Warm inflation and classicality conditions
In this work we analize the classicality conditions that must be satisfied to have an effective stochastic approach, in the framework of warm inflation scenarios. The radiation temperature at the end of inflation is of the order of 1014 GeV, for an scalar field with mass m ∼ (10-4-10-5) Mp, and the...
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| Formato: | JOUR |
| Lenguaje: | English |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_03702693_v428_n1-2_p31_Bellini |
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| Sumario: | In this work we analize the classicality conditions that must be satisfied to have an effective stochastic approach, in the framework of warm inflation scenarios. The radiation temperature at the end of inflation is of the order of 1014 GeV, for an scalar field with mass m ∼ (10-4-10-5) Mp, and the energy fluctuations decreases with the time. © 1998 Published by Elsevier Science B.V. All rights reserved. |
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