Supersymmetric inflation, matter and dark energy
King, S.F. (2001) Supersymmetric inflation, matter and dark energy. Pre-print, 1-7. (arXiv:hep-ph/0110385v1).
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Description/Abstract
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.
| Item Type: | Article |
|---|---|
| Additional Information: | Invited talk presented at COSMO-01, Rovaniemi, Finland, August 29-September 4, 2001 |
| Related URLs: | |
| Subjects: | Q Science > QC Physics |
| Divisions: | University Structure - Pre August 2011 > School of Physics and Astronomy |
| Item ID: | 57356 |
| Date Deposited: | 15 Aug 2008 |
| Last Modified: | 02 Mar 2012 12:12 |
| Contributors: | King, S.F. (Author) |
| Date: | 30 October 2001 |
| Additional Information: | Invited talk presented at COSMO-01, Rovaniemi, Finland, August 29-September 4, 2001 |
| Status: | Published |
| URI: | http://eprints.soton.ac.uk/id/eprint/57356 |
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