English

A Model of Dark Energy and Dark Matter

High Energy Physics - Phenomenology 2010-11-05 v2 Astrophysics

Abstract

A dynamical model for the dark energy is presented in which the ``quintessence'' field is the axion, aZa_Z, of a spontaneously broken global U(1)A(Z)U(1)_{A}^{(Z)} symmetry whose potential is induced by the instantons of a new gauge group SU(2)ZSU(2)_Z. The SU(2)ZSU(2)_Z coupling becomes large at a scale ΛZ103eV\Lambda_Z \sim 10^{-3} eV starting from an initial value MM at high energy which is of the order of the Standard Model (SM) couplings at the same scale MM. A perspective on a possible unification of SU(2)ZSU(2)_Z with the SM will be briefly discussed. We present a scenario in which aZa_Z is trapped in a false vacuum characterized by an energy density (103eV)4\sim (10^{-3} eV)^4. The lifetime of this false vacuum is estimated to be extremely large. Other estimates relevant to the ``coincidence issue'' include the ages of the universe when the aZa_Z potential became effective, when the acceleration ``began'' and when the energy density of the false vacuum became comparable to that of (baryonic and non-baryonic) matter. Other cosmological consequences include a possible candidate for the weakly interacting (WIMP) Cold Dark Matter as well as a scenario for leptogenesis. A brief discussion on possible laboratory detections of some of the particles contained in the model will also be presented.

Keywords

Cite

@article{arxiv.hep-ph/0512282,
  title  = {A Model of Dark Energy and Dark Matter},
  author = {P. Q. Hung},
  journal= {arXiv preprint arXiv:hep-ph/0512282},
  year   = {2010}
}

Comments

24 double-column pages, 14 figures; Added references; Corrected Typos