dc.contributor.author | Cincioglu, Elif | |
dc.contributor.author | Solmaz, Levent | |
dc.contributor.author | Demir, Durmus A. | |
dc.contributor.author | SERT, Hale | |
dc.date.accessioned | 2021-12-10T10:19:44Z | |
dc.date.available | 2021-12-10T10:19:44Z | |
dc.date.issued | 2010 | |
dc.identifier.citation | SERT H., Cincioglu E., Demir D. A. , Solmaz L., "Tevatron Higgs mass bounds: Projecting U(1)' models to LHC domain", PHYSICS LETTERS B, cilt.692, sa.5, ss.327-335, 2010 | |
dc.identifier.issn | 0370-2693 | |
dc.identifier.other | av_38fcfab5-b796-4a80-980d-b0c69704a883 | |
dc.identifier.other | vv_1032021 | |
dc.identifier.uri | http://hdl.handle.net/20.500.12627/169680 | |
dc.identifier.uri | https://doi.org/10.1016/j.physletb.2010.08.007 | |
dc.description.abstract | We study Higgs boson masses in supersymmetric models with an extra U(1) symmetry to be called U(1)'. Such extra gauge symmetries are urged by the mu problem of the MSSM, and they also arise frequently in low-energy supersymmetric models stemming from GUTs and strings. | |
dc.language.iso | eng | |
dc.subject | Temel Bilimler | |
dc.subject | Physics and Astronomy (miscellaneous) | |
dc.subject | General Physics and Astronomy | |
dc.subject | Space and Planetary Science | |
dc.subject | Nuclear and High Energy Physics | |
dc.subject | Astronomy and Astrophysics | |
dc.subject | Physical Sciences | |
dc.subject | Astronomi ve Astrofizik | |
dc.subject | Temel Parçacıklar ve Alanlar | |
dc.subject | FİZİK, PARTİKLER VE ALANLAR | |
dc.subject | Fizik | |
dc.subject | FİZİK, NÜKLEER | |
dc.subject | Temel Bilimler (SCI) | |
dc.subject | Uzay bilimi | |
dc.subject | ASTRONOMİ VE ASTROFİZİK | |
dc.title | Tevatron Higgs mass bounds: Projecting U(1)' models to LHC domain | |
dc.type | Makale | |
dc.relation.journal | PHYSICS LETTERS B | |
dc.contributor.department | Izmir Inst Technol , , | |
dc.identifier.volume | 692 | |
dc.identifier.issue | 5 | |
dc.identifier.startpage | 327 | |
dc.identifier.endpage | 335 | |
dc.contributor.firstauthorID | 2750076 | |