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相关论文: Constraints on Modified Gravity Models from White …

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We investigate the modified gravity theories in terms of the effective dark energy models. We compare the cosmic expansion history and the linear growth in different models. We also study the evolution of linear cosmological perturbations…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Seokcheon Lee

Gravitational waves have been shown to provide new constraints on gravitational theories beyond general relativity (GR), especially in the strong field regime. Gravitational wave signals from galactic double white dwarfs, expected to be…

广义相对论与量子宇宙学 · 物理学 2024-09-27 Shu Yan Lau , Kent Yagi , Phil Arras

The missing gravity in galaxies requires dark matter, or alternatively a modification of gravity or inertia. These theoretical possibilities of fundamental importance may be distinguished by the statistical relation between the observed…

星系天体物理 · 物理学 2022-12-21 Kyu-Hyun Chae

Over the last few decades, a plethora of modifications to general relativity have been proposed to solve a host of cosmological and astrophysical problems. Many modified gravity models are now ruled out with further astrophysical…

广义相对论与量子宇宙学 · 物理学 2023-11-15 Surajit Kalita , Shruti Bhatporia , Amanda Weltman

We investigate the application of an equation of state that incorporates corrections derived from the Snyder model (and the Generalized Uncertainty Principle) to describe the behavior of matter in a low-mass star. Remarkably, the resulting…

广义相对论与量子宇宙学 · 物理学 2023-12-05 Anna Pachoł , Aneta Wojnar

Modified theories of gravity usually present new degrees of freedom, as well as higher order derivatives, wrong signs in certain terms and complicated couplings already present in the Lagrangian from the beginning or originated by the field…

广义相对论与量子宇宙学 · 物理学 2022-07-28 Adrià Delhom , Alejandro Jiménez-Cano , Francisco José Maldonado Torralba

There is a growing interest in investigating modified theories of gravity, primarily, with the aim of explaining the universe's accelerated expansion, which has been confirmed by several independent observations. Compact objects, like…

广义相对论与量子宇宙学 · 物理学 2021-08-16 K Nobleson , Tuhin Malik , Sarmistha Banik

In the context of the non-relativistic theories, a generalization of the Chern--Weil-theorem allows us to show that extended Chern--Simons actions for gravity in d=4 invariant under some specific non-relativistic groups lead to modified…

高能物理 - 理论 · 物理学 2018-11-06 G. Rubio , P. Salgado

The modified Gauss-Bonnet gravity can be motivated by a number of physical reasons, including: the uniqueness of a gravitational Lagrangian in four and higher dimensions and the leading order $\alpha^\prime$ corrections in superstring…

高能物理 - 理论 · 物理学 2017-08-23 Ishwaree P. Neupane

In this paper, we explore the properties of white dwarfs with the modified TOV equation in Einstein-$\Lambda$ gravity, the equilibrium configurations predict a maximum mass limit for white dwarfs same as the Chandrasekhar limit when we…

广义相对论与量子宇宙学 · 物理学 2019-02-27 H. L. Liu , G. L. Lü

Mimetic gravity is a modified theory of gravity which is able to incorporate dark matter into the underlying geometry of space-time by isolating the conformal degree of freedom. The theory has been studied extensively in the cosmological…

广义相对论与量子宇宙学 · 物理学 2023-12-08 Leonid Sarieddine

Model-independent parametrisations of modified gravity have attracted a lot of attention over the past few years; numerous combinations of experiments and observables have been suggested to constrain these parameterisations, and future…

宇宙学与河外天体物理 · 物理学 2011-07-13 D. B. Thomas

Modified gravity theories generically predict a violation of Lorentz invariance, which may lead to a modified dispersion relation for propagating modes of gravitational waves. We construct a parametrized dispersion relation that can…

广义相对论与量子宇宙学 · 物理学 2014-12-02 Saeed Mirshekari , Nicolas Yunes , Clifford M. Will

The prediction of the spins of the compact remnants is a fundamental goal of the theory of stellar evolution. Here, we confront the predictions for white dwarf spins from evolutionary models including rotation with observational…

天体物理学 · 物理学 2009-11-13 M. P. L. Suijs , N. Langer , A. -J. Poelarends , S. -C. Yoon , A. Heger , F. Herwig

The mass-radius relation of white dwarfs is largely determined by the equation of state of degenerate electrons, which causes the stellar radius to decrease as mass increases. Here we observationally measure this relation using the…

太阳与恒星天体物理 · 物理学 2020-08-27 Vedant Chandra , Hsiang-Chih Hwang , Nadia L. Zakamska , Sihao Cheng

There are a few different mechanisms that can cause white dwarf stars to vary in brightness, providing opportunities to probe the physics, structures, and formation of these compact stellar remnants. The observational characteristics of the…

太阳与恒星天体物理 · 物理学 2025-02-20 Keaton J. Bell

The Dolgov-Kawasaki instability discovered in the matter sector of the modified gravity scenario incorporating a 1/R correction to Einstein gravity is studied in general f(R) theories. A stability condition is found in the metric version of…

天体物理学 · 物理学 2008-11-26 Valerio Faraoni

Chameleon fields may modify gravity on cluster scales while recovering general relativity locally. This article reviews signatures of chameleon modifications in the nonlinear cosmological structure, comparing different techniques to model…

宇宙学与河外天体物理 · 物理学 2015-01-06 Lucas Lombriser

Disformal theories of gravity are scalar-tensor theories where the scalar couples derivatively to matter via the Jordan frame metric. These models have recently attracted interest in the cosmological context since they admit accelerating…

广义相对论与量子宇宙学 · 物理学 2015-11-04 Hiu Yan Ip , Jeremy Sakstein , Fabian Schmidt

In this paper, we analyze the clustering of galaxies using a modified theory of gravity, in which the field content of general relativity has been be increased. This increasing in the field content of general relativity changes the large…

广义相对论与量子宇宙学 · 物理学 2019-11-06 Mir Hameeda , Behnam Pourhassan , Mir Faizal , C. P. Masroor , Rizwan Ul Haq Ansari , P. K. Suresh
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