DC Field | Value | Language |
---|---|---|
dc.contributor.author | Lee, Hye-Sung | ko |
dc.date.accessioned | 2017-10-23T02:02:25Z | - |
dc.date.available | 2017-10-23T02:02:25Z | - |
dc.date.created | 2017-10-11 | - |
dc.date.created | 2017-10-11 | - |
dc.date.created | 2017-10-11 | - |
dc.date.issued | 2008-12 | - |
dc.identifier.citation | MODERN PHYSICS LETTERS A, v.23, no.39, pp.3271 - 3283 | - |
dc.identifier.issn | 0217-7323 | - |
dc.identifier.uri | http://hdl.handle.net/10203/226500 | - |
dc.description.abstract | Supersymmetry is one of the best motivated new physics scenarios. To build a realistic supersymmetric standard model, however,a companion symmetry is necessary to address various issues. While R-parity is a popular candidate that can address the proton and dark matter issues simultaneously, it is not the only option for such a property. We review how a TeV scale U(1)' gauge symmetry can replace the R-parity. Discrete symmetries of the U(1)' can make the model still viable and attractive with distinguishable phenomenology. For instance, with a residual discrete symmetry of the U(1)', Z(6) = B-3 x U-2, the proton can be protected by the baryon triality (B-3) and a hidden sector dark matter candidate can be protected by the U-parity (U-2). | - |
dc.language | English | - |
dc.publisher | WORLD SCIENTIFIC PUBL CO PTE LTD | - |
dc.title | R-PARITY VIOLATING U(1)'-EXTENDED SUPERSYMMETRIC STANDARD MODEL | - |
dc.type | Article | - |
dc.identifier.wosid | 000262615500001 | - |
dc.type.rims | ART | - |
dc.citation.volume | 23 | - |
dc.citation.issue | 39 | - |
dc.citation.beginningpage | 3271 | - |
dc.citation.endingpage | 3283 | - |
dc.citation.publicationname | MODERN PHYSICS LETTERS A | - |
dc.contributor.localauthor | Lee, Hye-Sung | - |
dc.description.isOpenAccess | N | - |
dc.type.journalArticle | Review | - |
dc.subject.keywordAuthor | Supersymmetry | - |
dc.subject.keywordAuthor | R-parity violation | - |
dc.subject.keywordAuthor | darkmatter | - |
dc.subject.keywordPlus | CHANGING NEUTRAL CURRENTS | - |
dc.subject.keywordPlus | MU-PROBLEM | - |
dc.subject.keywordPlus | Z&apos | - |
dc.subject.keywordPlus | MODELS | - |
dc.subject.keywordPlus | CONSERVATION | - |
dc.subject.keywordPlus | SYMMETRIES | - |
dc.subject.keywordPlus | BREAKING | - |
dc.subject.keywordPlus | DECAYS | - |
dc.subject.keywordPlus | MASSES | - |
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