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The Origin of Matter in the Universe: Reheating after Inflation
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In the inflationary scenario all the matter constituting the universe was created from the process of reheating after inflation. Recent development of the theory of reheating is briefly reviewed. The list of topics includes elementary (perturbative) theory of reheating; quantum field theory in a time-varying background; parametric resonance and explosive particle creation; non-thermal phase transitions from reheating; baryogenesis from reheating; residual oscillations of the scalar field, and other cosmological applications.
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Cited by 4 Pith papers
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What spectators do during inflation
Spectator-field backreaction during slow-roll inflation changes the inflaton by a factor e^{Υ N_e²}, not the e^{Γ N_e} a local friction term would give.
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Dark Matter as an Inflationary Relic in Warm Inflation
In warm inflation with Υ∝T³, a residual inflaton condensate after rapid drop in Q evolves as cold dark matter with mass fixed at m≈0.02 MeV by the observed abundance.
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The $\alpha$-Attractor E-Model in Warm Inflation: Observational Viability from Planck 2018
The warm α-attractor E-model is claimed to be compatible with Planck 2018 in both weak and strong dissipative regimes, but the strong-regime derivation contains a missing ε² factor that invalidates the predicted tenso...
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Lectures on Reheating after Inflation
Lecture notes providing a generic introduction to reheating after inflation, covering its theoretical, phenomenological, and observational aspects.
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