Initial Conditions for Supersymmetric Inflation

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dc.creatorLazarides, G.
dc.creatorVlachos, N. D.
dc.date1997-07-09
dc.date.accessioned2026-07-07T11:35:23Z
dc.date.available2026-07-07T11:35:23Z
dc.descriptionWe perform a numerical investigation of the fields evolution in the supersymmetric inflationary model based on radiative corrections. Supergravity corrections are also included. We find that, out of all the examined initial data, only about 10% give an adequate amount of inflation and can be considered as ''natural''. Moreover, these successful initial conditions appear scattered and more or less isolated.
dc.description15 pages RevTeX 4 eps figures
dc.identifierhttps://arxiv.org/abs/hep-ph/9707296
dc.identifierhttp://arxiv.org/abs/hep-ph/9707296
dc.identifierPhys.Rev.D56:4562-4567,1997
dc.identifierdoi:10.1103/PhysRevD.56.4562
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198576
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleInitial Conditions for Supersymmetric Inflation
dc.typetext

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