Supersymmetric Inflation, Matter and Dark Energy

Details Supersymmetric Inflation, Matter and Dark Energy Supersymmetric Inflation, Matter and Dark Energy

2001-10-30

arxiv.org/abs/hep-ph/0110385v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

Invited talk presented at COSMO-01, Rovaniemi, Finland, August 29-September 4, 2001. 7 pages, Latex

Scientific paper

In this talk, based on \cite{Kane:2001rb}, we emphasise that intermediate scale supersymmetric inflation models are particularly attractive since inflation, baryogenesis and the relic abundance of cold dark matter (CDM) are all related by a set of parameters which also affect particle physics collider phenomena, neutrino masses and the strong CP problem. We also point out that the present day relic abundances of different forms of matter are (in principle) calculable from the supersymmetric inflation model together with a measurement of the CMB temperature and the Hubble constant. From these relic abundances one can deduce the amount of the present day dark energy (DE) density.

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