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Non-minimal gravitational reheating during kination

2018/03/31 by Konstantinos Dimopoulos, Tommi Markkanen · 2 citations
Mathematics · Physics and Astronomy · #Cosmology and Gravitation Theories #Coupling (piping) #Field (mathematics) #Gravitation #Gravitational field #Inflation (cosmology) #Inflaton #Mathematical and Theoretical Analysis #Relativity and Gravitational Theory #Standard Model (mathematical formulation) #Universe #astro-ph.CO #gr-qc #hep-ph

paper · pdf · doi:10.1088/1475-7516/2018/06/021

published as JCAP06(2018)021 · v3: 19 pages, 2 figures, some improvements, published version

openalex created_date 2018/03/29 · arxiv created 2018/06/12 · openalex publication_date 2018/06/12 · arxiv updated 2018/06/13 · openalex updated_date 2026/08/05

Abstract

A new mechanism is presented which can reheat the Universe in non-oscillatory models of inflation, where the inflation period is followed by a period dominated by the kinetic density for the inflaton field (kination). The mechanism considers an auxiliary field non-minimally coupled to gravity. The auxiliary field is a spectator during inflation, rendered heavy by the non-minimal coupling to gravity. During kination however, the non-minimal coupling generates a tachyonic mass, which displaces the field, until its bare mass becomes important, leading to coherent oscillations. Then, the field decays into the radiation bath of the hot big bang. The model is generic and predictive, in that the resulting reheating temperature is a function only of the model parameters (masses and couplings) and not of initial conditions. It is shown that reheating can be very efficient also when considering only the Standard Model.

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