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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

An accurate computational method is presented to determine the mass distribution in a rotating thin-disk galaxy from given rotation curve by applying Newtonian dynamics for an axisymmetrically rotating thin disk of finite size with or…

星系天体物理 · 物理学 2014-06-17 James Q. Feng , C. F. Gallo

By numerically solving the mass distribution in a rotating disk based on Newton's laws of motion and gravitation, we demonstrate that the observed flat rotation curves for most spiral galaxies correspond to exponentially decreasing mass…

星系天体物理 · 物理学 2011-08-17 James Q. Feng , C. F. Gallo

A mass distribution is analyzed in terms of classical gravitational field theory. Newton's law of gravitation is consistently applied on the assumption that the equivalence of energy and mass according to Einstein's theory of relativity is…

综合物理 · 物理学 2015-05-26 Helmut Kling

Given the dimensions (including thickness) of an axisymmetric galaxy, Newton's law is used in integral form to find the density distributions required to match a wide range of orbital speed profiles. Newton's law is not modified and no dark…

天体物理学 · 物理学 2009-09-25 Kenneth F. Nicholson

Given the dimensions (including thickness) of a galaxy, and its rotation profile, a method is shown that finds the mass and density distributions in the defined envelope that will cause that rotation profile with near-exact speed matches.…

天体物理学 · 物理学 2007-05-23 Kenneth F. Nicholson

The measured rotation velocity profiles of mature spiral galaxies are successfully described with a gravitational model consisting of a thin axisymmetric disk of finte radius. The disk is assumed uniformly thin but with variable radial mass…

天体物理学 · 物理学 2008-03-06 James Q. Feng , C. F. Gallo

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

We present an efficient, robust computational method for modeling the Newtonian dynamics for rotation curve analysis of thin-disk galaxies. For a disk galaxy with a typical flat rotation curve, our modeling results show that the surface…

星系天体物理 · 物理学 2015-05-27 James Q. Feng , C. F. Gallo

One obtains a Maxwell-like structure of gravitation by applying the weak-field approximation to the well accepted theory of general relativity or by extending Newton's laws to time-dependent systems. This splits gravity in two parts, namely…

广义相对论与量子宇宙学 · 物理学 2007-05-23 M. Tajmar , C. J. de Matos

Given the dimensions(including thickness) of an axisymmetric galaxy, Newton's law is used in integral form to find the density distributions required to match a wide range of orbital speed profiles. Newton's law is not modified and no…

天体物理学 · 物理学 2007-05-23 Kenneth F. Nicholson

This paper continues previous work on a novel alternative model of gravity, based on the theory of fractional-dimension spaces applied to Newton's law of gravitation. In particular, our Newtonian Fractional-Dimension Gravity is now applied…

广义相对论与量子宇宙学 · 物理学 2021-02-15 Gabriele U. Varieschi

The main purpose of this paper is to seek a mechanical interpretation of gravitational phenomena. We suppose that the universe may be filled with a kind of fluid which may be called the $\Omega (0)$ substratum. Thus, the inverse-square law…

综合物理 · 物理学 2017-12-29 Xiao-Song Wang

Gravitational force manifested in its affect on rotational velocity is what indicates the presence of dark matter in individual galaxies. Newtonian mechanics is generally used to derive the relationship between rotational velocity and…

综合物理 · 物理学 2007-05-23 D. M. Snyder

We study the statistics of the gravitational (Newtonian) force in a particular kind of weakly correlated distribution of point-like and unitary mass particles generated by the so-called Gauss-Poisson point process. In particular we extend…

天体物理学 · 物理学 2009-11-07 Andrea Gabrielli , Adolfo Paolo Masucci , Francesco Sylos Labini

The description of gravity in the form of an embedding theory is based on the hypothesis that our space-time is a four-dimensional surface in a flat ten-dimensional space. The choice of standard Einstein-Hilbert action leads in this case to…

广义相对论与量子宇宙学 · 物理学 2023-07-06 S. A. Paston , A. D. Kapustin

The relaxed motion of stars and gas in galactic discs is well approximated by a rotational velocity that is a function of radial position only, implying that individual components have lost any information about their prior states.…

星系天体物理 · 物理学 2020-02-11 John Herbert Marr

For mature spiral galaxies, the rotation velocities quickly increase from the galactic center and achieve a constant velocity from the core to the periphery. This dynamic behavior is described by models balancing Newtonian gravitational and…

天体物理学 · 物理学 2008-04-02 James Q. Feng , C. F. Gallo

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

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
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