Interacting Dark Energy
| dc.creator | Zhang, Xinmin | |
| dc.date | 2004-10-21 | |
| dc.date.accessioned | 2026-07-07T03:53:45Z | |
| dc.date.available | 2026-07-07T03:53:45Z | |
| dc.description | In this paper I discuss some of the phenomenologies of models of the dark energy interacting with the ordinary matter. After a very brief review about the current constraint on the equation of the state of the dark energy from the SN and a new scenario of dark energy {\it the Quintom}, I present models of Quintessential Baryo(Lepto)genesis, Quintessino dark matter and mass varying neutrinos in details. | |
| dc.description | Plenary talk at "SUSY2004", Tsukuba, Japan, June 2004: LaTeX with pdproc.sty (included), 13pages | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0410292 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0410292 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/43959 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Interacting Dark Energy | |
| dc.type | text |