N-flation in supergravity
We have constructed a large field N-flation model in the supergravity framework. In this simple set-up, N fields collectively drive inflation where each field traverses sub-Planckian field values. This has been realised with a generalisation of the single-field chaotic inflation in supergravity. Int...
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doaj-74d0e349a8b24eb9ade1ceac928a5b902020-11-24T21:32:02ZengElsevierPhysics Letters B0370-26932014-11-01738457463N-flation in supergravityKumar Das0Koushik Dutta1Corresponding author.; Theory Division, Saha Institute of Nuclear Physics, 1/AF Bidhan Nagar, Kolkata 700064, IndiaTheory Division, Saha Institute of Nuclear Physics, 1/AF Bidhan Nagar, Kolkata 700064, IndiaWe have constructed a large field N-flation model in the supergravity framework. In this simple set-up, N fields collectively drive inflation where each field traverses sub-Planckian field values. This has been realised with a generalisation of the single-field chaotic inflation in supergravity. Interestingly, despite the presence of the field interactions, the dynamics can be described in terms of an effective single field. The observable predictions of our model, i.e., tensor-to-scalar ratio r and scalar spectral index ns, are akin to the chaotic inflation.http://www.sciencedirect.com/science/article/pii/S0370269314007370 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Kumar Das Koushik Dutta |
spellingShingle |
Kumar Das Koushik Dutta N-flation in supergravity Physics Letters B |
author_facet |
Kumar Das Koushik Dutta |
author_sort |
Kumar Das |
title |
N-flation in supergravity |
title_short |
N-flation in supergravity |
title_full |
N-flation in supergravity |
title_fullStr |
N-flation in supergravity |
title_full_unstemmed |
N-flation in supergravity |
title_sort |
n-flation in supergravity |
publisher |
Elsevier |
series |
Physics Letters B |
issn |
0370-2693 |
publishDate |
2014-11-01 |
description |
We have constructed a large field N-flation model in the supergravity framework. In this simple set-up, N fields collectively drive inflation where each field traverses sub-Planckian field values. This has been realised with a generalisation of the single-field chaotic inflation in supergravity. Interestingly, despite the presence of the field interactions, the dynamics can be described in terms of an effective single field. The observable predictions of our model, i.e., tensor-to-scalar ratio r and scalar spectral index ns, are akin to the chaotic inflation. |
url |
http://www.sciencedirect.com/science/article/pii/S0370269314007370 |
work_keys_str_mv |
AT kumardas nflationinsupergravity AT koushikdutta nflationinsupergravity |
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1725958818110636032 |