Observational constraint on interacting Tsallis holographic dark energy in logarithmic Brans–Dicke theory

Y Aditya, S Mandal, PK Sahoo, DRK Reddy - The European Physical …, 2019 - Springer
In this paper, we investigate the dark energy phenomenon by studying the Tsallis
holographic dark energy within the framework of Brans–Dicke (BD) scalar–tensor theory of …

Shadow of rotating black holes surrounded by dark fluid with Chaplygin-like equation of state and constraints from EHT results

M Zahid, F Sarikulov, C Shen, S Ahmedov… - … and Quantum Gravity, 2024 - iopscience.iop.org
In this work, we mainly focus on testing the spacetime properties around black holes
surrounded by a dark fluid, which are potential candidates for dark energy described by the …

On the phenomenology of an accelerated large-scale universe

M Khurshudyan - Symmetry, 2016 - mdpi.com
In this review paper, several new results towards the explanation of the accelerated
expansion of the large-scale universe is discussed. On the other hand, inflation is the early …

[HTML][HTML] Kantowski–Sachs Tsallis holographic dark energy model with sign-changeable interaction

Y Sobhanbabu, M Vijaya Santhi - The European Physical Journal C, 2021 - Springer
In this work devoted to the investigation of the Tsallis holographic dark energy (IR cut-off is
Hubble radius) in homogeneous and anisotropic Kantowski–Sachs Universe within the …

Compartmentalization and coexistence in the dark sector of the universe

A Paliathanasis, K Duffy, A Halder, A Abebe - Physics of the Dark Universe, 2025 - Elsevier
We revise the cosmological interaction between dark energy and dark matter. More
precisely, we focus on models that support compartmentalization or coexistence in the dark …

Phase space analysis of some interacting Chaplygin gas models

M Khurshudyan, R Myrzakulov - The European Physical Journal C, 2017 - Springer
In this paper we discuss a phase space analysis of various interacting Chaplygin gas
models in general relativity. Linear and nonlinear sign changeable interactions are …

[PDF][PDF] Can extended Chaplygin gas source a Hubble tension resolved emergent universe?

R Sengupta, P Paul, BC Paul, M Kalam - arXiv preprint arXiv …, 2023 - academia.edu
In this paper, we attempt to explore the possibility of a obtaining a viable emergent universe
scenario supported by a type of fluid known as the extended Chaplygin gas, which extends …

Nonlinear stability of self-gravitating irrotational Chaplygin fluids in a FLRW geometry

PG LeFloch, C Wei - Annales de l'Institut Henri Poincaré C, Analyse non …, 2021 - Elsevier
We analyze the global nonlinear stability of FLRW (Friedmann-Lemaître-Robertson-Walker)
spacetimes in the presence of an irrotational perfect fluid. We assume that the fluid is …

Universe with quadratic equation of state: A dynamical systems perspective

R Raushan, A Singh, R Chaubey… - International Journal of …, 2020 - World Scientific
This paper deals with the dynamical systems analysis of Friedmann–Robertson–Walker
(FRW) model of the Universe in the framework of general relativity with quadratic equation of …

Chaplygin-gas solutions of gravity

M Elmardi, A Abebe, A Tekola - International Journal of Geometric …, 2016 - World Scientific
We explore exact f (R) gravity solutions that mimic Chaplygin-gas inspired Λ CDM
cosmology. Starting with the original, generalized and modified Chaplygin-gas (MCG) …