9789401055529 - observational tests of cosmological inflation: 348 (17 risultati)

Observational Tests of Cosmological Inflation
Shanks, T. (EDT); Banday, A. J. (EDT); Ellis, Richard S. (EDT); Frenk, Carlos S. (EDT); Wolfendale, A. W. (EDT)
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Observational Tests of Cosmological Inflation
Shanks, T. (EDT); Banday, A. J. (EDT); Ellis, Richard S. (EDT); Frenk, Carlos S. (EDT); Wolfendale, A. W. (EDT)
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Taschenbuch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - This book represents the proceedings from the NATO sponsored Advanced Research Workshop entitled 'Observational Tests of Inflation' held at the University of Durham, England on the 10th-14th December, 1990. In recent years, the cosmological inflat…ion model has drawn together the worlds of particle physics, theoretical cosmology and observational astronomy. The aim of the workshop was to bring together experts in all of these fields to discuss the current status of the inflation theory and its observational predictions. The simplest inflation model makes clear predictions which are testable by astronomical observation. Foremost is the prediction that the cosmological density parameter, no, should have a value negligibly different from the critical, Einstein-de Sitter value of 00=1. The other main prediction is that the spectrum of primordial density fluctuations should be Gaussian and take the Harrison-Zeldovich form. The prediction that n =l, in patticular, leads to several important consequences o for cosmology. Firstly, there is the apparent contradiction with the limits on baryon density from Big Bang nucleosynthesis which has led to the common conjecture that weakly interacting particles rather than baryons may form the dominant mass constituent of the Universe. Secondly, with n =l, the age of the Universe is uncomfortably short if o the Hubble constant and the ages of the oldest star clusters lie within their currently believed limits.

Observational Tests of Cosmological Inflation (Nato Science Series C: (closed))
Shanks, T. (Editor) / Banday, A.J. (Editor) / Ellis, Richard S. (Editor) / Frenk, Carlos S. (Editor) / Wolfendale, A.W. (Editor)
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Observational Tests of Cosmological Inflation
Shanks, T. (EDT); Banday, A. J. (EDT); Ellis, Richard S. (EDT); Frenk, Carlos S. (EDT); Wolfendale, A. W. (EDT)
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Observational Tests of Cosmological Inflation
Shanks, T. (EDT); Banday, A. J. (EDT); Ellis, Richard S. (EDT); Frenk, Carlos S. (EDT); Wolfendale, A. W. (EDT)
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Observational Tests of Cosmological Inflation
Shanks, T.|Banday, A. J.|Ellis, Richard S.|Frenk, Carlos S.|Wolfendale, A. W.
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Condizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Proceedings of the NATO Advanced Research Workshop on Observational Tests of Inflation, Durham, U.K., December 10-14, 1990 This book represents the proceedings from the NATO sponsored Advanced Research Workshop entit…led Observational Tests of Inflatio.
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Taschenbuch. Condizione: Neu. Observational Tests of Cosmological Inflation | T. Shanks (u. a.) | Taschenbuch | xx | Englisch | 2012 | Springer | EAN 9789401055529 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu Print on D…emand.

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Taschenbuch. Condizione: Neu. This item is printed on demand - Print on Demand Titel. Neuware -This book represents the proceedings from the NATO sponsored Advanced Research Workshop entitled 'Observational Tests of Inflation' held at the University of Durham, England on the 10th-14th December, 1990. In recent years, the cosmolo…gical inflation model has drawn together the worlds of particle physics, theoretical cosmology and observational astronomy. The aim of the workshop was to bring together experts in all of these fields to discuss the current status of the inflation theory and its observational predictions. The simplest inflation model makes clear predictions which are testable by astronomical observation. Foremost is the prediction that the cosmological density parameter, no, should have a value negligibly different from the critical, Einstein-de Sitter value of 00=1. The other main prediction is that the spectrum of primordial density fluctuations should be Gaussian and take the Harrison-Zeldovich form. The prediction that n =l, in patticular, leads to several important consequences o for cosmology. Firstly, there is the apparent contradiction with the limits on baryon density from Big Bang nucleosynthesis which has led to the common conjecture that weakly interacting particles rather than baryons may form the dominant mass constituent of the Universe. Secondly, with n =l, the age of the Universe is uncomfortably short if o the Hubble constant and the ages of the oldest star clusters lie within their currently believed limits.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 508 pp. Englisch.

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Condizione: New. Print on Demand pp. 508 49:B&W 6.14 x 9.21 in or 234 x 156 mm (Royal 8vo) Perfect Bound on White w/Gloss Lam.

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Taschenbuch. Condizione: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -This book represents the proceedings from the NATO sponsored Advanced Research Workshop entitled 'Observational Tests of Inflation' held at the University of Durham, England on the 10th-14th December, 1990. In recent years, the cos…mological inflation model has drawn together the worlds of particle physics, theoretical cosmology and observational astronomy. The aim of the workshop was to bring together experts in all of these fields to discuss the current status of the inflation theory and its observational predictions. The simplest inflation model makes clear predictions which are testable by astronomical observation. Foremost is the prediction that the cosmological density parameter, no, should have a value negligibly different from the critical, Einstein-de Sitter value of 00=1. The other main prediction is that the spectrum of primordial density fluctuations should be Gaussian and take the Harrison-Zeldovich form. The prediction that n =l, in patticular, leads to several important consequences o for cosmology. Firstly, there is the apparent contradiction with the limits on baryon density from Big Bang nucleosynthesis which has led to the common conjecture that weakly interacting particles rather than baryons may form the dominant mass constituent of the Universe. Secondly, with n =l, the age of the Universe is uncomfortably short if o the Hubble constant and the ages of the oldest star clusters lie within their currently believed limits. 508 pp. Englisch.