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相关论文: Particle Production in f(R) Gravity during Structu…

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While vector modes are usually ignored in cosmology since they are not produced during inflation they are inevitably produced from the interaction of density fluctuations of differing wavelengths. This effect may be calculated via a…

天体物理学 · 物理学 2008-12-18 Teresa Hui-Ching Lu , Kishore Ananda , Chris Clarkson

In this paper, we investigate and analyze the cosmological dynamics of the universe, with an effect of modified $f(R)$ gravity emerging at cosmological scale. We choose the Einstein frame as a physical frame. We consider phase portraits of…

天体物理学 · 物理学 2007-05-23 Daris Samart

Cosmic rays are thought to escape their sources streaming along the local magnetic field lines. We show that this phenomenon generally leads to the excitation of both resonant and non-resonant streaming instabilities. The self-generated…

高能天体物理现象 · 物理学 2022-03-02 Benedikt Schroer , Oreste Pezzi , Damiano Caprioli , Colby Haggerty , Pasquale Blasi

We investigate a cosmological scenario in which the dark matter particles can be created during the evolution of the Universe. By regarding the Universe as an open thermodynamic system and using non-equilibrium thermodynamics, we examine…

宇宙学与河外天体物理 · 物理学 2022-09-20 Z. Safari , K. Rezazadeh , B. Malekolkalami

The formation of cosmic structures is an important diagnostic for both the dynamics of the cosmological model and the underlying theory of gravity. At the linear level of these structures, certain degeneracies remain between different…

宇宙学与河外天体物理 · 物理学 2019-08-02 Lavinia Heisenberg , Matthias Bartelmann

Non radial oscillations of neutron stars are associated with the emission of gravitational waves. The characteristic frequencies of these oscillations can be computed using the theory of stellar perturbations, and they are shown to carry…

广义相对论与量子宇宙学 · 物理学 2011-05-10 Valeria Ferrari

We study the gravitational production of heavy X-particles of mass of the order of the inflaton mass, produced after the end of inflation. We find that, in the presence of a derivative coupling of the inflaton field or of the X-field to the…

广义相对论与量子宇宙学 · 物理学 2015-06-16 George Koutsoumbas , Konstantinos Ntrekis , Eleftherios Papantonopoulos

We analyze the propagating degrees of freedom in gravity models where the scalar curvature in the action is replaced by a generic function $f(R)$ of the curvature. That these gravity models are equivalent to Einstein's gravity with an extra…

高能物理 - 理论 · 物理学 2007-05-23 Alvaro Nunez , Slava Solganik

We show explicitly that there is particle creation in a static spacetime. This is done by studying the field in a coordinate system based on a physical principle which has recently been proposed. There the field is quantized by decomposing…

高能物理 - 理论 · 物理学 2015-06-26 D. J. Lamb , A. Z. Capri , S. M. Roy

We investigate the scalar mode quadrupole radiation of gravitational waves in $F(R)$ modified gravity. In $F(R)$ gravity a massive scalar mode appears in the gravitational waves. We find explicit expressions for the quadrupole radiation and…

广义相对论与量子宇宙学 · 物理学 2023-07-19 Tomohiro Inagaki , Masahiko Taniguchi

We show that, due to the nonlinear nature of gravity, fluctuations in spacetime curvature generate additional gravitational attraction. This fluctuation-induced extra attraction was overlooked in the conventional understanding of the…

广义相对论与量子宇宙学 · 物理学 2024-01-09 Qingdi Wang

We investigate inflation within $f(R,\phi)$-theories, where a dynamical scalar field is coupled to gravity. A class of models which can support early-time acceleration with the emerging of an effective cosmological constant at high…

广义相对论与量子宇宙学 · 物理学 2018-12-13 R. Myrzakulov , L. Sebastiani , S. Vagnozzi

The present paper tries to answer the question: Can a de Sitter phase in presence of radiation be a competitor of the standard inflationary paradigm for the early universe? This kind of a de Sitter phase can exist in cosmological models…

广义相对论与量子宇宙学 · 物理学 2022-08-03 Kaushik Bhattacharya , Anirban Chatterjee , Saddam Hussain

We study the evolution of perturbations during the domination and decay of a massive particle species whose mass and decay rate are allowed to depend on the expectation value of a light scalar field. We specialize in the case where the…

天体物理学 · 物理学 2009-11-10 Filippo Vernizzi

Recently, the phenomenological description of cosmological particle production processes in terms of effective viscous pressures has attracted some attention. Using a simple creation rate model we discuss the question to what extent this…

广义相对论与量子宇宙学 · 物理学 2009-10-28 Josep Triginer , Winfried Zimdahl , Diego Pavon

The standard theory of cosmic structure formation posits that the present-day rich structure of the Universe developed through gravitational amplification of tiny matter density fluctuations generated in its very early history. Recent…

宇宙学与河外天体物理 · 物理学 2009-06-25 Naoki Yoshida

Motivated by their potential role as dark matter, we study the cosmological evolution of light scalar and vector fields non-minimally coupled to gravity. Our focus is on a situation where the dominant contribution to the energy density…

高能物理 - 唯象学 · 物理学 2020-03-04 Gonzalo Alonso Álvarez , Joerg Jaeckel , Thomas Hugle

It has been speculated that gravity could be an emergent phenomenon, with classical general relativity as an effective, macroscopic theory, valid only for classical systems at large temporal and spatial scales. As in classical continuum…

广义相对论与量子宇宙学 · 物理学 2015-06-24 Huan Yang , Larry R. Price , Nicolas D. Smith , Rana X Adhikari , Haixing Miao , Yanbei Chen

Cosmic rays (CRs) leave their sources mainly along the local magnetic field; in doing so they excite both resonant and nonresonant modes through streaming instabilities. The excitation of these modes leads to enhanced scattering and in turn…

高能天体物理现象 · 物理学 2021-06-10 Benedikt Schroer , Oreste Pezzi , Damiano Caprioli , Colby Haggerty , Pasquale Blasi

In this paper, I point out that there is a curvature singularity problem appearing on non-linear level that generally plagues f(R) models that modify Einstein gravity in the infrared. It is caused by the fact that for the effective scalar…

天体物理学 · 物理学 2008-11-26 Andrei V. Frolov
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