Cosmological problems for the polonyi potential
dc.contributor.author | Coughlan, G. D. | en_US |
dc.contributor.author | Fischler, W. | en_US |
dc.contributor.author | Kolb, Edward W. | en_US |
dc.contributor.author | Raby, Stuart | en_US |
dc.contributor.author | Ross, G. G. | en_US |
dc.date.accessioned | 2006-04-07T18:36:58Z | |
dc.date.available | 2006-04-07T18:36:58Z | |
dc.date.issued | 1983-11-10 | en_US |
dc.identifier.citation | Coughlan, G. D., Fischler, W., Kolb, Edward W., Raby, S., Ross, G. G. (1983/11/10)."Cosmological problems for the polonyi potential." Physics Letters B 131(1-3): 59-64. <http://hdl.handle.net/2027.42/25062> | en_US |
dc.identifier.uri | http://www.sciencedirect.com/science/article/B6TVN-46YMCWH-90/2/cbe7602fdd480e96750fd614da271303 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/25062 | |
dc.description.abstract | We study the cosmological implications of N = 1 supergravity with the Polonyi potential. We find that for typical values of the gravitino mass (102-103 GeV) the universe goes through a late period of reheating (i.e., from a temperature of about 10-7 MeV to 10-2 MeV). Any baryon-to-photon ratio is thus diluted by an unacceptable 15 orders of magnitude, with no hope of regeneration. | en_US |
dc.format.extent | 379171 bytes | |
dc.format.extent | 3118 bytes | |
dc.format.mimetype | application/pdf | |
dc.format.mimetype | text/plain | |
dc.language.iso | en_US | |
dc.publisher | Elsevier | en_US |
dc.title | Cosmological problems for the polonyi potential | en_US |
dc.type | Article | en_US |
dc.rights.robots | IndexNoFollow | en_US |
dc.subject.hlbsecondlevel | Physics | en_US |
dc.subject.hlbsecondlevel | Mathematics | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA | en_US |
dc.contributor.affiliationother | Oxford University, Department of Theoretical Physics, Oxford, England | en_US |
dc.contributor.affiliationother | Department of Physics, University of Pennsylvania, Philadelphia, PA 19104, USA | en_US |
dc.contributor.affiliationother | Theoretical Division, Los Alamos National Laboratory, Los Alamos, NM 87545, USA | en_US |
dc.contributor.affiliationother | Rutherford Laboratory, Chilton, Didcot, England | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/25062/1/0000490.pdf | en_US |
dc.identifier.doi | http://dx.doi.org/10.1016/0370-2693(83)91091-2 | en_US |
dc.identifier.source | Physics Letters B | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
Files in this item
Remediation of Harmful Language
The University of Michigan Library aims to describe library materials in a way that respects the people and communities who create, use, and are represented in our collections. Report harmful or offensive language in catalog records, finding aids, or elsewhere in our collections anonymously through our metadata feedback form. More information at Remediation of Harmful Language.
Accessibility
If you are unable to use this file in its current format, please select the Contact Us link and we can modify it to make it more accessible to you.