Baryogenesis in supergravity inflationary models
NAGIOS: RODERIC FUNCIONANDO

Baryogenesis in supergravity inflationary models

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Baryogenesis in supergravity inflationary models

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Coughlan, G. D.; Ross, Graham G.; Holman, Richard; Ramond, Pierre; Ruiz-Altaba, Martí; Furtado Valle, José Wagner Perfil
This document is a artículoDate1985

Este documento está disponible también en : http://hdl.handle.net/10550/47208
Realistic N=1 supergravity theories with a gravitino mass of order 1 TeV require a period of inflation to dilute the gravitino abundance. Moreover, if the gravitino is unstable the reheat temperature is bounded to be no greater than O(108 GeV). We show that such models may still have acceptable rates of baryosynthesis and discuss possible mechanisms.

    Coughlan, G. D. Ross, Graham G. Holman, Richard Ramond, Pierre Ruiz-Altaba, Martí Furtado Valle, José Wagner 1985 Baryogenesis in supergravity inflationary models Physics Letters B 160 4-5 249 255
http://dx.doi.org/10.1016/0370-2693(85)91320-6

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