pith. sign in

arxiv: 1502.02475 · v2 · pith:WFKFR5IFnew · submitted 2015-02-09 · ✦ hep-ph · astro-ph.CO

Gravitational Effects on Inflaton Decay

classification ✦ hep-ph astro-ph.CO
keywords inflatondecaygravitonhubbleinflationjustnon-minimaloscillation
0
0 comments X
read the original abstract

We point out that the inflaton inevitably couples to all non-conformally coupled matters gravitationally through an oscillation in the Hubble parameter or the cosmic scale factor. It leads to particle production during the inflaton oscillation regime, which is most efficient just after inflation. Moreover, the analysis is extended to the model with non-minimal inflaton couplings to gravity, in which the Hubble parameter oscillates more violently. We apply our results to the graviton production by the inflaton: gravitons are also produced just after inflation, but the non-minimal coupling does not induce inflaton decay into the graviton pair.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. A Unified Bogoliubov Approach to Primordial Gravitational Waves: From Inflation to Reheating

    hep-ph 2026-04 unverdicted novelty 6.0

    An improved Bogoliubov numerical method computes the full primordial GW spectrum from inflation to reheating and shows that inflaton anharmonicity imprints distinctive features at high frequencies.

  2. Graviton Production from Inflaton Condensate: Boltzmann vs Bogoliubov

    hep-ph 2026-04 unverdicted novelty 6.0

    For quadratic inflaton potentials Boltzmann and Bogoliubov spectra agree at short wavelengths, but for steeper potentials non-adiabatic transition effects captured only by Bogoliubov are sizable across a broad momentum range.

  3. Probing Bose-enhanced Inflaton Decay with Gravitational Waves

    hep-ph 2026-01 unverdicted novelty 5.0

    Bose enhancement from a transient condensate of inflaton decay products dramatically increases decay efficiency and amplifies stochastic gravitational wave production to potentially observable levels.

  4. High Frequency Spectrum of Primordial Gravitational Waves

    hep-ph 2026-01 unverdicted novelty 5.0

    High-frequency primordial gravitational waves extend to higher frequencies due to post-inflation inflaton dynamics, and their detailed spectrum shape can distinguish inflation models.

  5. CMB signatures of gravity-mediated dark radiation in $\mathbf{\Delta N_{\rm eff}}$

    hep-ph 2026-04 unverdicted novelty 4.0

    Gravity-mediated production of scalar and vector dark radiation yields Planck 2018 constraints on reheating temperature T_RH and background equation of state w_Φ, with comparisons to right-handed neutrinos, ALPs, and ...