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High-frequency Graviton from Inflaton Oscillation

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arxiv 2006.09972 v1 pith:A4NE5H7P submitted 2020-06-17 astro-ph.CO hep-ph

High-frequency Graviton from Inflaton Oscillation

classification astro-ph.CO hep-ph
keywords inflatongravitonhigh-frequencyoscillationamplifiedbackgroundcoherentcomes
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We point out that there is a high-frequency tail of the stochastic inflationary gravitational wave background that scales as $f^{-1/2}$ with frequency $f$. This contribution comes from the graviton vacuum fluctuation amplified by the inflaton coherent oscillation during the reheating stage. It contains information on inflaton properties such as the inflaton mass as well as the thermal history of the early Universe.

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Cited by 9 Pith papers

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

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  3. 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.

  4. Graviton Production from Inflaton Condensate: Boltzmann vs Bogoliubov

    hep-ph 2026-04 accept novelty 6.0

    For n=2 inflaton potentials Boltzmann and Bogoliubov agree on short-wavelength gravitons; for n>2 the non-adiabatic transition dominates and requires the Bogoliubov formalism.

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    hep-ph 2026-04 unverdicted novelty 6.0

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    hep-ph 2026-05 unverdicted novelty 5.0

    Perturbative inflaton decay emits an irreducible stochastic GW background with Ω_GW ∝ f spectrum whose amplitude is set by the hard decay rate and reaches O(10^{-17}) at GHz scales.

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