Characterizing the non-linear evolution of dark energy models

Diplôme Thèse Characterizing the non-linear evolution of dark energy models eng 2020-09-03 author Hassani Farbod 858532 director Kunz Martin 109032 10.13097/archive-ouverte/unige:143066 urn:nbn:ch:unige-1430661 Sc. 5492 Understanding the reason behind the observed accelerating expansion of the Universe is one of the most notable puzzles in modern cosmology, and conceivably in fundamental physics. In the upcoming years, near-future surveys will probe structure formation with unprecedented precision and will put firm constraints on the cosmological parameters, including those that describe properties of dark energy. In light of this, in this thesis, we mainly focus on characterizing the non-linear evolution of dark energy and modified gravity models with the aim to probe some of these models precisely while treating all cosmological components including the dark energy part accurately. This treatment of the dark sector is especially required by the future high precision cosmological surveys. Dewey 500.2 37 Département de physique théorique 133 false 3d8a7635-fa62-485e-8156-92e19cefbdb6 Thesis Public Thesis_Farbod_Hassani.pdf 23403238 application/pdf openAccess Faculté des sciences / Section de physique / Département de physique théorique

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Characterizing the non-linear evolution of dark energy models				2020	686	790

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Hassani, Farbod