English

Characterizing the post-inflationary reheating history, Part II: Multiple interacting daughter fields

Cosmology and Nongalactic Astrophysics 2023-02-15 v2 High Energy Physics - Phenomenology High Energy Physics - Theory

Abstract

We characterize the post-inflationary dynamics of an inflaton ϕ\phi coupled to multiple interacting daughter fields XnX_n (n=1,Ndn=1,\dots N_d) through quadratic-quadratic interactions gn2ϕ2Xn2g_n^ 2\phi^2 X_n^2. We assume a monomial inflaton potential V(ϕ)ϕpV(\phi) \propto |\phi|^p (p2p \geq 2) around the minimum. By simulating the system in 2+1-dimensional lattices, we study the post-inflationary evolution of the energy distribution and equation of state, from the end of inflation until a stationary regime is achieved. We show that in this scenario, the energy transferred to the daughter field sector can be larger than 50%50\%, surpassing this way the upper bound found previously for single daughter field models. In particular, for p4p \geq 4 the energy at very late times is equally distributed between all fields, and only 100/(Nd+1)%100/(N_d + 1) \% of the energy remains in the inflaton. We also consider scenarios in which the daughter fields have scale-free interactions λnmXn2Xm2\lambda_{nm} X_n^2 X_m^2, including the case of quartic daughter field self-interactions (for n=mn=m). We show that these interactions trigger a resonance process during the non-linear regime, which in the single daughter field case already allows to deplete more than 50%50\% of the energy from the inflaton for p4p\geq 4.

Keywords

Cite

@article{arxiv.2206.06319,
  title  = {Characterizing the post-inflationary reheating history, Part II: Multiple interacting daughter fields},
  author = {Stefan Antusch and Kenneth Marschall and Francisco Torrenti},
  journal= {arXiv preprint arXiv:2206.06319},
  year   = {2023}
}

Comments

23 pages + appendix, 15 figures