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相关论文: Rotation of galaxies and dark matter

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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

Galactic rotation curves have proven to be the testing ground for dark matter bounds in spiral galaxies of all morphologies. Dwarf galaxies serve as an increasingly interesting case of rotation curve dynamics due to their typically rising…

广义相对论与量子宇宙学 · 物理学 2018-01-10 James G. O'Brien , Thomas L. Chiarelli , Jeremy Dentico , Modestas Stulge , Brian Stefanski , Robert Moss , Spasen Chaykov

We wish to carry forward to higher dimensions the insightful and novel method of obtaining the Kerr metric proposed by one of us [Gen. Relativ. Gravit. 45, 2383 (2013)] for deriving the Myers-Perry rotating black hole metric. We begin with…

广义相对论与量子宇宙学 · 物理学 2022-06-30 Amin Aghababaie Dastgerdi , Behrouz Mirza , Naresh Dadhich

Recently, it has been suggested that the phenomenology of flat rotation curves observed at large radii in the equatorial plane of disk galaxies can be explained as a manifestation of General Relativity instead of the effect of Dark Matter…

星系天体物理 · 物理学 2022-09-21 Luca Ciotti

According to General Relativity, there are three factors namely mass, rotation and charge that can influence the path of light ray. Many authors showed that there is another factor which can influence the path of light ray namely…

广义相对论与量子宇宙学 · 物理学 2016-04-04 Sarani Chakrabortya , A. K. Sen

Context. Latest papers on the rotation curve of the Milky Way galaxy, i. e. Ou et al. (2024); Jiao et al. (2023); Sylos Labini et al. (2023) suggest a Keplerian decrease in the rotation curve. This behavior is not consistent with other…

星系天体物理 · 物理学 2025-08-01 Jozef Klačka , Michal Šturc

We investigate the properties of a galaxy similar to the Milky Way within the context of standard disk formation theory in a LCDM universe. Using the standard assumption that baryons conserve specific angular momentum when they collapse, we…

天体物理学 · 物理学 2007-05-23 Rachel S. Somerville

This paper investigates the trajectories of light beams in a Kerr metric, which describes the gravitational field in the neighborhood of a rotating black hole. After reduction by cyclic coordinates, this problem reduces to analysis of a…

动力系统 · 数学 2025-01-23 Ivan Bizyaev

The non-gauge vector field with as simple as possible Lagrangian (\ref{Lagrangian}) turned out an adequate tool for macroscopic description of the main properties of dark matter. The dependence of the velocity of a star on the radius of the…

广义相对论与量子宇宙学 · 物理学 2016-05-24 Boris E. Meierovich

The following is a comment on the recent letter by Iocco et al. (2015, arXiv:1502.03821) where the authors claim to have found "...convincing proof of the existence of dark matter...". The letter in question presents a compilation of recent…

星系天体物理 · 物理学 2015-03-26 R. Durazo , X. Hernandez , S. Mendoza

Dark matter, believed to be present in many galaxies, is interpreted as a hydrodynamical system in interaction with the gravitational field and with nothing else. The gravitational field of our Galaxy can be inferred from observation of…

广义相对论与量子宇宙学 · 物理学 2012-04-11 Christian Fronsdal , Thomas J. Wilcox

EGRET gamma-ray archival data used with GALPROP software show two ringlike structures in Milky Way Plane which roughly tally with distribution of stars ([1] & references therein). To understand fully the implications of this and similar…

天体物理学 · 物理学 2008-07-10 Dilip G. Banhatti

Recent results from gravitational lensing are combined with new modeling of the stellar velocity distributions in nearby galaxies to probe the connection between the luminous and the dark matter in elliptical galaxies. From analysing a…

天体物理学 · 物理学 2007-05-23 H. -W. Rix

For nearly a century, more mass has been measured in galaxies than is contained in the luminous stars and gas. Through continual advances in observations and theory, it has become clear that the dark matter in galaxies is not comprised of…

宇宙学与河外天体物理 · 物理学 2015-06-12 Louis E. Strigari

We have performed a statistical analysis of a sample of 1100 extra-galactic rotation measures (RMs) obtained from the literature. Using a subsample of approximately 800 reliable RMs we compute a rotation measure sky and determine reliable…

天体物理学 · 物理学 2007-05-23 M. Johnston-Hollitt , C. P. Hollitt , R. D. Ekers

An Adaptive Mesh Refinement cosmological resimulation is analyzed in order to test whether filamentary flows of cold gas are responsible for the build-up of angular momentum within a Milky Way like disk at z>=3. A set of algorithms is…

宇宙学与河外天体物理 · 物理学 2016-10-26 Henry Tillson , Julien Devriendt , Adrianne Slyz , Lance Miller , Christophe Pichon

In this work we study rotation curves of spiral galaxies using a model of dark matter based on a scalar-tensor theory of gravity. We show how to estimate the scalar field dark matter parameters using a sample of observed rotation curves.

星系天体物理 · 物理学 2012-10-26 Mario A. Rodriguez-Meza

The role of the parameter `$a$' associated with the Kerr metric which represents the angular momentum per unit mass of a rotating massive object has been converted into determining the rotationally induced quadrapole electric field outside…

广义相对论与量子宇宙学 · 物理学 2016-08-31 Sujan Sengupta

Gravitational redshift is being generally calculated without considering the rotation of a body. Neglecting the rotation, the geometry of space time can be described by using the spherically symmetric Schwarzschild geometry. Rotation has…

广义相对论与量子宇宙学 · 物理学 2013-10-04 Anuj Kumar Dubey , Asoke Kumar Sen

Dwarf satellite galaxies of the Milky Way appear to be gravitationally bound, but their stars' orbital motion seems too fast to allow this given their visible mass. This is akin to the larger-scale galaxy rotation problem. In this paper, a…

综合物理 · 物理学 2017-03-06 M. E. McCulloch