Towards the theory of reheating after inflation

@article{Kofman1997TowardsTT,
  title={Towards the theory of reheating after inflation},
  author={Lev Kofman and Andrei Linde and Alexei A. Starobinsky},
  journal={Physical Review D},
  year={1997},
  volume={56},
  pages={3258-3295}
}
Reheating after inflation occurs due to particle production by the oscillating inflaton field. In this paper we describe the perturbative approach to reheating, and then concentrate on effects beyond the perturbation theory. They are related to the stage of parametric resonance called preheating. It may occur in an expanding universe if the initial amplitude of oscillations of the inflaton field is large enough. We investigate a simple model of a massive inflaton field coupled to another scalar… 
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References

SHOWING 1-8 OF 8 REFERENCES
Particle Physics and Inflationary Cosmology
With the invention of unified theories of strong, weak, electromagnetic and gravitational interactions, elementaryparticle physics has entered a very interesting and unusual stage of its development.
Structure of resonance in preheating after inflation
We consider preheating in the theory $1/4 \lambda \phi^4 + 1/2 g^2\phi^2\chi^2 $, where the classical oscillating inflaton field $\phi$ decays into $\chi$-particles and $\phi$-particles. The
An Introduction To Quantum Field Theory
Feynman Diagrams and Quantum Electrodynamics * Invitation: Pair Production in e+e- Annihilation * The Klein-Gordon Field * The Dirac Field * Interacting Fields and Feynman Diagrams * Elementary
Chaos in Dynamic Systems
Handbook of Mathematical Functions
Quantum Mechanics-Nonrelativistic Theory