Mirror World with Broken Mirror Parity, E(6) Unification and Cosmology
| dc.creator | Das, C. R. | |
| dc.creator | Laperashvili, L. V. | |
| dc.date | 2007-12-09 | |
| dc.date | 2008-01-27 | |
| dc.date.accessioned | 2026-07-07T09:45:42Z | |
| dc.date.available | 2026-07-07T09:45:42Z | |
| dc.description | In the present paper we have developed a concept of parallel ordinary (O) and mirror (M) worlds. We have shown that in the case of a broken mirror parity (MP), the evolutions of fine structure constants in the O- and M-worlds are not identical. It is assumed that E_6-unification inspired by superstring theory restores the broken MP at the scale \sim 10^{18} GeV, what unavoidably leads to the different E_6-breakdowns at this scale: E_6 \to SO(10)\times U(1)_Z - in the O-world, and E'_6 \to SU(6)'\times SU(2)'_Z - in the M-world. Considering only asymptotically free theories, we have presented the running of all the inverse gauge constants α_i^{-1} in the one-loop approximation. Then a `quintessence' scenario is discussed for our model of accelerating universe. Such a scenario is related with an axion (`acceleron') of a new gauge group SU(2)'_Z which has a coupling constant g_Z extremely growing at the scale Λ_Z\sim 10^{-3} eV. | |
| dc.description | 31 pages, 7 figures | |
| dc.identifier | https://arxiv.org/abs/0712.1326 | |
| dc.identifier | http://arxiv.org/abs/0712.1326 | |
| dc.identifier | Int.J.Mod.Phys.A23:1863-1890,2008 | |
| dc.identifier | doi:10.1142/S0217751X08039712 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/163284 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Astrophysics | |
| dc.title | Mirror World with Broken Mirror Parity, E(6) Unification and Cosmology | |
| dc.type | text |