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相关论文: Dynamics of Teleparallel Dark Energy

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A cosmic potential which can relax the vacuum energy is proposed in a framework of scalar-tensor gravity. In the phase of the gravity scalar field around the evolution with an approximate emergent conformal symmetry, we have obtained a set…

广义相对论与量子宇宙学 · 物理学 2013-08-30 Yongsung Yoon

The present work deals with holographic dark energy in the context of unimodular $f(T)$ gravity, which is a modification of teleparallel gravity. We develop the general reconstruction procedure of the $f(T)$ form that can yield the…

综合物理 · 物理学 2017-11-07 A. E. Godonou , M. J. S. Houndjo , J. Tossa

We perform a detailed investigation of interacting phantom cosmology, by applying the powerful method of dynamical system analysis. We consider two well-studied interaction forms, namely one global and one local one, while the novel…

广义相对论与量子宇宙学 · 物理学 2025-07-11 Sudip Halder , S. D. Odintsov , Supriya Pan , Tapan Saha , Emmanuel N. Saridakis

We study a new type of the modified teleparallel gravity of the form $F(T,\,\Theta)$ in which $T$, the torsion scalar, is coupled with $\Theta$, the trace of the stress-energy tensor. In a perturbational approach, we study the stability of…

广义相对论与量子宇宙学 · 物理学 2015-06-17 Faeze Kiani , Kourosh Nozari

We investigate a cosmological model in which dark energy, represented by a quintessential scalar field, is coupled to a dark-matter perfect fluid in the spatially flat Friedmann-Robertson-Walker Universe. This allows an energy exchange in…

广义相对论与量子宇宙学 · 物理学 2023-08-22 Yousef Bisabr

In a spatially flat \ Friedmann--Lema\^{\i}tre--Robertson--Walker background space we consider a scalar-torsion gravitational model which has similar properties with the dilaton theory. This teleparallel model is invariant under a discrete…

广义相对论与量子宇宙学 · 物理学 2021-07-19 Andronikos Paliathanasis

To explain the acceleration of the cosmological expansion researchers have considered an unusual form of mass-energy generically called dark energy. Dark energy has a ratio of pressure over mass density which obeys $w=p/\rho <-1/3$. This…

高能物理 - 理论 · 物理学 2008-12-19 Max Chaves , Douglas Singleton

We apply the teleparallelism condition to the Poincar\'{e} gauge theory of gravity. The resultant teleparallelized cosmology is completely equivalent to the Friedmann cosmology derived from Einstein's general theory of relativity. The…

广义相对论与量子宇宙学 · 物理学 2014-09-10 Wenjie Lu , Wolung Lee , Kin-Wang Ng

Scalar-tensor theory of gravity with non-minimal coupling is a fairly good candidate for dark energy, required to explain late-time cosmic evolution. Here we study the very early stage of evolution of the universe with a modified version of…

高能物理 - 理论 · 物理学 2018-05-22 Ranajit Mandal , Chandramouli Sarkar , Abhik Kumar Sanyal

Recent DESI DR2 observations indicate that dark energy has crossed from phantom to quintessence regime, a behavior known as the quintom-B realization. In this work we constrain dynamical dark energy and modified gravity using the swampland…

宇宙学与河外天体物理 · 物理学 2025-04-21 Chunyu Li , Junkai Wang , Dongdong Zhang , Emmanuel N. Saridakis , Yi-Fu Cai

In the context of the induced matter theory of gravity, we investigate the possibility of deriving a 4D quintessential scenario where an interaction between dark energy and dark matter is allowed, and the dark energy component is modeled by…

广义相对论与量子宇宙学 · 物理学 2009-08-11 L. M. Reyes , Jose Edgar Madriz Aguilar

Dynamical dark energy has gained renewed interest due to recent theoretical and observational developments. In the present paper, we focus on a string-motivated dark energy set-up, and perform a detailed cosmological analysis of exponential…

宇宙学与河外天体物理 · 物理学 2024-06-04 Sukannya Bhattacharya , Giulia Borghetto , Ameek Malhotra , Susha Parameswaran , Gianmassimo Tasinato , Ivonne Zavala

The distinction between modified gravity and quintessence or dynamical dark energy is difficult. Many models of modified gravity are equivalent to models of coupled quintessence by virtue of variable transformations. This makes an…

宇宙学与河外天体物理 · 物理学 2015-06-18 C. Wetterich

We study the dynamics of a phantom scalar field dark energy interacting with dark matter in loop quantum cosmology (LQC). Two kinds of coupling of the form $\alpha{\rho_m}{\dot\phi}$ (case I) and $3\beta H (\rho_\phi +\rho_m)$ (case II)…

广义相对论与量子宇宙学 · 物理学 2009-02-20 Xiangyun Fu , Hongwei Yu , Puxun Wu

In trace-free Einstein gravity, the stress-energy tensor of matter is not necessarily conserved and so the theory offers a natural framework for interacting dark energy models where dark energy has a constant equation of state $w=-1$. We…

广义相对论与量子宇宙学 · 物理学 2022-07-29 Marco de Cesare , Edward Wilson-Ewing

Quasi-constant external fields in nonlinear electromagnetism generate a contribution to the energy-momentum tensor with the form of dark energy. To provide a thorough understanding of the origin and strength of the effects, we undertake a…

高能物理 - 理论 · 物理学 2010-04-14 Lance Labun , Johann Rafelski

Extended quintessence is obtained by coupling a normal scalar field to the Ricci scalar defined in the metric formalism. In this paper, we propose a new extended quintessence dark energy by introducing a non-minimal coupling between the…

广义相对论与量子宇宙学 · 物理学 2013-02-27 Peng Wang , Puxun Wu , Hongwei Yu

Many parity violating gravity models suffer from the ghost instability problem. In this paper, we consider a symmetric teleparallel gravity model that extends the general relativity equivalent model by several parity violating interactions…

广义相对论与量子宇宙学 · 物理学 2022-08-23 Mingzhe Li , Yeheng Tong , Dehao Zhao

We point out that dark matter and dark energy arise naturally in a recently proposed model of combinatorial quantum gravity. Dark energy is due to the ground-state curvature at finite coupling, dark matter arises from allotropy in the…

广义相对论与量子宇宙学 · 物理学 2024-09-17 Carlo A. Trugenberger

It seems necessary to suppress, at least partially, the formation of structure on subgalactic scales. As an alternative to warm or collisional dark matter, I postulate a condensate of massive bosons interacting via a repulsive interparticle…

天体物理学 · 物理学 2009-10-31 Jeremy Goodman
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