中文
相关论文

相关论文: Dynamical Shortcomings in the Generalized SU(2) Pr…

200 篇论文

We discuss cosmology based on a Cuscuta-Galileon gravity theory, which preserves just two degrees of freedom. Although there exists no additional degrees of freedom, introduction of a potential of a scalar field changes the dynamics. The…

广义相对论与量子宇宙学 · 物理学 2022-05-17 Kei-ichi Maeda , Sirachak Panpanich

We describe the dynamics of strongly coupled field theories in de Sitter spacetime using the holographic gauge/gravity duality. The main motivation for this is to explore the possibility of dynamical phase transitions during cosmological…

高能物理 - 理论 · 物理学 2011-04-28 Donald Marolf , Mukund Rangamani , Mark Van Raamsdonk

The impact of topological terms that modify the Hilbert-Einstein action is here explored by virtue of a further $f(G)$ contribution. In particular, we investigate the phase-space stability and critical points of an equivalent scalar field…

广义相对论与量子宇宙学 · 物理学 2025-05-01 Giannis Papagiannopoulos , Orlando Luongo , Genly Leon , Andronikos Paliathanasis

Dynamical systems methods are used to investigate dynamics of a flat Friedmann-Robertson-Walker cosmological model with the non-minimally coupled scalar field and a potential function. Performed analysis distinguishes the value of…

广义相对论与量子宇宙学 · 物理学 2020-09-07 Orest Hrycyna

In this letter we apply dynamical system methods to study all evolutional paths admissible for all initial conditions of the FRW cosmological model with a non-minimally coupled to gravity scalar field and a barotropic fluid. We choose…

天体物理学 · 物理学 2011-07-13 Marek Szydlowski , Orest Hrycyna

In the context of the new standard LambdaCDM cosmology we resolve conflicts in the literature regarding fundamental aspects of the expansion of the universe and cosmic horizons and we link these concepts to observational tests. We derive…

天体物理学 · 物理学 2007-05-23 Tamara M. Davis

We have performed the dynamical system analysis to obtain the critical point in which, the value of the geometric and dynamical parameters satisfy the late-time cosmic behavior of the Universe. At the outset, the modified Friedmann…

广义相对论与量子宇宙学 · 物理学 2025-10-30 Rahul Bhagat , B. Mishra

In the present mainstream cosmology, matter and spacetime emerged from a singularity and evolved through four distinct periods: early inflation, radiation, dark matter and late-time inflation (driven by dark energy). During the radiation…

宇宙学与河外天体物理 · 物理学 2013-10-02 E. L. D. Perico , J. A. S. Lima , Spyros Basilakos , Joan Sola

A new cosmic scenario with gravitationally induced particle creation is proposed. In this model the Universe evolves from an early to a late time de Sitter era, with the recent accelerating phase driven only by the negative creation…

广义相对论与量子宇宙学 · 物理学 2015-06-22 J. A. S. Lima , L. L. Graef , D. Pavón , S. Basilakos

In the present lore of cosmology, matter and space-time emerged from a singularity and evolved through four different regimes: inflation, radiation, dark matter and dark energy dominated eras. In the radiation and dark matter dominated…

宇宙学与河外天体物理 · 物理学 2011-06-13 J. A. S. Lima , S. Basilakos

We study the evolution of homogeneous and isotropic, flat cosmological models within the general scalar-tensor theory of gravity with arbitrary coupling function and potential. After introducing the limit of general relativity we describe…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Laur Jarv , Piret Kuusk , Margus Saal

We have used the dynamical system approach in order to investigate the dynamics of cosmological models of the flat Universe with a non-minimally coupled canonical and phantom scalar field and the Ratra-Peebles potential. Applying methods of…

广义相对论与量子宇宙学 · 物理学 2019-09-27 Franciszek Humieja , Marek Szydlowski

We formulate a generalized $k$-essence model in the presence of a Palatini $f(\mathcal{R})$ gravitational sector. In the corresponding biscalar-tensor theory, we discuss the distinguished dynamical properties of the two scalar fields,…

广义相对论与量子宇宙学 · 物理学 2026-04-15 Fabio Moretti , Flavio Bombacigno

The standard big bang cosmology has been greatly successful in explaining many observational aspects of the real universe. However, two particular diffficulties faced by it are the so-called ``horizon'' and ``flatness'' problems. By…

综合物理 · 物理学 2007-05-23 Abhas Mitra

In this work we study the phase-space analysis of generalized Rastall gravity (GRG) which has recently been introduced as a modification to the original version of Rastall gravity (RG). In GRG, the coupling parameter assumes a dynamical…

广义相对论与量子宇宙学 · 物理学 2022-06-01 Hamid Shabani , Hooman Moradpour , Amir Hadi Ziaie

We study cosmic evolution based on the fixed points in the dynamical analysis of the Degenerate Higher-Order Scalar-Tensor (DHOST) theories. We consider the DHOST theory in which the propagation speed of gravitational waves is equal to the…

宇宙学与河外天体物理 · 物理学 2022-05-10 Wittaya Thipaksorn , Khamphee Karwan

We study gravitational theories with a cosmological constant and the Gauss-Bonnet curvature squared term and analyze the possibility of de Sitter expanding spacetime with a constant internal space. We find that there are two branches of the…

高能物理 - 理论 · 物理学 2015-06-19 Kei-ichi Maeda , Nobuyoshi Ohta

Homogeneous isotropic spatial flat cosmological models with two torsion functions in vacuum are built and investigated in the framework of de Sitter gauge theory of gravity. It is shown that by certain choices of parameters of gravitational…

广义相对论与量子宇宙学 · 物理学 2011-10-18 Guo-Ying Qi

The $f(T)$ gravity is one of the extensions of teleparallel equivalent of general relativity, in which more general functions of the torsion scalar $T$ can be described. With the proposed functional form of $f(T) = \alpha T - \beta u^{-n} +…

广义相对论与量子宇宙学 · 物理学 2026-04-14 Suraj Kumar Behera , S. A. Kadam , Pratik P. Ray , B. Mishra

We study in detail the phase space of a Friedmann-Robertson-Walker Universe filled with various cosmological fluids which may or may not interact. We use various expressions for the equation of state, and we analyze the physical…

广义相对论与量子宇宙学 · 物理学 2017-09-13 S. D. Odintsov , V. K. Oikonomou , Petr V. Tretyakov