Abstract
We study brane-world preheating in a massive chaotic inflationary scenario where Scalar fields are confined on the three-brane. Assuming that the quadratic contribution in energy densities dominates the Hubble expansion rate during preheating, the amplitude of the inflaton decreases slowly relative to the standard dust-dominated case. This leads to an efficient production of X particles via the nonperturbative decay of the inflaton even if its coupling is of the order of g = 10-5. We also discuss massive particle creation heavier than the inflaton, which may play an important role for baryogenesis and leptogenesis scenarios.
| Original language | English |
|---|---|
| Article number | 123511 |
| Pages (from-to) | 1235111-1235115 |
| Number of pages | 5 |
| Journal | Physical Review D - Particles, Fields, Gravitation and Cosmology |
| Volume | 63 |
| Issue number | 12 |
| Publication status | Published - 2001 Aug 15 |
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ASJC Scopus subject areas
- Nuclear and High Energy Physics
- Physics and Astronomy (miscellaneous)
Cite this
Tsujikawa, S., Maeda, K. I., & Mizuno, S. (2001). Brane preheating. Physical Review D - Particles, Fields, Gravitation and Cosmology, 63(12), 1235111-1235115. [123511].