Non-Gaussianity and Statistical Anisotropy - in Cosmological Inflationary Models - Taschenbuch

2010, ISBN: 9783838399850

[ED: Taschenbuch / Paperback], [PU: LAP Lambert Academic Publishing], Cosmology is in a golden age, and some experiments of high complexity are running up or have been proposed in order t… Mehr…

[ED: Taschenbuch / Paperback], [PU: LAP Lambert Academic Publishing], Cosmology is in a golden age, and some experiments of high complexity are running up or have been proposed in order to know about the properties of our Universe and test theoretical cosmological models. So, it is pertinent to study some of these models and confront them with observations. In this book we use the N formalism to study the statistical descriptors for some cosmological inflationary models that allow us to obtain large levels of non-gaussianity and violations of the statistical isotropy. Basically, we study two different classes of models: a class of models that includes only scalar field perturbations, specifically a subclass of small-field slow-roll models of inflation with canonical kinetic terms, and the class of models that admits both vector and scalar field perturbations. The theoretical results are compared with the most recent observations and the available parameter window where these models are valid is extracted. This book will be of great help for both graduate students and researchers interested in the latest developments in the subjects of primordial non-gaussianity and statistical anisotropy., DE, [SC: 0.00], Neuware, gewerbliches Angebot, 128, Selbstabholung und Barzahlung, PayPal, Offene Rechnung, Banküberweisung, Internationaler Versand<

Versandkosten:Versandkostenfrei, Versand nach Deutschland. (EUR 0.00)

2010, ISBN: 9783838399850

[ED: Taschenbuch / Paperback], [PU: LAP Lambert Academic Publishing], Cosmology is in a golden age, and some experiments of high complexity are running up or have been proposed in order t… Mehr…

[ED: Taschenbuch / Paperback], [PU: LAP Lambert Academic Publishing], Cosmology is in a golden age, and some experiments of high complexity are running up or have been proposed in order to know about the properties of our Universe and test theoretical cosmological models. So, it is pertinent to study some of these models and confront them with observations. In this book we use the N formalism to study the statistical descriptors for some cosmological inflationary models that allow us to obtain large levels of non-gaussianity and violations of the statistical isotropy. Basically, we study two different classes of models: a class of models that includes only scalar field perturbations, specifically a subclass of small-field slow-roll models of inflation with canonical kinetic terms, and the class of models that admits both vector and scalar field perturbations. The theoretical results are compared with the most recent observations and the available parameter window where these models are valid is extracted. This book will be of great help for both graduate students and researchers interested in the latest developments in the subjects of primordial non-gaussianity and statistical anisotropy., DE, [SC: 0.00], Neuware, gewerbliches Angebot, 128, Selbstabholung und Barzahlung, PayPal, offene Rechnung, Banküberweisung, Internationaler Versand<

Versandkosten:Versandkostenfrei, Versand nach Deutschland. (EUR 0.00)

2010

ISBN: 9783838399850

Cosmology is in a golden age, and some experiments of high complexity are running up or have been proposed in order to know about the properties of our Universe and test theoretical cosmo… Mehr…

Cosmology is in a golden age, and some experiments of high complexity are running up or have been proposed in order to know about the properties of our Universe and test theoretical cosmological models. So, it is pertinent to study some of these models and confront them with observations. In this book we use the dN formalism to study the statistical descriptors for some cosmological inflationary models that allow us to obtain large levels of non-gaussianity and violations of the statistical isotropy. Basically, we study two different classes of models: a class of models that includes only scalar field perturbations, specifically a subclass of small-field slow-roll models of inflation with canonical kinetic terms, and the class of models that admits both vector and scalar field perturbations. The theoretical results are compared with the most recent observations and the available parameter window where these models are valid is extracted. This book will be of great help for both graduate students and researchers interested in the latest developments in the subjects of primordial non-gaussianity and statistical anisotropy. Buch (fremdspr.) Yeinzon Rodríguez García#César Alonso Valenzuela Toledo Taschenbuch, LAP LAMBERT Academic Publishing, 17.09.2010, LAP LAMBERT Academic Publishing, 2010<

Nr. 24434587. Versandkosten:, Versandfertig innert 4 - 7 Werktagen, zzgl. Versandkosten. (EUR 17.01)

2010, ISBN: 9783838399850

Erscheinungsdatum: 09/2010, Medium: Taschenbuch, Einband: Kartoniert / Broschiert, Titel: Non-Gaussianity and Statistical Anisotropy, Titelzusatz: in Cosmological Inflationary Models, Aut… Mehr…

Erscheinungsdatum: 09/2010, Medium: Taschenbuch, Einband: Kartoniert / Broschiert, Titel: Non-Gaussianity and Statistical Anisotropy, Titelzusatz: in Cosmological Inflationary Models, Autor: Valenzuela Toledo, César Alonso // Rodríguez García, Yeinzon, Verlag: LAP Lambert Acad. Publ., Sprache: Englisch, Rubrik: Physik // Astronomie, Sonstiges, Seiten: 128, Informationen: Paperback, Gewicht: 208 gr, Verkäufer: averdo Belletristik<

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ISBN: 3838399854

Non-Gaussianity and Statistical Anisotropy ab 58.99 € als Taschenbuch: in Cosmological Inflationary Models. Aus dem Bereich: Bücher, Wissenschaft, Physik, Medien > Bücher, LAP Lambert Aca… Mehr…

Non-Gaussianity and Statistical Anisotropy ab 58.99 € als Taschenbuch: in Cosmological Inflationary Models. Aus dem Bereich: Bücher, Wissenschaft, Physik, Medien > Bücher, LAP Lambert Acad. Publ.<

Nr. 12952216. Versandkosten:, , DE. (EUR 0.00)