Observational constraints on the product of dark energy chemical potential and number density in out-of-equilibrium models

Abstract

In this work, we impose observational limits on the product of dark energy chemical potential, $\mu$, and number density, $n$, at the present time in out-of-equilibrium models, considering that particles can be created or destroyed in the fluid at a rate $\Gamma =3\alpha H(a)$, where $\alpha$ is a constant and $H(a)\equiv \dot{a}/a$ is the Hubble parameter. We combine the bounds derived from the positivity of entropy and the second law of thermodynamics with observational constraints on the Chevallier-Polarski-Linder (CPL) and Barboza-Alcaniz (BA) parameterizations of the equation of state (EoS) of the component. We use Type Ia supernovae (SN Ia) data from Pantheon+; baryon acoustic oscillation (BAO) data from DESI DR2; and cosmic microwave background (CMB) measurements from Planck. For $\alpha >0$ (particle creation), the thermodynamic restrictions yield only upper limits for the ${\mu }_0{n}_0$ product, while in the case of $\alpha <0$ (particle destruction) they establish both upper and lower limits, allowing for a range of values to be obtained. In both scenarios, however, we find that the chemical potential of dark energy must be negative, $\mu <0$, which indicates a preference for the phantom regime. In particular, when $\alpha <0$, it is noted that the thermodynamic bounds are simultaneously compatible only for very small absolute values of $\alpha$, with $\alpha =-0.0002$ being the limiting case and resulting in ${\mu }_0{n}_0(\alpha =-0.0002)=-2.2_{-0.7}^{+1.0}GeV/m^3$.

11 pages, 6 figures, 3 tables