Supersymmetric hybrid inflation with non-minimal Kähler potential
Supersymmetric hybrid inflation with non-minimal Kähler potential
Minimal supersymmetric hybrid inflation based on a minimal Kähler potential predicts a spectral index ns0.98. On the other hand, WMAP three year data prefers a central value ns?0.95. We propose a class of supersymmetric hybrid inflation models based on the same minimal superpotential but with a non-minimal Kähler potential. Including radiative corrections using the one-loop effective potential, we show that the prediction for the spectral index is sensitive to the small non-minimal corrections, and can lead to a significantly red-tilted spectrum, in agreement with WMAP.
345-351
Bastero-Gil, M.
b329c554-20e8-4180-af13-faaa34be2f84
King, S.F.
f8c616b7-0336-4046-a943-700af83a1538
Shafi, Q.
c4e82501-7565-4a39-b584-db15fb35a260
9 August 2007
Bastero-Gil, M.
b329c554-20e8-4180-af13-faaa34be2f84
King, S.F.
f8c616b7-0336-4046-a943-700af83a1538
Shafi, Q.
c4e82501-7565-4a39-b584-db15fb35a260
Bastero-Gil, M., King, S.F. and Shafi, Q.
(2007)
Supersymmetric hybrid inflation with non-minimal Kähler potential.
Physics Letters B, 651 (5-6), .
(doi:10.1016/j.physletb.2006.06.085).
Abstract
Minimal supersymmetric hybrid inflation based on a minimal Kähler potential predicts a spectral index ns0.98. On the other hand, WMAP three year data prefers a central value ns?0.95. We propose a class of supersymmetric hybrid inflation models based on the same minimal superpotential but with a non-minimal Kähler potential. Including radiative corrections using the one-loop effective potential, we show that the prediction for the spectral index is sensitive to the small non-minimal corrections, and can lead to a significantly red-tilted spectrum, in agreement with WMAP.
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Published date: 9 August 2007
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Local EPrints ID: 57041
URI: http://eprints.soton.ac.uk/id/eprint/57041
ISSN: 0370-2693
PURE UUID: 23a1accf-6f1e-4e7a-a19f-8b7f01797565
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Date deposited: 13 Aug 2008
Last modified: 15 Mar 2024 11:04
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Author:
M. Bastero-Gil
Author:
Q. Shafi
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