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dc.contributor.authorCheung, Clifford
dc.contributor.authorNomura, Yasunori
dc.contributor.authorThaler, Jesse
dc.date.accessioned2011-06-17T16:45:37Z
dc.date.available2011-06-17T16:45:37Z
dc.date.issued2010-03
dc.date.submitted2010-02
dc.identifier.issn1029-8479
dc.identifier.urihttp://hdl.handle.net/1721.1/64478
dc.description.abstractSupersymmetric phenomenology has been largely bound to the hypothesis that supersymmetry breaking originates from a single source. In this paper, we relax this underlying assumption and consider a multiplicity of sectors which independently break supersymmetry, thus yielding a corresponding multiplicity of goldstini. While one linear combination of goldstini is eaten via the super-Higgs mechanism, the orthogonal combinations remain in the spectrum as physical degrees of freedom. Interestingly, supergravity effects induce a universal tree-level mass for the goldstini which is exactly twice the gravitino mass. Since visible sector fields can couple dominantly to the goldstini rather than the gravitino, this framework allows for substantial departures from conventional supersymmetric phenomenology. In fact, this even occurs when a conventional mediation scheme is augmented by additional supersymmetry breaking sectors which are fully sequestered. We discuss a number of striking collider signatures, including various novel decay modes for the lightest observable-sector supersymmetric particle, gravitinoless gauge-mediated spectra, and events with multiple displaced vertices. We also describe goldstini cosmology and the possibility of goldstini dark matter.en_US
dc.description.sponsorshipUnited States. Dept. of Energy (Contract No. DE-AC02-05CH11231)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant No. PHY-0555661)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant No. PHY-0855653)en_US
dc.description.sponsorshipUnited States. Dept. of Energy (DE-FG0205ER41360)en_US
dc.language.isoen_US
dc.publisherSpringer Berlin / Heidelbergen_US
dc.relation.isversionofhttp://dx.doi.org/10.1007/jhep03(2010)073en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alike 3.0en_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/en_US
dc.sourceProf. Thaler via Mat Willmotten_US
dc.titleGoldstinien_US
dc.typeArticleen_US
dc.identifier.citationCheung, Clifford, Yasunori Nomura, and Jesse Thaler. “Goldstini.” Journal of High Energy Physics 2010.3 (2010) : 1-27-27.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.approverThaler, Jesse
dc.contributor.mitauthorThaler, Jesse
dc.relation.journalJournal of High Energy Physicsen_US
dc.eprint.versionAuthor's final manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsCheung, Clifford; Nomura, Yasunori; Thaler, Jesseen
dc.identifier.orcidhttps://orcid.org/0000-0002-2406-8160
mit.licenseOPEN_ACCESS_POLICYen_US
mit.metadata.statusComplete


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