SearcharxivSearch

arXiv subjects

Chi-Yi Chen

Publications and source records attributed to Chi-Yi Chen.

2 recordsLinked to original sources

Scalar Gravity and Higgs Mechanism

The role that the auxiliary scalar field $ϕ$ played in Brans-Dicke cosmology is discussed. If a constant vacuum energy is assumed to be the origin of dark energy, then the corresponding density parameter would be a quantity varying with $ϕ$; and almost all of the fundamental components of our universe can be unified into the dynamical equation for $ϕ$. As a generalization of Brans-Dicke theory, we propose a new gravity theory with a complex scalar field $ϕ$ which is coupled to the cosmological curvature scalar. Through such a coupling, the Higgs mechanism is naturally incorporated into the evolution of the universe, and a running density of the field vacuum energy is obtained which may release the particle standard model from the rigorous cosmological constant problem in some sense. Our model predicts a running mass scale of the fundamental particles in which the gauge symmetry breaks spontaneously. The running speed of the mass scale in our case could survive all existing experiments.

gr-qc

Spontaneous Leptogenesis in Brans-Dicke Cosmology

The role of the auxiliary scalar field $ϕ$ of Brans-Dicke theory played in baryon number asymmetry is discussed in this paper. We consider a derivative coupling of this gravitational scalar field to the baryon current ${J^μ}_B$ or the current of the baryon number minus lepton number ${J^μ}_{B-L}$ based on a series of works of R. Morganstern about the Brans-Dicke cosmology. We find that the spontaneous baryogenesis by this coupling is capable to yield a sufficient baryon asymmetry $n_B/s\sim 10^{10} $ for the time of the grand unification is in a little advanced. In addition, Davoudiasl et al have recently introduced a new type of interaction between the Ricci scalar $R$ and the bayon current $J^μ$, $\partial_μR J^μ$ and also proposed a mechanism for baryogenesis, the gravitational baryogenesis. However, the Einstein equation tell us that $\dot{R}=0$ in the radiation-dominated epoch of the standard FRW cosmology. In this paper we reconsider the feasibility of having gravitational baryongenesis with such a form of interaction in radiation-filled Brans-Dicke cosmology. We will show that $\dot{R}$ does not vanish in this case and the required baryon number asymmetry can also be achieved.

hep-ph