Baryogenesis during reheating in natural inflation and comments on spontaneous baryogenesis

被引:69
作者
Dolgov, A
Freese, K
Rangarajan, R
Srednicki, M
机构
[1] UNIV MICHIGAN, DEPT PHYS, ANN ARBOR, MI 48109 USA
[2] HOUSTON ADV RES CTR, ASTROPARTICLE PHYS GRP, THE WOODLANDS, TX 77381 USA
[3] UNIV CALIF SANTA BARBARA, DEPT PHYS, SANTA BARBARA, CA 93106 USA
[4] ITEP, MOSCOW 113259, RUSSIA
关键词
D O I
10.1103/PhysRevD.56.6155
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We calculate the baryon asymmetry created by the decay of a pseudo Nambu-Goldstone boson (PNGB) whose interactions violate baryon number conservation. Our results are in disagreement with previous results in the original spontaneous baryogenesis models for the asymmetry produced by the decay of an oscillating scalar field with B-number-violating derivative couplings; we find that the net baryon number density is proportional to theta(i)(3), where theta(i) is the amplitude of the PNGB field in natural inflation at the onset of reheating. While our calculation of the asymmetry is carried out in the context of natural inflation our approach is generally valid for baryogenesis models using decaying classical fields. We include a complete derivation of the number density of particles produced by the decay of a classical scalar field. [S0556-2821(97)07422-5].
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页码:6155 / 6165
页数:11
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