This book presents a study of inflationary dynamics of the early Universe in the large extra-dimensional braneworld cosmology. We first provide an introduction to the standard cosmology. Motivated by some of its shortcomings, we introduce the theory of cosmic inflation followed by the detailed derivations of scalar and tensor power spectra. We also discuss the mechanism for reducing the tensor to scalar ratio in Gauss-Bonnet inflationary models. In braneworld, Friedmann equations are modified to include a quadratic term in energy density.We review some of the essential ingredients of swampland program, and discuss its constraints on the theory of cosmic inflation.In particular, the tensor-to-scalar ratio can be reduced without changing the spectral index. Moreover, the constraints on the slope of the potential can be relaxed that are important to realize de Sitter Universe supported by observations.
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Vendeur : BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Allemagne
Taschenbuch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -This book presents a study of inflationary dynamics of the early Universe in the large extra-dimensional braneworld cosmology. We first provide an introduction to the standard cosmology. Motivated by some of its shortcomings, we introduce the theory of cosmic inflation followed by the detailed derivations of scalar and tensor power spectra. We also discuss the mechanism for reducing the tensor to scalar ratio in Gauss-Bonnet inflationary models. In braneworld, Friedmann equations are modified to include a quadratic term in energy density.We review some of the essential ingredients of swampland program, and discuss its constraints on the theory of cosmic inflation.In particular, the tensor-to-scalar ratio can be reduced without changing the spectral index. Moreover, the constraints on the slope of the potential can be relaxed that are important to realize de Sitter Universe supported by observations. 128 pp. Englisch. N° de réf. du vendeur 9786202565097
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Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Autor/Autorin: Sabir MudassarMudassar Sabir: Huazhong University of Science & TechnologyThis book presents a study of inflationary dynamics of the early Universe in the large extra-dimensional braneworld cosmology. We first provide an introduc. N° de réf. du vendeur 385947746
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Taschenbuch. Etat : Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - This book presents a study of inflationary dynamics of the early Universe in the large extra-dimensional braneworld cosmology. We first provide an introduction to the standard cosmology. Motivated by some of its shortcomings, we introduce the theory of cosmic inflation followed by the detailed derivations of scalar and tensor power spectra. We also discuss the mechanism for reducing the tensor to scalar ratio in Gauss-Bonnet inflationary models. In braneworld, Friedmann equations are modified to include a quadratic term in energy density.We review some of the essential ingredients of swampland program, and discuss its constraints on the theory of cosmic inflation.In particular, the tensor-to-scalar ratio can be reduced without changing the spectral index. Moreover, the constraints on the slope of the potential can be relaxed that are important to realize de Sitter Universe supported by observations. N° de réf. du vendeur 9786202565097
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Taschenbuch. Etat : Neu. This item is printed on demand - Print on Demand Titel. Neuware -This book presents a study of inflationary dynamics of the early Universe in the large extra-dimensional braneworld cosmology. We first provide an introduction to the standard cosmology. Motivated by some of its shortcomings, we introduce the theory of cosmic inflation followed by the detailed derivations of scalar and tensor power spectra. We also discuss the mechanism for reducing the tensor to scalar ratio in Gauss-Bonnet inflationary models. In braneworld, Friedmann equations are modified to include a quadratic term in energy density.We review some of the essential ingredients of swampland program, and discuss its constraints on the theory of cosmic inflation.In particular, the tensor-to-scalar ratio can be reduced without changing the spectral index. Moreover, the constraints on the slope of the potential can be relaxed that are important to realize de Sitter Universe supported by observations.VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 128 pp. Englisch. N° de réf. du vendeur 9786202565097
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