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相关论文: New Tsallis agegraphic Dark Energy in Chern-Simons…

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Recently, Tsallis, R\'{e}nyi and Sharma-Mitall and entropies have widely been used to study the gravitational and cosmological setups. We consider a flat FRW universe with linear interaction between dark energy and dark matter. We discuss…

综合物理 · 物理学 2019-01-08 M. Younas , Abdul Jawad , Saba Qummer , H. Moradpour , Shamaila Rani

In this paper, we study the new Tsallis agegraghic dark energy model in the context of fractal cosmology. The different cosmic implications such as statefinder diagnosis, cosmological plane and squared of sound speed in both interacting and…

广义相对论与量子宇宙学 · 物理学 2024-01-17 M. Abdollahi Zadeh

In this manuscript, we examine the cosmological significance of the new agegraphic dark energy model by investigating different cosmological parameters such as the equation of state parameter, $\omega_{D}-\omega^{\prime}_{D}$ and the $r-s$…

广义相对论与量子宇宙学 · 物理学 2025-01-03 Madiha Ajmal , M. Sharif

In this work, we explore the recently proposed new Tsallis agegraphic dark energy model in a flat FLRW Universe by taking the conformal time as IR cutoff with interaction. The deceleration parameter of the interacting new Tsallis agegraphic…

广义相对论与量子宇宙学 · 物理学 2021-05-07 Shikha Srivastava , Umesh Kumar Sharma , Vipin Chandra Dubey

The purpose of this paper is to study the Tsallis agegraphic dark energy with an interaction term between dark energy and dark matter in the DGP brane-world scenario. For this, we assume some initial conditions to obtain the dark energy…

广义相对论与量子宇宙学 · 物理学 2022-03-17 Z. Feizi Mangoudehi

We investigate the new Tsallis agegraphic dark energy (NTADE) scenario in the framework of Horava-Lifshitz cosmology. Considering interacting and non-interacting scenarios of NTADE with dark matter in a spatially non-flat universe, we…

广义相对论与量子宇宙学 · 物理学 2020-01-22 M. Abdollahi Zadeh

The paper investigates the Tsallis holographic dark energy (THDE) model in accordance with the apparent horizon as an infrared cut-off, in a non-flat universe. The cosmological evolution of the deceleration parameter and equation of state…

综合物理 · 物理学 2020-01-16 Vipin Chandra Dubey , Umesh Kumar Sharma , A. Beesham

In this work, we have considered the recently proposed new Tsallis Agegraphic Dark Energy model (NTADE) (Mod. Phys. Lett. A 34, 1950086, 2019) within the framework of a flat Friedmann-Robertson-Walker(FRW) Universe by taking various values…

广义相对论与量子宇宙学 · 物理学 2021-05-18 Umesh Kumar Sharma , Shikha Srivastava

The paper explores the interacting Tsallis holographic dark energy (THDE) model in a non-flat universe following an infrared cutoff as the apparent horizon. The equation of state (EoS) and the deceleration parameter of THDE model are…

综合物理 · 物理学 2021-08-02 Umesh Kumar Sharma , Vipin Chandra Dubey , A. Pradhan

In this paper we study cosmological application of new agegraphic dark energy density in the $f(R)$ gravity framework. We employ the new agegraphic model of dark energy to obtain the equation of state for the new agegraphic energy density…

广义相对论与量子宇宙学 · 物理学 2010-04-30 M. R. Setare

In this study, we explore the reconstruction of a new agegraphic dark energy model in a flat Friedmann-Robertson-Walker spacetime by $f(Q)$ gravity framework, where $Q$ represents non-metricity. We assume that the scale factor follows a…

广义相对论与量子宇宙学 · 物理学 2025-11-10 M. Sharif , Madiha Ajmal

We discuss the recently suggested Ricci-Gauss-Bonnet holographic dark energy in Chern-Simons modified gravity. We have tested some general forms of the scale factor $a(t)$, and used two physically reasonable forms which have been proved to…

广义相对论与量子宇宙学 · 物理学 2020-03-04 Nasr Ahmed

We investigate the ghost model of dark energy in the framework of DGP braneworld. We explore the cosmological consequences of this model by determining the equation of state parameter, $\omega_D$, the deceleration and the density…

广义相对论与量子宇宙学 · 物理学 2018-10-31 M. Abdollahi Zadeh , A. Sheykhi

This paper is devoted to study some holographic dark energy models in the context of Chern-Simon modified gravity by considering FRW universe. We analyze the equation of state parameter using Granda and Oliveros infrared cut-off proposal…

广义相对论与量子宇宙学 · 物理学 2017-08-31 M. Jamil Amir , Sarfraz Ali

In this paper, we investigate the cosmological consequences of ghost dark energy model in modified Gauss-Bonnet gravity. We construct ghost dark energy $f(G)$ model by using correspondence scenario for both interacting and non-interacting…

广义相对论与量子宇宙学 · 物理学 2019-08-21 M. Sharif , Saadia Saba

The proposed model is a study of the nature of dark energy through non-extensive Tsallis entropy. The method is based on the Karolyhazy relation which is a combined idea from quantum physics and general relativity. Dark energy is the energy…

广义相对论与量子宇宙学 · 物理学 2022-11-23 Pankaj , Bramha Dutta Pandey , P. Suresh Kumar , Umesh Kumar Sharma

The present work is based on the idea of an interacting framework of new holographic dark energy with cold dark matter in the background of $f(T)$ gravity. Here, we have considered the flat modified Friedmann universe for $f(T)$ gravity…

广义相对论与量子宇宙学 · 物理学 2016-02-17 Chayan Ranjit , Prabir Rudra

We investigate the agegraphic dark energy models which were recently proposed to explain the dark energy-dominated universe. For this purpose, we calculate their equation of states and squared speeds of sound. We find that the squared speed…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Kyoung Yee Kim , Hyung Won Lee , Yun Soo Myung

We explore the cosmological aspects of interacting Tsallis holographic dark energy (THDE) in a $q$-modified DGP braneworld setup emerging from non-Gaussian statistical mechanics.To this end, three classes of superstatistics, that is,…

广义相对论与量子宇宙学 · 物理学 2022-11-15 Naouel Boulkaboul

In this paper, we study R\'{e}nyi holographic dark energy model in the context of Chern Simons (CS) modified gravity theory. Different cosmological parameters such as energy density, deceleration parameter, equation of state, square of…

广义相对论与量子宇宙学 · 物理学 2021-10-04 Sarfraz Ali , Sarfaraz Khan , Sadia Sattar , Amare Abebe
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