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dc.contributor.authorKane, Gordon L.en_US
dc.contributor.authorKing, S. F.en_US
dc.date.accessioned2006-12-19T19:10:29Z
dc.date.available2006-12-19T19:10:29Z
dc.date.issued2001-11-01en_US
dc.identifier.citationKane, 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.issn1367-2630en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/49052
dc.description.abstractWe 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.extent3118 bytes
dc.format.extent200627 bytes
dc.format.mimetypetext/plain
dc.format.mimetypeapplication/pdf
dc.language.isoen_US
dc.publisherIOP Publishing Ltden_US
dc.titleIntermediate scale supersymmetric inflation, matter and dark energyen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationotherRandall Physics Laboratory, University of Michigan, Ann Arbor, MI 48109-1120, USAen_US
dc.contributor.affiliationotherDepartment of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ, UKen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/49052/2/nj1121.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1088/1367-2630/3/1/321en_US
dc.identifier.sourceNew Journal of Physics.en_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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