Intermediate scale supersymmetric inflation, matter and dark energy
dc.contributor.author | Kane, Gordon L. | en_US |
dc.contributor.author | King, Stephen F. | en_US |
dc.date.accessioned | 2006-12-19T19:10:29Z | |
dc.date.available | 2006-12-19T19:10:29Z | |
dc.date.issued | 2001-11-01 | en_US |
dc.identifier.citation | Kane, G L; King, S F (2001). "Intermediate scale supersymmetric inflation, matter and dark energy." New Journal of Physics. 3(1): 21.1-21.5. <http://hdl.handle.net/2027.42/49052> | en_US |
dc.identifier.issn | 1367-2630 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/49052 | |
dc.description.abstract | We consider supersymmetric inflation models in which inflation occurs at an intermediate scale and which provide a solution to the µ problem and the strong CP problem. Such models are particularly attractive since inflation, baryogenesis and the relic abundance of cold dark matter are all related by a set of parameters which also affect particle physics collider phenomena, neutrino masses and the strong CP problem. For such models the natural situation is a universe containing matter composed of baryons, massive neutrinos, lightest superpartner cold dark matter and axions. The present-day relic abundances of these different forms of matter are (in principle) calculable from the supersymmetric inflation model together with a measurement of the cosmic microwave background temperature and the Hubble constant. From these relic abundances one can deduce the amount of the present-day dark energy density. | en_US |
dc.format.extent | 3118 bytes | |
dc.format.extent | 200627 bytes | |
dc.format.mimetype | text/plain | |
dc.format.mimetype | application/pdf | |
dc.language.iso | en_US | |
dc.publisher | IOP Publishing Ltd | en_US |
dc.title | Intermediate scale supersymmetric inflation, matter and dark energy | en_US |
dc.type | Article | en_US |
dc.subject.hlbsecondlevel | Physics | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationother | Randall Physics Laboratory, University of Michigan, Ann Arbor, MI 48109-1120, USA | en_US |
dc.contributor.affiliationother | Department of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ, UK | en_US |
dc.contributor.affiliationumcampus | Ann Arbor | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/49052/2/nj1121.pdf | en_US |
dc.identifier.doi | http://dx.doi.org/10.1088/1367-2630/3/1/321 | en_US |
dc.identifier.source | New Journal of Physics. | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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