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Автор Bartjan van Tent
Дата выпуска 2004-01-21
dc.description In this paper, we investigate some consequences of multiple-field inflation for the cosmic microwave background radiation (CMB). We derive expressions for the amplitudes, the spectral indices and the derivatives of the indices of the CMB power spectrum in the context of a very general multiple-field theory of slow-roll inflation, where the field metric can be non-trivial. Both scalar (adiabatic, isocurvature and mixing) and tensor perturbations are treated and the differences with single-field inflation are discussed. From these expressions, several relations are derived that can be used to determine the importance of multiple-field effects observationally from the CMB. We also study the evolution of the total entropy perturbation during radiation and matter domination and the influence of this on the isocurvature spectral quantities.
Формат application.pdf
Издатель Institute of Physics Publishing
Копирайт 2004 IOP Publishing Ltd
Название Multiple-field inflation and the CMB
Тип paper
DOI 10.1088/0264-9381/21/2/002
Electronic ISSN 1361-6382
Print ISSN 0264-9381
Журнал Classical and Quantum Gravity
Том 21
Первая страница 349
Последняя страница 369
Аффилиация Bartjan van Tent; Institute for Theoretical Physics, University of Amsterdam, Valckenierstraat 65, 1018 XE Amsterdam, The Netherlands
Выпуск 2

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