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The basic idea in this Letter is the assumption that masses of the galactic constituents (particles of short-living fluctuations) may be functions of strength of the gravitational field. They may be in galactic space heavier than in the…

综合物理 · 物理学 2015-01-30 V. Majernik

Modified gravity is one of the most promising candidates for explaining the current accelerating expansion of the Universe, and even its unification with the inflationary epoch. Nevertheless, the wide range of models capable to explain the…

广义相对论与量子宇宙学 · 物理学 2015-06-03 Álvaro de la Cruz-Dombriz , Diego Sáez-Gómez

In the last years, we saw more and more attempts to explain dark matter as a general relativistic effect, at least for some fraction. Following this philosophy, we considered the gravitational distortions due to the inhomogeneous…

广义相对论与量子宇宙学 · 物理学 2020-06-02 Federico Re

Modified Gravity (MOG) has been used successfully to explain the rotation curves of galaxies, the motion of galaxy clusters, the Bullet Cluster, and cosmological observations without the use of dark matter or Einstein's cosmological…

宇宙学与河外天体物理 · 物理学 2015-03-17 J. W. Moffat

We review progress in understanding dark matter by astrophysics, and particularly via the effect of gravitational lensing. Evidence from many different directions now all imply that five sixths of the material content of the universe is in…

宇宙学与河外天体物理 · 物理学 2015-05-14 Richard Massey , Thomas Kitching , Johan Richard

The existence of dark matter is supported by multiple astrophysical observations, yet its particle nature remains unknown. The development of gravitational wave astronomy, especially with future space-based detectors such as LISA, provides…

宇宙学与河外天体物理 · 物理学 2026-03-10 Yuezhe Chen , Pan-Pan Wang , Bo Wang , Rui Luo , Cheng-Gang Shao

We push ahead the idea developed in [24], that some fraction of the dark matter and the dark energy can be explained as a relativistic effect. The inhomogeneity matter generates gravitational distortions, which are general relativistically…

广义相对论与量子宇宙学 · 物理学 2021-05-12 Federico Re

Recently, an interesting gravitational model was proposed in order to mimic the effect of Dark Matter. Chamseddine and Mukhanov in the arXiv preprint 1308.5410 have separated the conformal mode of a physical metric in the form of a squared…

广义相对论与量子宇宙学 · 物理学 2013-12-02 Alexey Golovnev

The apparent missing mass in galaxies and galaxy clusters, commonly viewed as evidence for dark matter, could possibly originate from gradients in the gravitational coupling parameter, $G$, and active gravitational mass, $M_{act}$, rather…

广义相对论与量子宇宙学 · 物理学 2022-04-05 Meir Shimon

Massive gravity with second and fourth derivatives is shown to give both attractive and repulsive gravities. In contrast to the attractive gravity correlated with the energy-momentum tensor, the repulsive gravity is related to a fixed mass…

天体物理学 · 物理学 2007-05-23 Xiang-Song Chen

There is evidence that Newton and Einstein's theories of gravity cannot explain the dynamics of a universe made up solely of baryons and radiation. To be able to understand the properties of galaxies, clusters of galaxies and the universe…

天体物理学 · 物理学 2014-02-18 T. G Zlosnik , P. G Ferreira , G. D Starkman

The arguments connecting detections of a reason of difficulties of a solution of a problem of a cold dark matter are adduced.

高能物理 - 唯象学 · 物理学 2010-07-26 V. P. Efrosinin

The gravitational field of an isolated, axisymmetric flat disk of spinning dust is calculated approximately in the weak-field limit of quasi-metric gravity. Boundary conditions single out the exponential disk as a "preferred" physical…

广义相对论与量子宇宙学 · 物理学 2024-03-26 Dag Østvang

Modifications of General Relativity generically contain additional degrees of freedom that can mediate forces between matter particles. One of the common manifestations of a fifth force in alternative gravity theories is a difference…

宇宙学与河外天体物理 · 物理学 2023-09-22 Camille Bonvin , Levon Pogosian

We show that Newton's gravitational potential, augmented by a logarithmic term, partly or wholly mitigates the need for dark matter. As a bonus, it also explains why MOND seems to work at galactic scales. We speculate on the origin of such…

广义相对论与量子宇宙学 · 物理学 2022-12-07 Saurya Das , Sourav Sur

In astro-ph/0601489, within the framework of the Einsteinian general relativity, we made the observation that if the universe is described by a spatially flat Friedmann-Robertson-Walker (FRW) cosmology with Einsteinian cosmological constant…

天体物理学 · 物理学 2007-05-23 D. V. Ahluwalia-Khalilova

We explain the effect of dark matter (flat rotation curve) using modified gravitational dynamics. We investigate in this context a low energy limit of generalized general relativity with a nonlinear Lagrangian ${\cal L}\propto R^n$, where…

天体物理学 · 物理学 2008-11-26 Andrzej Borowiec , Wlodzimierz Godlowski , Marek Szydlowski

We show that in cosmology the gravitational action of the far away matter has quite relevant effects, if retardation of the forces and discreteness of matter (with its spatial correlation) are taken into account. The expansion rate is found…

宇宙学与河外天体物理 · 物理学 2009-08-03 A. Carati , S. L. Cacciatori , L. Galgani

We investigate the possibility that the observed behavior of test particles outside galaxies, which is usually explained by assuming the presence of dark matter, is the result of the dynamical evolution of particles in higher dimensional…

广义相对论与量子宇宙学 · 物理学 2009-04-21 M. E. Kahil , T. Harko

Recently, the static spherically symmetric solution of the gravitational field equations have been found in theories describing massive graviton with spontaneous breaking of the Lorentz invariance. These solutions, which show off two…

广义相对论与量子宇宙学 · 物理学 2009-05-07 Michael V. Bebronne