Warm inflation and classicality conditions

被引：37

作者：

Bellini, M

机构：

[1] Univ Nacl Mar Del Plata, Fac Ciencias Exactas & Nat, Dept Fis, RA-7600 Mar Del Plata, Buenos Aires, Argentina

[2] Univ Michoacana, Inst Fis & Matemat, Morelia 58060, Michoacan, Mexico

来源：

PHYSICS LETTERS B | 1998年 / 428卷 / 1-2期

关键词：

D O I：

10.1016/S0370-2693(98)00385-2

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 10(14) GeV, for an scalar field with mass m similar to (10(-4)-10(-5)) M-p, and the energy fluctuations decreases with the time. (C) 1998 Published by Elsevier Science B.V. All rights reserved.

引用

页码：31 / 36

页数：6

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