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• W2019616092 abstract "We investigate a possibility of reheating in a scenario of D-brane inflation in a warped deformed conifold background which includes perturbative corrections to throat geometry sourced by a chiral operator of dimension $3/2$ in the conformal field theory. The effective D-brane potential, in this case, belongs to the class of nonoscillatory models of inflation for which the conventional reheating mechanism does not work. We find that gravitational particle production is inefficient and leads to reheating temperature of the order of ${10}^{8}text{ }text{ }mathrm{GeV}$. We show that instant preheating is quite suitable to the present scenario and can easily reheat the universe to a temperature which is higher by about 3 orders of magnitude than its counterpart associated with gravitational particle production. The reheating temperature is shown to be insensitive to a particular choice of inflationary parameters suitable to observations." @default.
• W2019616092 created "2016-06-24" @default.
• W2019616092 creator A5033062049 @default.
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• W2019616092 date "2010-05-05" @default.
• W2019616092 modified "2023-09-25" @default.
• W2019616092 title "Reheating the D-brane universe via instant preheating" @default.
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• W2019616092 doi "https://doi.org/10.1103/physrevd.81.103506" @default.
• W2019616092 hasPublicationYear "2010" @default.
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