4.4 Article

Spillway preheating

期刊

JOURNAL OF HIGH ENERGY PHYSICS
卷 -, 期 5, 页码 -

出版社

SPRINGER
DOI: 10.1007/JHEP05(2021)069

关键词

Cosmology of Theories beyond the SM; Beyond Standard Model

资金

  1. DOE [DE-SC-0013607, DE-SC-0010010]
  2. NASA [80NSSC20K0506, 80NSSC18K1010]
  3. US Department of Energy [DE-SC0015655]

向作者/读者索取更多资源

The proposed spillway preheating mechanism can more efficiently dissipate the energy density of the inflaton, using fast perturbative decays of resonantly produced daughter particles to act as a spillway, reducing their backreaction on the inflaton. This leads to a more effective resonant production and a simple inverse power-law scaling in the fraction of energy density remaining in the inflaton.
In traditional models only an order one fraction of energy is transferred from the inflaton to radiation through nonperturbative resonance production in preheating immediately after inflation, due to backreaction effects. We propose a particle production mechanism that could improve the depletion of the inflaton energy density by up to four orders of magnitude. The improvement comes from the fast perturbative decays of resonantly produced daughter particles. They act as a spillway to drain these daughter particles, reducing their backreaction on the inflaton and keeping the resonant production effective for a longer period. Thus we dub the scenario spillway preheating. We also show that the fraction of energy density remaining in the inflaton has a simple inverse power-law scaling in the scenario. In general, spillway preheating is a much more efficient energy dissipation mechanism, which may have other applications in model building for particle physics.

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