Gravitational Radiation from Preheating with Many Fields
Parametric resonances provide a mechanism by which particles can be created just after inflation. Thus far, attention has focused on a single or many inflaton fields coupled to a single scalar field. However, generically we expect the inflaton to couple to many other relativistic degrees of freedom present in the early universe. Using simulations in an expanding Friedmann-Lemaître-Robertson-Walker spacetime, in this paper we show how preheating is affected by the addition of multiple fields coupled to the inflaton. We focus our attention on gravitational wave production — an important potential observational signature of the preheating stage. We find that preheating and its gravitational wave signature is robust to the coupling of the inflaton to more matter fields.
Giblin, John T.; Price, Larry R.; and Siemens, Xavier, "Gravitational Radiation from Preheating with Many Fields" (2010). Journal of Cosmology and Astroparticle Physics 2010. Faculty Publications. Paper 174.
Journal of Cosmology and Astroparticle Physics