dc.contributorUniversidade Estadual Paulista (UNESP)
dc.creatorNastase, Horatiu
dc.creatorWeltman, Amanda
dc.date2014-05-27T11:30:45Z
dc.date2016-10-25T18:54:30Z
dc.date2014-05-27T11:30:45Z
dc.date2016-10-25T18:54:30Z
dc.date2013-09-30
dc.date.accessioned2017-04-06T02:40:01Z
dc.date.available2017-04-06T02:40:01Z
dc.identifierJournal of High Energy Physics, v. 2013, n. 8, 2013.
dc.identifier1126-6708
dc.identifier1029-8479
dc.identifierhttp://hdl.handle.net/11449/76658
dc.identifierhttp://acervodigital.unesp.br/handle/11449/76658
dc.identifier10.1007/JHEP08(2013)059
dc.identifierWOS:000324113700059
dc.identifier2-s2.0-84884561511.pdf
dc.identifier2-s2.0-84884561511
dc.identifierhttp://dx.doi.org/10.1007/JHEP08(2013)059
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/897350
dc.descriptionWe modify the ansatz for embedding chameleon scalars in string theory proposed in [1] by considering a racetrack superpotential with two KKLT-type exponentials e ia instead of one. This satisfies all experimental constraints, while also allowing for the chameleon to be light enough on cosmological scales to be phenomenologically interesting. © 2013 SISSA, Trieste, Italy.
dc.languageeng
dc.relationJournal of High Energy Physics
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectCosmology of Theories beyond the SM
dc.subjectdS vacua in string theory
dc.subjectSupergravity Models
dc.titleChameleons on the racetrack
dc.typeOtro


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