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DC Field | Value | Language |
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dc.contributor.author | Datta, Amitava | - |
dc.contributor.author | Datta, Aseshkrishna | - |
dc.contributor.author | Drees, Manuel | - |
dc.contributor.author | Roy, D. P. | - |
dc.date.accessioned | 2014-05-27T11:19:53Z | - |
dc.date.accessioned | 2016-10-25T18:16:18Z | - |
dc.date.available | 2014-05-27T11:19:53Z | - |
dc.date.available | 2016-10-25T18:16:18Z | - |
dc.date.issued | 2000-03-01 | - |
dc.identifier | http://dx.doi.org/10.1103/PhysRevD.61.055003 | - |
dc.identifier.citation | Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 61, n. 5, p. 1-9, 2000. | - |
dc.identifier.issn | 0556-2821 | - |
dc.identifier.issn | 1550-7998 | - |
dc.identifier.uri | http://hdl.handle.net/11449/66110 | - |
dc.identifier.uri | http://acervodigital.unesp.br/handle/11449/66110 | - |
dc.description.abstract | We study signals for the production of superparticles at the Fermilab Tevatron in supergravity scenarios based on the grand unified group SO(10). The breaking of this group introduces extra contributions to the masses of all scalars, described by a single new parameter. We find that varying this parameter can considerably change the size of various expected signals studied in the literature, with different numbers of jets and/or charged leptons in the final state. The ratios of these signals can thus serve as a diagnostic to detect or constrain deviations from the much-studied scenario where all scalar masses are universal at the GUT scale. Moreover, under favorable circumstances some of these signals, and/or new signals involving hard b jets, should be observable at the next run of the Fermilab Tevatron collider even if the average scalar mass lies well above the gluino mass. ©2000 The American Physical Society. | en |
dc.format.extent | 1-9 | - |
dc.language.iso | eng | - |
dc.source | Scopus | - |
dc.title | Effects of SO(10) D terms on SUSY signals at the Fermilab Tevatron | en |
dc.type | outro | - |
dc.contributor.institution | Jadavpur University | - |
dc.contributor.institution | Mehta Research Institute | - |
dc.contributor.institution | Universidade Estadual Paulista (UNESP) | - |
dc.contributor.institution | Tata Inst. of Fundamental Research | - |
dc.description.affiliation | Department of Physics Jadavpur University, Calcutta 700 032 | - |
dc.description.affiliation | Mehta Research Institute, Chhatnag Road, Jhusi; Allahabad 211 019 | - |
dc.description.affiliation | IFT Universidad Estadual Paulista, 01405-900 São Paulo | - |
dc.description.affiliation | Tata Inst. of Fundamental Research, Mumbai 400 005 | - |
dc.description.affiliationUnesp | IFT Universidad Estadual Paulista, 01405-900 São Paulo | - |
dc.identifier.doi | 10.1103/PhysRevD.61.055003 | - |
dc.identifier.wos | WOS:000085685600038 | - |
dc.rights.accessRights | Acesso restrito | - |
dc.identifier.file | 2-s2.0-17044436921.pdf | - |
dc.relation.ispartof | Physical Review D: Particles, Fields, Gravitation and Cosmology | - |
dc.identifier.scopus | 2-s2.0-17044436921 | - |
Appears in Collections: | Artigos, TCCs, Teses e Dissertações da Unesp |
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