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General Relativistic effects in preheating

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arxiv hep-ph/9808404 v3 pith:2X334Y2L submitted 1998-08-25 hep-ph astro-phgr-qchep-th

General Relativistic effects in preheating

classification hep-ph astro-phgr-qchep-th
keywords effectsgravitationalmetricfieldfluctuationsgeneralperturbationspreheating
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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General relativistic effects in the form of metric perturbations are usually neglected in the preheating era that follows inflation. We argue that in realistic multi-field models these effects are in fact crucial, and the fully coupled system of metric and quantum field fluctuations needs to be considered. Metric perturbations are resonantly amplified, breaking the scale-invariance of the primordial spectrum, and in turn stimulate scalar field resonances via gravitational rescattering. This non-gravitationally dominated nonlinear growth of gravitational fluctuations may have significant effects on the Doppler peaks in the cosmic background radiation, primordial black hole formation, gravitational waves and nonthermal symmetry restoration.

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Cited by 2 Pith papers

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    astro-ph.CO 2026-07 accept novelty 6.0

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  2. The art of simulating the early Universe. Part III: Scalar-Gauge-Fluid Dynamics

    astro-ph.CO 2026-07 accept novelty 5.0

    Detailed continuum-to-lattice schemes are given for perfect/imperfect fluids alone or coupled to scalars/gauges in FLRW, enabling self-consistent CosmoLattice simulations of early-Universe plasma dynamics and GWs.