Stock Image

Observational Tests of Cosmological Inflation

A. J. Banday

0 ratings by GoodReads
ISBN 10: 079231431X / ISBN 13: 9780792314318
Published by Springer Sep 1991, 1991
New Condition: Neu Buch
From Agrios-Buch (Bergisch Gladbach, Germany)

AbeBooks Seller Since 11 January 2012

Seller Rating 5-star rating

Quantity Available: 1

Available from more sellers

View all  copies of this book
Buy New
List Price:
Price: 284.12 Convert Currency
Shipping: 14.82 From Germany to U.S.A. Destination, Rates & Speeds
Add to basket

Payment Methods
accepted by seller

Visa Mastercard American Express

Check PayPal Invoice Bank/Wire Transfer

About this Item

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 cosmological 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. 483 pp. Englisch. Bookseller Inventory # 9780792314318

Ask Seller a Question

Bibliographic Details

Title: Observational Tests of Cosmological ...

Publisher: Springer Sep 1991

Publication Date: 1991

Binding: Buch

Book Condition:Neu

About this title

Reseña del editor:

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 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.

"About this title" may belong to another edition of this title.