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Non-equilibrium dynamics of a scalar field with quantum backreaction

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arxiv 2105.09598 v2 pith:7YSC5AGX submitted 2021-05-20 hep-ph astro-ph.COgr-qchep-th

classification hep-phastro-ph.COgr-qchep-th
keywords effectivefieldmodespotentialscalarbackreactionevolutionfinite
verification ladder T0 review T1 audit T2 compute T3 formal
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We study the dynamical evolution of coupled one- and two-point functions of a scalar field in the 2PI framework at the Hartree approximation, including backreaction from out-of-equilibrium modes. We renormalize the 2PI equations of motion in an on-shell scheme in terms of physical parameters. We present the Hartree-resummed renormalized effective potential at finite temperature and critically discuss the role of the effective potential in a non-equilibrium system. We follow the decay and thermalization of a scalar field from an initial cold state with all energy stored in the potential, into a fully thermalized system with a finite temperature. We identify the non-perturbative processes of parametric resonance and spinodal instability taking place during the reheating stage. In particular we study the unstable modes in the region where the vacuum 1PI effective action becomes complex and show that such spinodal modes can have a dramatic effect on the evolution of the one-point function. Our methods can be easily adapted to simulate reheating at the end of inflation.

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Cited by 3 Pith papers

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

  1. Cosmological phase transitions without high-temperature expansions

    hep-ph 2025-07 conditional novelty 7.0 of 10

    A hard-soft split combined with a finite-temperature Loop-Tree Duality method computes the resummed 4d thermal effective potential without high-temperature expansions, demonstrated in a scalar-Yukawa model.

  2. Consistent Thermal Resummation and Phase Transitions with 2PI Methods

    hep-ph 2026-08 conditional novelty 6.0 of 10

    A 2PI-Hartree effective potential for two mixing scalars is renormalized and used to show that self-consistent thermal resummation can substantially alter predicted phase transition strengths and gravitational wave spectra.

  3. Primordial Gravitational Waves from Phase Transitions during Reheating

    astro-ph.CO 2025-06 conditional novelty 5.0 of 10

    Phase transitions happening during reheating can produce gravitational-wave signals that are delayed, prolonged, and shifted in amplitude and frequency by orders of magnitude compared with standard cosmology.

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