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Centro de Ciencias Matemáticas UNAM

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Type: Article

Inflationary attractors and their measures

Abstract:

Several recent misconceptions about the measure problem in inflation and the nature of inflationary attractors are addressed. We clarify some issues regarding the Hamiltonian dynamics of a flat Friedmann-Lemaitre-Robertson-Walker cosmology coupled to a massive scalar field. In particular we show that the focusing of the Liouville measure on attractor solutions is recovered by properly dealing with a gauge degree of freedom related to the rescaling of the spatial volume. Furthermore, we show how the Liouville measure formulated on a surface of constant Hubble rate, together with the assumption of constant a priory probability, induces a non-uniform probability distribution function on any other surfaces of other Hubble rates. The attractor behaviour is seen through the focusing of this function on a narrow range of physical observables. This qualitative behaviour is robust under change of potential and underlying measure. One can then conclude that standard techniques from Hamiltonian dynamics suffice to provide a satisfactory description of attractor solutions and the measure problem for inflationary dynamics.
Keywords: Loop Quantum Cosmology
MSC: 60E05; 83C45; 83F05
Journal: Classical and Quantum Gravity
ISSN: 0264-9381
Year: 2014
Volume: 31
Number: 6
Pages: 62001-62001
MR Number: 3176055
Revision: 1
Notas: Accession Number: CCC:000332207100001
Created Created: 2014-04-07 10:21:06
Modified Modified: 2015-03-17 13:26:23
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