The Standard Big Bang Cosmology
Chapter in Large Scale Structure Formation, Springer Nature 247 (2000) 37-96
A supersymmetric solution to the KARMEN time anomaly
ArXiv hep-ph/9911365 (1999)
Abstract:
We interpret the KARMEN time anomaly as being due to the production of a (dominantly bino) neutralino with mass 33.9 MeV, which is the lightest supersymmetric particle but decays into 3 leptons through the violation of R-parity. For independent gaugino masses M_1 and M_2 we find regions in the (M_1, M_2, mu, tan beta) parameter space where such a light neutralino is consistent with all experiments. Future tests of this hypothesis are outlined.A supersymmetric solution to the KARMEN time anomaly
(1999)
Implementing quadratic supergravity inflation
ArXiv hep-ph/9908380 (1999)
Abstract:
We study inflation driven by a slow-rolling inflaton field, characterised by a quadratic potential, and incorporating radiative corrections within the context of supergravity. In this model the energy scale of inflation is not overly constrained by the requirement of generating the observed level of density fluctuations and can have a physically interesting value, e.g. the supersymmetry breaking scale of $10^{10}$ GeV or the electroweak scale of $10^3$ GeV. In this mass range the inflaton is light enough to be confined at the origin by thermal effects, naturally generating the initial conditions for a (last) stage of inflation of the new inflationary type.Implementing quadratic supergravity inflation
(1999)