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Non-thermal dark matter and the moduli problem in string frameworks

dc.contributor.authorAcharya, Bobby S.en_US
dc.contributor.authorBobkov, Konstantinen_US
dc.contributor.authorKane, Gordon L.en_US
dc.contributor.authorShao, Jingen_US
dc.contributor.authorWatson, Scotten_US
dc.contributor.authorKumar, Piyushen_US
dc.date.accessioned2009-10-08T15:32:58Z
dc.date.available2009-10-08T15:32:58Z
dc.date.issued2008en_US
dc.identifier.citationAcharya, Bobby S.; Bobkov, Konstantin; Kane, Gordon; Shao, Jing; Watson, Scott; Kumar, Piyush (2008). "Non-thermal dark matter and the moduli problem in string frameworks." Journal of High Energy Physics 2008(6):64. <http://hdl.handle.net/2027.42/64181>en_US
dc.identifier.issn1029-8479en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/64181
dc.description.abstract"We address the cosmological moduli/gravitino problems and the issue of too little thermal but excessive non-thermal dark matter from the decays of moduli. The main examples we study are the G2-MSSM models arising from M theory compactifications, which allow for a precise calculation of moduli decay rates and widths. We find that the late decaying moduli satisfy both BBN constraints and avoid the gravitino problem. The non-thermal production of Wino LSPs, which is a prediction of G2-MSSM models, gives a relic density of about the right order of magnitude."en_US
dc.format.extent528364 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.titleNon-thermal dark matter and the moduli problem in string frameworksen_US
dc.typeArticleen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/64181/1/jhep062008_064.pdf
dc.identifier.doihttp://dx.doi.org/10.1088/1126-6708/2008/06/064en_US
dc.identifier.sourceJournal of High Energy Physicsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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