Constraints on a special running vacuum model
arXiv:2001.05092 · doi:10.1140/epjc/s10052-020-7653-z
Abstract
We study a special running vacuum model (RVM) with , where , and are the model parameters and is the Hubble one. This RVM has non-analytic background solutions for the energy densities of matter and radiation, which can only be evaluated numerically. From the analysis of the CMB power spectrum and baryon acoustic oscillation along with the prior of to avoid having a negative dark energy density, we find that and (95 C.L.). We show that the RVM fits the cosmological data comparably to the CDM. In addition, we relate the fluctuation amplitude to the neutrino mass sum .
16 pages, 6 figures, accepted for publication in EPJC
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