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Title: Supersymmetric and smooth hybrid inflation in the light of WMAP3

Abstract

In their minimal form both supersymmetric and smooth hybrid inflation yield a scalar spectral index n{sub s} close to 0.98, to be contrasted with the result n{sub s}=0.951{sub -0.019}{sup +0.015} from WMAP3. To realize better agreement, following Bastero-Gil, King, and Shafi, we extend the parameter space of these models by employing a nonminimal Kaehler potential. We also discuss nonthermal leptogenesis by inflaton decay and obtain new bounds in these models on the reheat temperature to explain the observed baryon asymmetr000.

Authors:
; ;  [1]
  1. Bartol Research Institute, Department of Physics and Astronomy, University of Delaware, Newark, Delaware 19716 (United States)
Publication Date:
OSTI Identifier:
21011065
Resource Type:
Journal Article
Resource Relation:
Journal Name: Physical Review. D, Particles Fields; Journal Volume: 75; Journal Issue: 4; Other Information: DOI: 10.1103/PhysRevD.75.043522; (c) 2007 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; ACCELERATION; ANISOTROPY; ASYMMETRY; BARYONS; COSMOLOGICAL MODELS; COSMOLOGY; PARTICLE PRODUCTION; POTENTIALS; RELICT RADIATION; SUPERGRAVITY; SUPERSYMMETRY

Citation Formats

Rehman, Mansoor ur, Senoguz, V. N., and Shafi, Qaisar. Supersymmetric and smooth hybrid inflation in the light of WMAP3. United States: N. p., 2007. Web. doi:10.1103/PHYSREVD.75.043522.
Rehman, Mansoor ur, Senoguz, V. N., & Shafi, Qaisar. Supersymmetric and smooth hybrid inflation in the light of WMAP3. United States. doi:10.1103/PHYSREVD.75.043522.
Rehman, Mansoor ur, Senoguz, V. N., and Shafi, Qaisar. Thu . "Supersymmetric and smooth hybrid inflation in the light of WMAP3". United States. doi:10.1103/PHYSREVD.75.043522.
@article{osti_21011065,
title = {Supersymmetric and smooth hybrid inflation in the light of WMAP3},
author = {Rehman, Mansoor ur and Senoguz, V. N. and Shafi, Qaisar},
abstractNote = {In their minimal form both supersymmetric and smooth hybrid inflation yield a scalar spectral index n{sub s} close to 0.98, to be contrasted with the result n{sub s}=0.951{sub -0.019}{sup +0.015} from WMAP3. To realize better agreement, following Bastero-Gil, King, and Shafi, we extend the parameter space of these models by employing a nonminimal Kaehler potential. We also discuss nonthermal leptogenesis by inflaton decay and obtain new bounds in these models on the reheat temperature to explain the observed baryon asymmetr000.},
doi = {10.1103/PHYSREVD.75.043522},
journal = {Physical Review. D, Particles Fields},
number = 4,
volume = 75,
place = {United States},
year = {Thu Feb 15 00:00:00 EST 2007},
month = {Thu Feb 15 00:00:00 EST 2007}
}
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