Scalar Bilepton Dark Matter
| dc.creator | Pires, C. A. de S. | |
| dc.creator | da Silva, P. S. Rodrigues | |
| dc.date | 2007-10-11 | |
| dc.date | 2008-01-18 | |
| dc.date.accessioned | 2026-07-07T12:24:00Z | |
| dc.date.available | 2026-07-07T12:24:00Z | |
| dc.description | In this work we show that 3-3-1 model with right-handed neutrinos has a natural weakly interacting massive particle (WIMP) dark mater candidate. It is a complex scalar with mass of order of some hundreds of GeV which carries two units of lepton number, a scalar bilepton. This makes it a very peculiar WIMP, very distinct from Supersymmetric or Extra-dimension candidates. Besides, although we have to make some reasonable assumptions concerning the several parameters in the model, no fine tunning is required in order to get the correct dark matter abundance. We also analyze the prospects for WIMP direct detection by considering recent and projected sensitivities for WIMP-nucleon elastic cross section from CDMS and XENON Collaborations. | |
| dc.description | 21 pages, 8 figures, uses iopart.cls, same text as published version with a small different arrangement of figures | |
| dc.identifier | https://arxiv.org/abs/0710.2104 | |
| dc.identifier | http://arxiv.org/abs/0710.2104 | |
| dc.identifier | JCAP 0712:012,2007 | |
| dc.identifier | doi:10.1088/1475-7516/2007/12/012 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/214186 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Scalar Bilepton Dark Matter | |
| dc.type | text |