Synopsis
Introduction.- The Effective Field Theory of Dark Energy.- Beyond Horndeski.- Predictions for Primordial Tensor Modes.- Consistency Relations of the Large Scale Structure.- Conclusion.
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Dark Energy and the Formation of the Large Scale Structure of the Universe (Springer Theses)
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Dark Energy and the Formation of the Large Scale Structure of the Universe
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Springer International Publishing Jul 2016, 2016
ISBN 10 : 3319412094
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Buch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -This thesis presents several significant new results that shed light on two major puzzles of modern cosmology: the nature of inflation, the very early phase of the universe that is thought to have given rise to the large-scale structures that we observe today; and that of the current accelerated expansion. In particular, it develops a clean method for characterizing linear cosmological perturbations for general theories where gravity is modified and/or affected by a new component, called dark energy, responsible for the accelerated expansion. It proposes a new extension to what were long thought to be the most general scalar field theories devoid of instabilities, and demonstrates the robustness of the relation between the energy scale of inflation and the predicted amplitude of gravitational waves. Finally, it consolidates a set of consistency relations between correlation functions of the cosmological density field and investigates the phenomenological consequences of their potential violation. Presented in a clear, succinct and rigorous style, each of these original results is both profound and important and will leave a deep mark on the field. 132 pp. Englisch. N° de réf. du vendeur 9783319412092
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Dark Energy and the Formation of the Large Scale Structure of the Universe
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Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Nominated as an outstanding Ph.D. thesis by the Institute for Theoretical Physics-CEA Saclay, FranceIntroduces and explains the current exciting quest to understand the nature of cosmic inflation and accelerated expansion of the universe&nbs. N° de réf. du vendeur 121774890
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Dark Energy and the Formation of the Large Scale Structure of the Universe
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Dark Energy and the Formation of the Large Scale Structure of the Universe
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Springer, Springer Jul 2016, 2016
ISBN 10 : 3319412094
ISBN 13 : 9783319412092
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Buch. Etat : Neu. This item is printed on demand - Print on Demand Titel. Neuware -This thesis presents several significant new results that shed light on two major puzzles of modern cosmology: the nature of inflation, the very early phase of the universe that is thought to have given rise to the large-scale structures that we observe today; and that of the current accelerated expansion. In particular, it develops a clean method for characterizing linear cosmological perturbations for general theories where gravity is modified and/or affected by a new component, called dark energy, responsible for the accelerated expansion. It proposes a new extension to what were long thought to be the most general scalar field theories devoid of instabilities, and demonstrates the robustness of the relation between the energy scale of inflation and the predicted amplitude of gravitational waves. Finally, it consolidates a set of consistency relations between correlation functions of the cosmological density field and investigates the phenomenological consequences of their potential violation. Presented in a clear, succinct and rigorous style, each of these original results is both profound and important and will leave a deep mark on the field.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 132 pp. Englisch. N° de réf. du vendeur 9783319412092
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Dark Energy and the Formation of the Large Scale Structure of the Universe
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Springer International Publishing, 2016
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ISBN 13 : 9783319412092
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Buch. Etat : Neu. Druck auf Anfrage Neuware - Printed after ordering - This thesis presents several significant new results that shed light on two major puzzles of modern cosmology: the nature of inflation, the very early phase of the universe that is thought to have given rise to the large-scale structures that we observe today; and that of the current accelerated expansion. In particular, it develops a clean method for characterizing linear cosmological perturbations for general theories where gravity is modified and/or affected by a new component, called dark energy, responsible for the accelerated expansion. It proposes a new extension to what were long thought to be the most general scalar field theories devoid of instabilities, and demonstrates the robustness of the relation between the energy scale of inflation and the predicted amplitude of gravitational waves. Finally, it consolidates a set of consistency relations between correlation functions of the cosmological density field and investigates the phenomenological consequences of their potential violation. Presented in a clear, succinct and rigorous style, each of these original results is both profound and important and will leave a deep mark on the field. N° de réf. du vendeur 9783319412092
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Dark Energy and the Formation of the Large Scale Structure of the Universe
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ISBN 10 : 3319412094
ISBN 13 : 9783319412092
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Etat : Sehr gut. Zustand: Sehr gut | Sprache: Englisch | Produktart: Bücher | This thesis presents several significant new results that shed light on two major puzzles of modern cosmology: the nature of inflation, the very early phase of the universe that is thought to have given rise to the large-scale structures that we observe today; and that of the current accelerated expansion. In particular, it develops a clean method for characterizing linear cosmological perturbations for general theories where gravity is modified and/or affected by a new component, called dark energy, responsible for the accelerated expansion. It proposes a new extension to what were long thought to be the most general scalar field theories devoid of instabilities, and demonstrates the robustness of the relation between the energy scale of inflation and the predicted amplitude of gravitational waves. Finally, it consolidates a set of consistency relations between correlation functions of the cosmological density field and investigates the phenomenological consequences of their potential violation. Presented in a clear, succinct and rigorous style, each of these original results is both profound and important and will leave a deep mark on the field. N° de réf. du vendeur 26812042/12
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