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Einstein gravity coupled to a massive skew symmetric field F_{\mu\nu\lambda} leads to an acceleration law that modifies the Newtonian law of attraction between particles. We use a framework of non-perturbative renormalization group…

天体物理学 · 物理学 2009-11-10 J. W. Moffat

In the weak field approximation, the nonsymmetric gravitational theory (NGT) has, in addition to the Newtonian gravitational potential, a Yukawa-like potential produced by the exchange of a spin $1^+$ boson between fermions. If the range…

天体物理学 · 物理学 2010-11-30 J. W. Moffat , I. Yu. Sokolov

In the weak field approximation, the nonsymmetric gravitational theory has, in addition to the Newtonian gravitational potential, a Yukawa potential produced by the exchange of a spin $1^+$ boson between fermions. If the range $r_0$ is of…

天体物理学 · 物理学 2015-06-24 J. W. Moffat

We apply the modified acceleration law obtained from Einstein gravity coupled explaining galaxy rotation curves without exotic dark matter. Our sample of galaxies includes low surface brightness (LSB) and high surface brightness (HSB)…

天体物理学 · 物理学 2016-08-30 J. R. Brownstein , J. W. Moffat

Rotation curves of spiral galaxies are known with reasonable precision for a large number of galaxies with similar morphologies. The data implies that non-Keplerian fall--off is seen. This implies that (i) large amounts of dark matter must…

天体物理学 · 物理学 2011-05-23 C. Rodrigo-Blanco , J. Pérez-Mercader

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

The equation of motion in the generally covariant modified gravity (MOG) theory leads for weak gravitational fields and the non-relativistic limit to a modification of the Newtonian gravitational acceleration law, expressed in terms of two…

星系天体物理 · 物理学 2016-10-31 J. W. Moffat

It was recently proposed that the effects usually attributed to particle dark matter on galaxy scales are due to the displacement of dark energy by baryonic matter, a paradigm known as emergent gravity. This formalism leads to predictions…

星系天体物理 · 物理学 2017-03-22 Aurelien Hees , Benoit Famaey , Gianfranco Bertone

The observed flat rotation curves of galaxies require either the presence of dark matter in Newtonian gravitational potentials or a significant modification to the theory of gravity at galactic scales. Detecting relativistic Doppler shifts…

星系天体物理 · 物理学 2012-02-15 Alan Cooney , Dimitrios Psaltis , Dennis Zaritsky

We study the possibility that galactic rotation curves can be explained by a gravitational potential that contains a linear term as well as a Newtonian one. This hypothesis, suggested by conformal gravity, does allow good fits to the…

天体物理学 · 物理学 2007-05-23 Carl E. Carlson , Eric J. Lowenstein

We investigate the proof of concept and the implications of \textit{refracted gravity}, a novel modified gravity aimed to solve the discrepancy between the luminous and the dynamical mass of cosmic structures without resorting to dark…

星系天体物理 · 物理学 2016-03-17 Titos Matsakos , Antonaldo Diaferio

The GRT modification taking into account the dependence of metric on the velocities of the sources is built. It is shown that this dependence follows from the equivalence principle and from the inseparability of the field equations and…

综合物理 · 物理学 2010-01-12 Sergey Siparov

The equation of motion in the generally covariant modified gravity (MOG) theory leads, for weak gravitational fields and non-relativistic motion, to a modification of Newton's gravitational acceleration law. In addition to the metric…

广义相对论与量子宇宙学 · 物理学 2019-05-24 M. A. Green , J. W. Moffat

While the standard and most popular explanation for the flatness of galaxy rotation curves is dark matter, one cannot at this stage rule out an explanation based on a modified law of gravitation, which agrees with Newtonian gravitation on…

星系天体物理 · 物理学 2012-06-18 Priti Mishra , Tejinder P. Singh

MOG is a fully relativistic modified theory of gravity based on an action principle. The MOG field equations are exactly solvable numerically in two important cases. In the spherically symmetric, static case of a gravitating mass, the…

广义相对论与量子宇宙学 · 物理学 2010-11-25 J. W. Moffat , V. T. Toth

Flat galaxy rotation curves and the accelerating Universe both imply the existence of a critical acceleration, which is of the same order of magnitude in both the cases, in spite of the galactic and cosmic length scales being vastly…

广义相对论与量子宇宙学 · 物理学 2012-07-16 Priti Mishra , Tejinder P. Singh

We consider the consequences of applying general relativity to the description of the dynamics of a galaxy, given the observed flattened rotation curves. The galaxy is modeled as a stationary axially symmetric pressure-free fluid. In spite…

天体物理学 · 物理学 2010-10-27 F. I. Cooperstock , S. Tieu

Globular clusters (GCs) in the Milky Way have characteristic velocity dispersions that are consistent with the predictions of Newtonian gravity, and may be at odds with Modified Newtonian Dynamics (MOND). We discuss a modified gravity (MOG)…

天体物理学 · 物理学 2008-06-14 J. W. Moffat , V. T. Toth

A modified gravitational theory explains early universe and late time cosmology, galaxy and galaxy cluster dynamics. The modified gravity (MOG) theory extends general relativity (GR) by three extra degrees of freedom: a scalar field $G$,…

广义相对论与量子宇宙学 · 物理学 2020-10-30 J. W. Moffat

As an alternative to dark matter models, MOdified Gravity (MOG) theory can compensate for dark matter by a covariant modification of Einstein gravity. The theory introduces two additional scalar fields and one vector field. The aim is to…

星系天体物理 · 物理学 2015-06-16 J. W. Moffat , S. Rahvar
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