Stability of HDE model with sign-changeable interaction in Brans-Dicke theory
M. Abdollahi Zadeh, A.Sheykhi

TL;DR
This paper investigates the stability and cosmological behavior of a sign-changeable interacting holographic dark energy model within Brans-Dicke theory, analyzing different IR cutoffs and their implications for universe acceleration and stability.
Contribution
It introduces a detailed analysis of the stability of sign-changeable HDE in Brans-Dicke cosmology with various IR cutoffs, highlighting the event horizon as the most stable choice.
Findings
The EoS parameter can cross the phantom line, enabling universe acceleration.
The universe can be stable with the future event horizon cutoff depending on parameters.
GO and Ricci cutoffs generally do not lead to stable DE-dominated universe except in special cases.
Abstract
We consider the Brans-Dicke (BD) theory of gravity and explore the cosmological implications of the sign-changeable interacting holographic dark energy (HDE) model in the background of Friedmann-Robertson-Walker (FRW) universe. As the system's infrared (IR) cutoff, we choose the future event horizon, the Granda-Oliveros (GO) and the Ricci cutoffs. For each cutoff, we obtain the density parameter, the equation of state (EoS) and the deceleration parameter of the system. In case of future event horizon, we find out that the EoS parameter, , can cross the phantom line, as a result the transition from deceleration to acceleration expansion of the universe can be achieved provided the model parameters are chosen suitably. Then, we investigate the instability of the sign-changeable interacting HDE model against perturbations in BD theory. For this purpose, we study the squared sound…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories
