Instant preheating

被引:294
作者
Felder, G [1 ]
Kofman, L
Linde, A
机构
[1] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
[2] Univ Toronto, Canadian Inst Theoret Astrophys, Toronto, ON M5S 1A1, Canada
[3] CEA Saclay, Serv Phys Theor, F-91191 Gif Sur Yvette, France
基金
美国国家科学基金会;
关键词
D O I
10.1103/PhysRevD.59.123523
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We describe a new efficient mechanism of reheating. Immediately after rolling down the rapidly moving inflaton field phi produces particles chi, which may be either bosons or fermions. This is a nonperturbative process which occurs almost instantly; no oscillations or parametric resonance is required. The effective masses of the chi particles may be very small at the moment when they are produced, but they "fatten" when the field phi increases. When the particles chi become sufficiently heavy, they rapidly decay to other, lighter particles. This leads to an almost instantaneous reheating accompanied by the production of particles with masses which may be as large as 10(17)-10(18) GeV. This mechanism works in the usual inflationary models where V(phi) has a minimum, where it takes only a half of a single oscillation of the inflaton field phi, but it is especially efficient in models with effective potentials slowly decreasing at large phi as in the theory of quintessence. [S0556-2821(99)07912-6].
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页数:7
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