Constraining the Lorentz-Violating Bumblebee Vector Field with Big Bang Nucleosynthesis and Gravitational Baryogenesis
arXiv:2211.07934 · doi:10.1140/epjc/s10052-023-11546-3
Abstract
By keeping the cosmological principle i.e., an isotropic and homogeneous universe, we consider the cosmology of a vector-tensor theory of gravitation known as the \textit{bumblebee} model. In this model a single Lorentz-violating timelike vector field with a nonzero vacuum expectation value (VEV) couples to the Ricci tensor and scalar, as well. Taking the ansatz for the time evolution of the vector field we derive the relevant dynamic equations of the Universe, where is a free parameter. In particular, by employing observational data coming from the Big Bang Nucleosynthesis (BBN) and the matter-antimatter asymmetry in the Baryogenesis era, we impose some constraints on the VEV of the bumblebee timelike vector field i.e., , and the exponent parameter . The former and the latter limit the size of Lorentz violation, and the rate of the time evolution of the background Lorentz-violating bumblebee field, respectively.
18 pages (two columns), 8 figures.v2: discussion and analysis improved, some references and figures added, version accepted in EPJC
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- Dark matter spike around Bumblebee black holes
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