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Robustness of inflation to large tensor perturbations

Abstract:
Extending our previous work on the robustness of inflation to perturbations in the scalar field, we investigate the effects of perturbations in the transverse traceless part of the extrinsic curvature on the evolution of an inhomogeneous inflaton field. Focusing on small field models, we show that these additional metric inhomogeneities initially reduce the total number of e-folds as the amplitude increases, but that the reduction saturates and even reverses above a certain amplitude. We present an argument that this is due to the presence of a large initial Hubble friction when metric perturbations are large.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1088/1475-7516/2018/05/065

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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Sub department:
Astrophysics
Department:
Unknown
Role:
Author


Publisher:
IOP Publishing
Journal:
Journal of Cosmology and Astroparticle Physics More from this journal
Volume:
2018
Issue:
5
Pages:
065-065
Publication date:
2018-05-29
Acceptance date:
2018-05-16
DOI:
ISSN:
1475-7516


Keywords:
Pubs id:
pubs:942609
UUID:
uuid:9a399326-844b-4d64-9faa-49808fe0b66e
Local pid:
pubs:942609
Source identifiers:
942609
Deposit date:
2018-11-15

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