Mu Problem and Hybrid Inflation in Supersymmetric SU(2)_L x SU(2)_R x U(1)_B-L
| dc.creator | Dvali, G. | |
| dc.creator | Lazarides, G. | |
| dc.creator | Shafi, Q. | |
| dc.date | 1997-10-10 | |
| dc.date.accessioned | 2026-07-07T11:35:24Z | |
| dc.date.available | 2026-07-07T11:35:24Z | |
| dc.description | We present a solution of the mu problem within a supersymmetric model based on the SU(2)_L x SU(2)_R x U(1)_{B-L} gauge group. We show that this solution implies a built-in hybrid inflationary scenario, which may result in a successful baryogenesis via leptogenesis. Baryon number is essentially conserved as a result of an R-symmetry. Neutrinos with mass in the eV range can provide the `hot' dark matter component. | |
| dc.description | 11 pages, LaTeX, RevTeX, no figs | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9710314 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9710314 | |
| dc.identifier | Phys.Lett.B424:259-264,1998 | |
| dc.identifier | doi:10.1016/S0370-2693(98)00145-2 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/198583 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Mu Problem and Hybrid Inflation in Supersymmetric SU(2)_L x SU(2)_R x U(1)_B-L | |
| dc.type | text |