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Автор John D Barrow
Автор David F Mota
Дата выпуска 2002-12-07
dc.description Assuming a Friedmann universe which evolves with a power-law scale factor, a t <sup>n</sup>, we analyse the phase space of the system of equations that describes a time-varying fine structure constant, α, in the Bekenstein–Sandvik–Barrow–Magueijo generalization of general relativity. We have classified all the possible behaviours of α(t) in ever-expanding universes with different n and find new exact solutions for α(t). We find the attractor points in the phase space for all n. In general, α will be a non-decreasing function of time that increases logarithmically in time during a period when the expansion is dust dominated (n 2/3), but becomes constant when n > 2/3. This includes the case of negative-curvature domination (n 1). α also tends rapidly to a constant when the expansion scale factor increases exponentially. A general set of conditions is established for α to become asymptotically constant at late times in an expanding universe.
Формат application.pdf
Издатель Institute of Physics Publishing
Название Qualitative analysis of universes with varying alpha
Тип paper
DOI 10.1088/0264-9381/19/23/317
Electronic ISSN 1361-6382
Print ISSN 0264-9381
Журнал Classical and Quantum Gravity
Том 19
Первая страница 6197
Последняя страница 6212
Аффилиация John D Barrow; Department of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, UK
Аффилиация David F Mota; Department of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, UK
Выпуск 23

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