Titlebook: Dark Energy and the Formation of the Large Scale Structure of the Universe; Jérôme Gleyzes Book 2016 The Editor(s) (if applicable) and The

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Consistency Relations of the Large Scale Structure,ark matter distribution can be predicted through N-body simulations for example, this cannot be said for galaxies. The problem is that galaxies are what we observe when doing those experiments, so that one needs models to relate their distribution to that of dark matter. This limits the theoretical

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Book 2016the 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..

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XLeitfäden der angewandten Informatikark matter distribution can be predicted through N-body simulations for example, this cannot be said for galaxies. The problem is that galaxies are what we observe when doing those experiments, so that one needs models to relate their distribution to that of dark matter. This limits the theoretical

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Book 2016 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

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2190-5053 iting quest to understand the nature of cosmic inflation andThis 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 th

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Predictions for Primordial Tensor Modes,for the scalar, or the shape of the potential. This means that it is difficult to use temperature measurements to put robust constraints on models of inflation. The situation is even worse, since the almost scale invariant spectrum that Planck observed can be produced without having inflation [.].

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https://doi.org/10.1007/978-3-319-41210-8Theory of Dark Energy; Large Scale Structure; Nature of Inflation; Cosmological Perturbations; Scalar Fi