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Parametric resonance in the early Universe—a fitting analysis
Particle production via parametric resonance in the early Universe, is a nonperturbative, non-linear and out-of-equilibrium phenomenon. Although it is a well studied topic, whenever a new scenario exhibits parametric resonance, a full re-analysis is normally required. To avoid this tedious task, man...
| Autores principales: | , |
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| Lenguaje: | eng |
| Publicado: |
2016
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| Acceso en línea: | https://dx.doi.org/10.1088/1475-7516/2017/02/001 http://cds.cern.ch/record/2216638 |