Scalar Field Equations from Quantum Gravity during Inflation

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dc.creatorKahya, E. O.
dc.creatorWoodard, R. P.
dc.date2007-10-28
dc.date.accessioned2026-07-07T11:12:42Z
dc.date.available2026-07-07T11:12:42Z
dc.descriptionWe exploit a previous computation of the self-mass-squared from quantum gravity to include quantum corrections to the scalar evolution equation. The plane wave mode functions are shown to receive no significant one loop corrections at late times. This result probably applies as well to the inflaton of scalar-driven inflation. If so, there is no significant correction to the $ϕϕ$ correlator that plays a crucial role in computations of the power spectrum.
dc.description19 pages, 5 tables
dc.identifierhttps://arxiv.org/abs/0710.5282
dc.identifierhttp://arxiv.org/abs/0710.5282
dc.identifierPhys.Rev.D77:084012,2008
dc.identifierdoi:10.1103/PhysRevD.77.084012
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191468
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleScalar Field Equations from Quantum Gravity during Inflation
dc.typetext

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