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The Newtonian gravitational constant $G$ obeys the dimensional relation $[G] [M] [a] = [v]^4$, where $M$, $a$, and $v$ denote mass, acceleration, and speed, respectively. Since the baryonic Tully-Fisher (BTF) and Faber-Jackson (BFJ)…

广义相对论与量子宇宙学 · 物理学 2018-07-11 Dimitris M. Christodoulou , Demosthenes Kazanas

We have recently shown that the baryonic Tully-Fisher (BTF) and Faber-Jackson (BFJ) relations imply that the gravitational "constant" $G$ in the force law vary with acceleration $a$ as $1/a$. Here we derive the converse from first…

星系天体物理 · 物理学 2018-11-26 Dimitris M. Christodoulou , Demosthenes Kazanas

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

Modified Newtonian Dynamics is an empirical modification to Poisson's equation which has had success in accounting for the `gravitational field' $\Phi$ in a variety of astrophysical systems. The field $\Phi$ may be interpreted in terms of…

广义相对论与量子宇宙学 · 物理学 2013-05-30 C. Skordis , T. G. Zlosnik

Gravitational waves are being shown to derive directly from Newtonian dynamics for a continuous mass distribution, e g compressible fluids or equivalent. It is shown that the equations governing a continuous mass distribution, i e the…

综合物理 · 物理学 2024-05-20 Peter Vadasz

The field equations of a generalized $f(R)$ type gravity model, in which there is an arbitrary coupling between matter and geometry, are obtained. The equations of motion for test particles are derived from a variational principle in the…

广义相对论与量子宇宙学 · 物理学 2009-05-26 T. Harko

The Newtonian approximation with a nonvanishing nonlocal background field is analyzed for the scalar-tensor nonlocal gravity and nonlocal Gauss-Bonnet gravity. For these two theories, our calculations show that the Newtonian gravitational…

广义相对论与量子宇宙学 · 物理学 2019-03-28 S. X. Tian , Zong-Hong Zhu

Newton's second law: "force = time-derivative of momentum", may also be defined for theories of gravitation endowing space-time with a curved metric. Thus, Einstein's assumption of a geodesic motion may be rewritten in that form, and it…

综合物理 · 物理学 2007-05-23 Mayeul Arminjon

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

We consider the gravitational potential and the gravitational rotation field generated by an spherical mass distribution with exponential density, when the force between any two mass elements is not the usual Newtonian one, but some general…

天体物理学 · 物理学 2007-05-23 Carlos Rodrigo-Blanco

The gravitational potential and the gravitational rotation field generated by a thin-disk mass distribution with exponential density are considered in the case when the force between any two mass elements is not the usual Newtonian one, but…

天体物理学 · 物理学 2007-05-23 Carlos Rodrigo-Blanco

An idealized "test" object in general relativity moves along a geodesic. However, if the object has a finite mass, this will create additional curvature in the spacetime, causing it to deviate from geodesic motion. If the mass is…

广义相对论与量子宇宙学 · 物理学 2020-03-30 Marius Oltean , Richard J. Epp , Carlos F. Sopuerta , Alessandro D. A. M. Spallicci , Robert B. Mann

A new formulation of MOND as a modified-potential theory of gravity is propounded. In effect, the theory dictates that the MOND potential phi produced by a mass distribution rho is a solution of the Poisson equation for the modified source…

宇宙学与河外天体物理 · 物理学 2014-11-20 Mordehai Milgrom

In this paper, we discuss the self-consistency condition for the spherical symmetric Klein-Gordon equation, and then discuss a natural possibility that gravity and weak coupling constants g_G and g_W may be defined after g_{EM}. In this…

高能物理 - 理论 · 物理学 2016-09-06 Miyuki Nishikawa

In this paper we directly constrain possible spatial variations of the Newtonian gravitational constant G over ranges 0.01-5 AU in various extrasolar multi-planet systems. By means of the third Kepler's law we determine the quantity \Gamma_…

广义相对论与量子宇宙学 · 物理学 2013-10-09 Lorenzo Iorio

We propose a Lagrangian formulation for a varying $G$ Newtonian-like theory inspired by the Brans-Dicke gravity. Rather than imposing an {\it ad hoc} dependence for the gravitational coupling, as previously done in the literature, in our…

广义相对论与量子宇宙学 · 物理学 2021-01-20 Júlio C. Fabris , Tales Gomes , Júnior D. Toniato , Hermano Velten

On the basis of the coincidence of the physical dimensions (in natural units $\hbar = c = 1$) of the Newton's gravitational constant $G_{N} $ and the phenomenological Fermi constant $G_{F} $ for weak interaction, it is suggested that there…

广义相对论与量子宇宙学 · 物理学 2017-07-27 E. A. Pashitskii , V. I. Pentegov

In the pursuit of a general formulation for a modified gravitational theory at the non-relativistic level and as an alternative to the dark matter hypothesis, we construct a model valid over a wide variety of astrophysical scales. Through…

星系天体物理 · 物理学 2011-12-13 S. Mendoza , X. Hernandez , J. C. Hidalgo , T. Bernal

A specific form of the inertial law is presented by which we can have some deeper insight into the essence of mass and inertia. In this modified theory, there is no need to keep the concept of absolute space and Newton's third law as…

经典物理 · 物理学 2007-05-23 Amir H. Abbassi , Amir M. Abbassi

In its canonical formulation, general relativity is subject to gauge transformations that are equivalent to space-time coordinate changes of general covariance only when the gauge generators, given by the Hamiltonian and diffeomorphism…

广义相对论与量子宇宙学 · 物理学 2023-10-31 Martin Bojowald , Erick I. Duque
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