中文
相关论文

相关论文: Galactic Potentials

200 篇论文

We argue that combined observations of galaxy rotation curves and gravitational lensing not only allow the deduction of a galaxy's mass profile, but also yield information about the pressure in the galactic fluid. We quantify this statement…

天体物理学 · 物理学 2008-11-26 Tristan Faber , Matt Visser

A galaxy is modeled as a stationary axially symmetric pressure-free fluid in general relativity. For the weak gravitational fields under consideration, the field equations and the equations of motion ultimately lead to one linear and one…

天体物理学 · 物理学 2007-05-23 F. I. Cooperstock , S. Tieu

We consider the singular configurations of gravitating gas [1] which could be used as a model for disk galaxies. The simplest steady configuration, which corresponds to rotation of stars around center gives flat rotational curve, provided…

天体物理学 · 物理学 2007-05-23 G. Pronko

A special form of the isotropic metric in cylindrical coordinates is used to construct what may be interpreted as the General Relativistic versions of some wellknown potential-density pairs used in Newtonian gravity to model…

天体物理学 · 物理学 2009-11-13 D. Vogt , P. S. Letelier

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

Dark matter has been a long-standing and important issue in physics, but direct evidence of its existence is lacking. This work aims to elucidate the mystery and show that the dark matter hypothesis is unnecessary. We can nicely reproduce…

星系天体物理 · 物理学 2023-03-07 Jau Tang , Qiang Tang

Many cosmological observations call for the existence of dark matter. The most direct evidence for dark matter is inferred from the measured flatness of galactic rotation curves. The latter is based on Newtonian gravity. Alternative…

广义相对论与量子宇宙学 · 物理学 2008-11-19 Aleksandar Rakic , Dominik J. Schwarz

We derive a simple, closed form expression for the potential of a thin exponential disk of stars interacting through gravitational potentials of the form $V(r)=-\beta /r+\gamma r/2$, the potential associated with fundamental sources in the…

高能物理 - 唯象学 · 物理学 2009-10-22 Philip D. Mannheim

A unified parametrization of the circular velocity, which accurately fits 850 galaxy rotation curves without needing in advance the knowledge of the luminous matter components, nor a fixed dark matter halo model, is proposed. A notable…

星系天体物理 · 物理学 2018-03-14 E. Lopez Fune

We investigate the possibility that the behavior of the rotational velocities of test particles gravitating around galaxies can be explained in the framework of modified gravity models with non-minimal matter-geometry coupling. Generally,…

广义相对论与量子宇宙学 · 物理学 2010-05-28 T. Harko

The circular velocities of the inner region of disk galaxies are predicted by standard physics but velocities beyond the stellar disks are not consistent with Newtonian physics if the material there is in stable circular orbits. However,…

星系天体物理 · 物理学 2023-09-19 Earl Schulz

The paths of stars in galaxies have circular velocity independent of their distance from the centre of the galaxy. Newtonian mechanics with a logarithmic potential has such paths. In relativity these paths can be taken to be geodesics and…

天体物理学 · 物理学 2011-04-04 Mark D. Roberts

The motion in a simple, time independent rational galactic potential is studied. The potential is a generalization of a two dimensional harmonic oscillator potential and can be considered to describe plane motion in the central parts of a…

混沌动力学 · 物理学 2013-03-05 Euaggelos E. Zotos

Dark matter, believed to be present in many galaxies, is interpreted as a hydrodynamical system in interaction with the gravitational field and nothing else. An equation of state determines the mass distribution and the associated…

宇宙学与河外天体物理 · 物理学 2011-06-14 Christian Fronsdal , Thomas J. Wilcox

In the currently accepted paradigm, dark matter is hypothesized as an explanation of the flat rotation curves of galaxies under the assumption of virialized orbits. The use of millisecond pulsar timing as a probe of Galactic dark matter…

星系天体物理 · 物理学 2021-04-21 Kiley Heflin , Richard Lieu

It is a well known fact that, in the absence of Dark Matter, the observation of the rotation curves of galaxies cannot be explained in terms of Newtonian gravity. Rotation curves become flat in the outer regions, in contrast to what is…

广义相对论与量子宇宙学 · 物理学 2022-11-01 Matteo Luca Ruggiero , Antonello Ortolan , Clive C. Speake

We review some recent work by Mannheim and O'Brien on the systematics of galactic rotation curves in the conformal gravity theory. In this work the conformal theory was applied to a comprehensive, high quality sample of spiral galaxies…

宇宙学与河外天体物理 · 物理学 2015-06-12 Philip D. Mannheim , James G. O'Brien

We explore the possibility that the entire departure of galactic rotational velocities from their luminous Newtonian expectation be cosmological in origin, and show that within the framework of conformal gravity (but not Einstein gravity…

天体物理学 · 物理学 2016-08-30 Philip D. Mannheim

A mysterious dark matter is supposed to exist in the galactic halos. In this contrast, we discuss the possibility of explaining the flat rotational velocity curves in f(R) gravity by solving field equations numerically in vacuum and for…

综合物理 · 物理学 2021-03-30 Muhammad Usman

In spherical symmetry, the gravitational potential is uniquely determined by the rotational velocity profile. Numerous galaxies exhibit a universal velocity profile from which a universal gravitational profile is inferred. When treating…

星系天体物理 · 物理学 2025-04-23 Andrés Aceña , Juan Barranco , Argelia Bernal , Ericson López