Cosmological evolution of the rolling tachyon

被引:513
作者
Gibbons, GW [1 ]
机构
[1] Univ Cambridge, CMS, DAMTP, Cambridge CB3 0WA, England
关键词
D O I
10.1016/S0370-2693(02)01881-6
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The cosmological effects of the tachyon rolling down to its ground state are discussed by coupling a simple effective field theory for the tachyon field to Einstein gravity. As the tachyon rolls down to the minimum of its potential the universe expands. Depending upon initial conditions, the scale factor may or may not start off accelerating. but ultimately it ceases to do so and the final flat spacetime is either static in the rest frame of the tachyon (if k=0) or (if k = -1) given by the Milne model. (C) 2002 Elsevier Science B.V. All rights reserved.
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页码:1 / 4
页数:4
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