中文

Brane preheating

高能物理 - 唯象学 2009-10-31 v1 天体物理学 广义相对论与量子宇宙学 高能物理 - 理论

摘要

We study brane-world preheating in massive chaotic inflationary scenario where scalar fields are confined on the 3-brane. Assuming that quadratic contribution in energy densities dominates the Hubble expansion rate during preheating, the amplitude of inflaton decreases slowly relative to the standard dust-dominated case. This leads to an efficient production of χ\chi particles via nonperturbative decay of inflaton even if its coupling is of order g=105g=10^{-5}. We also discuss massive particle creation heavier than inflaton, which may play important roles for the baryo- and lepto-genesis scenarios.

关键词

引用

@article{arxiv.hep-ph/0012141,
  title  = {Brane preheating},
  author = {Shinji Tsujikawa and Kei-ichi Maeda and Shuntaro Mizuno},
  journal= {arXiv preprint arXiv:hep-ph/0012141},
  year   = {2009}
}

备注

6 pages, 2 figures, submitted to Physical Review D