesis and writing a report. I also want to thank Pierre Salati for being the president of my examining committee, for the very interesting discussions we had on the scalar model for dark matter at the beginning of my PhD and at Cargèse last september. Thank you also for all the help gave me in my research career. iii I also want to thank Roland Triay and Rolf Walder for having accepted to be examiner of my thesis. Thanks to Jan Ostrowski for everything: from physics to beers and ping-pong. Thanks also to Pierre Mourier for the scientific discussions and the nice time we had together. Good luck with your PhD! Thanks to Thomas Buchert, Martin France, Boud Roukema, Rolf Walder, Frank Steiner, Léo Brunswick, Jan Ostrowski, Tomek Kazimierczak and Pierre Mourier for the really nice dinners we had together. It is a pleasure to talk about science or something else around a glass of wine! Je voudrais aussi remercier Stephanie Vignier, Sylvie Réa and Sylvie Flores pour avoir rendu tous les aspects administratifs bien plus simples. C’est toujours avec grand plaisir que je suis allée vous poser des questions et vous demander de l’aide. Merci pour votre patience et votre bonne humeur! Vielen Dank an Marie von München. Les quelques jours de rédaction à Munich ont étés un vrai plaisir! Merci à tous mes amis lyonnais, qui m’ont fait passer d’excellents moments pendant ces trois ans! Merci à Julien, Catherine, Martin, Elisa, Tatjana, Camille, Grégoire, Lila, Elsa, Thiago, Mariana, Mirella et Matei. Un grand merci à mes colocs adorés, Matteo et Lucy. Quel bonheur d’avoir partagé avec vous le même toit! Martin, merci aussi pour tous tes conseils sur la rédaction de la thèse! Tatjana, merci de m’avoir acceuillie après cette longue période de rédaction à Milano, la ville qui ne se couche jamais. Julien, merci de m’avoir aidée à certains moments particulièrement délicats! Merci aussi à mes amis parisiens! Julia, Fanny et Victoria, les moments que nous avons passés ensemble et les fous rires que nous avons eus ont grandement participé à mon équilibre mental. Merci aussi à Daniel, Louison, Olivier, Léo. J’espère vous voir plus souvent maintenant. Merci enfin à Mohamad et Amélie pour avoir toujours étés là pour moi. Vous m’avez beaucoup aidée. Merci aussi à mon frère Meyar pour m’avoir prêté son coffret Paradjanov. Constance, il faudrait un chapitre entier pour te remercier. Alors, je préfère le faire de vive voix dans un bon restaurant! Sans ces rencontres et ces échanges, mon travail de thèse n’aurait pas été possible. Je vous remercie donc sincèrement. iv Abstract The dynamics of structure formation in the Universe is usually described by Newto- nian numerical simulations and analytical models in the frame of the Standard Model of Cosmology. The structures are then defined on a homogeneous and isotropic background. Such a description has major drawbacks since, to be self-consistent, it entails a large amount of dark components in the content of the Universe. Different strategies are considered to solve this enigma. Particle physicists have been searching for some exotic sources of the stress-energy tensor to account for these dark components. Nevertheless, no direct evidence of these 26% of dark matter and 69% of dark energy has yet been given. Therefore, some alternative theories to General Relativity are explored. To address the problem of dark matter and dark energy, we will neither suppose that exotic sources contribute to the content of the Universe, nor that General Rela- tivity is obsolete. We will develop a more realistic description of structure formation in the frame of General Relativity and thus no longer assume that the average model is a homogeneous-isotropic solution of the Einstein equations, as claimed by the Standard Model of Cosmology. During my work under the supervision of Thomas Buchert, I contributed to the devel- opment of the perturbative formalism that enables a more realistic description of space- time dynamics. In the framework of the intrinsic Lagrangian approach, which avoids defin- ing physical quantities on a flat background, I contributed to the building of relativistic solutions to the gravitoelectric part of the Einstein equations from the generalization of the Newtonian perturbative solutions. Moreover, the gravitoelectromagnetic approach I worked with has provided a new understanding of the dynamics of the analytical solu- tions to the field equations. Finally, treating globally the spatial manifold, I used powerful mathematical tools and theorems to describe the impact of topology on the dynamics of gravitational waves. v Résumé La dynamique de formation des structures de l’Univers est habituellement décrite dans le cadre du modèle standard de Cosmologie par des simulations numériques newtoniennes et des modèles analytiques. Les structures sont alors associées à des grandeurs définies sur un fond homogène et isotrope. Cependant, pour que les observations cosmologiques soient cohérentes avec le modèle standard, il est nécessaire de supposer l’existance d’une grande proportion d’éléments de nature inconnue dans le contenu de l’Univers. Différentes stratégies sont envisagées pour déterminer la nature de ces éléments.
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