Dynamical constraints on variable vacuum energy in Brans-Dicke theory

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Autori principali: Patle, Khomesh R., Singh, G. P., Garg, Romanshu
Natura: Preprint
Pubblicazione: 2026
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author Patle, Khomesh R.
Singh, G. P.
Garg, Romanshu
author_facet Patle, Khomesh R.
Singh, G. P.
Garg, Romanshu
contents In this research work, we investigate the late-time accelerated expansion of the universe within the framework of Brans-Dicke theory by considering dynamical vacuum energy models with a time-varying cosmological constant. Two vacuum energy models are studied, namely the hybrid vacuum law $Λ(t)=αH^{2}+β\dot{H}$ and the power vacuum law $Λ(H)=α_{1}H^{n}$, where $α$, $β$, $α_{1}$ and $n$ are free parameters. We derive analytical solutions for the Hubble parameter and other relevant cosmological quantities. The evolution of the deceleration parameter, the effective equation of state parameter, the cosmographic parameters, the behaviour of Om($\mathit{z}$) diagnostics and the present age of the universe are examined. Furthermore, the analysis of the $ω_{\rm eff}-ω'_{\rm eff}$ plane shows that the model evolves in the freezing region and the thermodynamic analysis confirms that the generalized second law of thermodynamics is satisfied within the power vacuum law model.
format Preprint
id arxiv_https___arxiv_org_abs_2601_00419
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Dynamical constraints on variable vacuum energy in Brans-Dicke theory
Patle, Khomesh R.
Singh, G. P.
Garg, Romanshu
General Relativity and Quantum Cosmology
In this research work, we investigate the late-time accelerated expansion of the universe within the framework of Brans-Dicke theory by considering dynamical vacuum energy models with a time-varying cosmological constant. Two vacuum energy models are studied, namely the hybrid vacuum law $Λ(t)=αH^{2}+β\dot{H}$ and the power vacuum law $Λ(H)=α_{1}H^{n}$, where $α$, $β$, $α_{1}$ and $n$ are free parameters. We derive analytical solutions for the Hubble parameter and other relevant cosmological quantities. The evolution of the deceleration parameter, the effective equation of state parameter, the cosmographic parameters, the behaviour of Om($\mathit{z}$) diagnostics and the present age of the universe are examined. Furthermore, the analysis of the $ω_{\rm eff}-ω'_{\rm eff}$ plane shows that the model evolves in the freezing region and the thermodynamic analysis confirms that the generalized second law of thermodynamics is satisfied within the power vacuum law model.
title Dynamical constraints on variable vacuum energy in Brans-Dicke theory
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2601.00419