Reheating of the Universe and evolution of the inflaton
The problem of the reheating of the Universe after inflation is considered. Our approach is based on the use, as "first principles," of the renormalized version of (a) the evolution equation for the mean value of an interacting scalar field and (b) the semiclassical Einstein equations. We...
Guardado en:
| Publicado: |
1989
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v40_n4_p955_Mazzitelli http://hdl.handle.net/20.500.12110/paper_05562821_v40_n4_p955_Mazzitelli |
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