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A new class of FLRW cosmological models with time-evolving fundamental parameters should emerge naturally from a description of the expansion of the universe based on the first principles of quantum field theory and string theory. Within…

宇宙学与河外天体物理 · 物理学 2011-08-09 Javier Grande , Joan Sola , Spyros Basilakos , Manolis Plionis

In this work, we study the evolution of a fractal universe composed of Tsallis holographic dark energy (THDE) and a pressureless dark matter that interact with each other through a mutual interaction. We then reconstruct the interaction…

广义相对论与量子宇宙学 · 物理学 2020-10-28 Abdulla Al Mamon

We perform a comparative study of different types of dynamical dark energy models (DDES) using the cosmographic method. Among the models being examined herein we have the Running Vacuum models (RVMs), which have demonstrated considerable…

宇宙学与河外天体物理 · 物理学 2022-09-01 Mehdi Rezaei , Joan Sola Peracaula

Background cosmological dynamics for a universe with matter, a scalar field non-minimally derivative coupling to Einstein tensor under power-law potential and holographic vacuum energy is considered here. The holographic IR cutoff scale is…

广义相对论与量子宇宙学 · 物理学 2024-06-17 Amornthep Tita , Burin Gumjudpai , Pornrad Srisawad

In this work we explore a Holographic Dark Energy Model in a flat Friedmann-Lema\^itre-Robertson-Walker Universe, which contains baryons, radiation, cold dark matter and dark energy within the framework of General Relativity. Furthermore,…

广义相对论与量子宇宙学 · 物理学 2019-05-10 Carlos Rodriguez-Benites , Mauricio Cataldo , Antonella Cid , Carlos Ríos

The model of generalized Tsallis holographic dark energy (which is known to be particular representative of Nojiri-Odintsov HDE) with event horizon as cut-off is investigated using methods of dynamical analysis. We take into consideration…

广义相对论与量子宇宙学 · 物理学 2023-08-16 A. V. Astashenok , A. S. Tepliakov

The braneworld model proposed by Dvali, Gabadadze and Porrati (DGP) leads to an accelerated universe without cosmological constant or other form of dark energy for the positive branch $(\epsilon =+1)$. For the negative branch $(\epsilon…

宇宙学与河外天体物理 · 物理学 2015-06-17 Yeremy Aguilera , Arturo Avelino , Norman Cruz , Samuel Lepe , Francisco Peña

Considering the holographic dark energy (HDE) with two different Infrared (IR) cutoffs, we study the evolution of a cyclic universe which avoids the Big-Rip singularity. Our results show that, even in the absence of a mutual interaction…

广义相对论与量子宇宙学 · 物理学 2018-10-17 A. Sheykhi , M. Tavayef , H. Moradpour

In this study, we employ a two-step method to analyze models of holographic dark energy (HDE) and interacting holographic dark energy (IHDE), incorporating three distinct dark energy (DE)-dark matter (DM) interaction terms. First, using the…

宇宙学与河外天体物理 · 物理学 2025-10-21 N. Nazari Pooya

We study cosmological application of interacting holographic energy density in the framework of Brans-Dicke cosmology. We obtain the equation of state and the deceleration parameter of the holographic dark energy in a non-flat universe. As…

高能物理 - 理论 · 物理学 2009-11-05 Ahmad Sheykhi

In this paper we study the cosmological evolution of the holographic dark energy in a cyclic universe, generalizing the model of holographic dark energy proposed by Li. The holographic dark energy with $c<1$ can realize a quintom behavior;…

高能物理 - 理论 · 物理学 2008-11-26 Jingfei Zhang , Xin Zhang , Hongya Liu

We study non-viscous and viscous holographic dark energy models for a homogeneous and isotropic flat Friedmann-Robertson-Walker Universe in $f(R,T)$ gravity. We find that the Hubble horizon as an IR cut-off is suitable for both the models…

广义相对论与量子宇宙学 · 物理学 2015-10-15 C. P. Singh , Pankaj Kumar

We have studied the effect of dynamical radiation in the interacting barrow holographic dark energy model for a non-flat universe. For both open and closed universes, we have obtained the evolution equation for the energy density parameters…

广义相对论与量子宇宙学 · 物理学 2026-05-08 Gopinath Guin , Souvik Paul , Sunandan Gangopadhyay

We present a Bayesian comparative analysis of five cosmological models: $\Lambda$CDM, $w$CDM, $w_0w_a$CDM, $\phi$CDM (with scalar-field dark energy), and an interacting dark energy scenario (the $\xi$-index model), to investigate dark…

宇宙学与河外天体物理 · 物理学 2025-12-19 Zhuoming Zhang , Tengpeng Xu , Yun Chen

Using the first law of thermodynamics, we propose a relation between the system entropy ($S$) and its IR ($L$) and UV ($\Lambda$) cutoffs. In addition, applying this relation to the apparent horizon of flat FRW universe, whose entropy meets…

综合物理 · 物理学 2018-10-18 H. Moradpour , S. A. Moosavi , I. P. Lobo , J. P. Morais Graça , A. Jawad , I. G. Salako

In present research, we construct Kaniadakis holographic dark energy (KHDE) model within a non-flat Universe by considering the Friedmann-Robertson-Walker (FRW) metric with open and closed spatial geometries. We therefore investigate cosmic…

综合物理 · 物理学 2022-04-19 Umesh Kumar Sharma , Vipin Chandra Dubey , A. H. Ziaie , H. Moradpour

In this paper, we examine two types of interacting holographic dark energy model using Pantheon supernova data, BAO BOSS DR12, CMB Planck 2015, fgas (gas mass fraction) and SZ/Xray (Sunyaev-Zeldovich effect and X-ray emission) data from…

广义相对论与量子宇宙学 · 物理学 2020-07-14 Ehsan Sadri , Martiros Khurshudyan , Ding-fang Zeng

Using the nonextensive Tsallis entropy and the holographic hypothesis, we propose a new dark energy (DE) model with time scale as infrared (IR) cutoff. Considering the age of the Universe as well as the conformal time as IR cutoffs, we…

综合物理 · 物理学 2019-04-01 M. Abdollahi Zadeh , A. Sheykhi , H. Moradpour

In this paper we investigate the possible direct, non-gravitational interaction between holographic dark energy (HDE) and dark matter. Firstly, we start with two simple models with the interaction terms $Q \propto \rho_{dm}$ and $Q \propto…

宇宙学与河外天体物理 · 物理学 2012-06-13 Zhenhui Zhang , Song Li , Xiao-Dong Li , Xin Zhang , Miao Li

In this review we consider in detail different theoretical topics associated with interaction in the dark sector. We study linear and nonlinear interactions which depend on the dark matter and dark energy densities. We consider a number of…

宇宙学与河外天体物理 · 物理学 2015-03-25 Yu. L. Bolotin , A. Kostenko , O. A. Lemets , D. A. Yerokhin