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Considering galaxies as self - gravitating systems of many collisionless particles allows to use methods of statistical mechanics inferring the distribution function of these stellar systems. Actually, the long range nature of the…

宇宙学与河外天体物理 · 物理学 2014-02-04 V. F. Cardone , M. P. Leubner , A. Del Popolo

There should be two ways to describe the flat rotation curves of galaxies and cluster of galaxies. Either one can introduce a dark matter component for the matter filling the halo, or by modifying the gravity theory and give the flat…

广义相对论与量子宇宙学 · 物理学 2014-04-02 F. Shojai , A. Shojai

We work in the framework of an inflationary cold dark matter universe with cosmological constant, in which the cosmological inhomogeneities are considered as gravitational lenses for the CMB photons. This lensing deforms the angular…

天体物理学 · 物理学 2009-11-10 P. Cerdá-Durán , V. Quilis , D. Sáez

The theory of noncommutative geometry provides an interesting mathematical background for developing new physical models. In particular, it allows one to describe the classical Standard Model coupled to Euclidean gravity. However,…

数学物理 · 物理学 2014-09-05 Nicolas Franco , Michał Eckstein

Conformal gravity theory can explain observed flat rotation curves of galaxies without invoking hypothetical dark matter. Within this theory, we obtain a generic formula for the sizes of galaxies exploiting the stability criterion of…

广义相对论与量子宇宙学 · 物理学 2012-08-28 Kamal K. Nandi , Arunava Bhadra

This paper is a very brief and gentle introduction to non-commutative geometry geared primarily towards physicists and geometers. It starts with a brief historical description of the motivation for non-commutative geometry and then goes on…

高能物理 - 理论 · 物理学 2020-08-20 Ernesto Lupercio

In a sense of deformation quantization, noncommutative (NC) geometry introduces a quantum structure of spacetime. Using the twist-deformation formalism, we show that the dynamical effects of spacetime noncommutativity can amount to a…

高能物理 - 理论 · 物理学 2025-07-17 Dušan Đorđević , Dragoljub Gočanin

The noncommutative spectral action extends our familiar notion of commutative spaces, using the data encoded in a spectral triple on an almost commutative space. Varying a rather simple action, one can derive all of the standard model of…

高能物理 - 理论 · 物理学 2010-11-11 William Nelson , Joseph Ochoa , Mairi Sakellariadou

We investigate the influence of the nonextensive q-statistics and kinetic theory on galactic scales through the analysis of a devised sample of Spiral Rotation Curves. Largely supported by recent developments on the foundations of…

星系天体物理 · 物理学 2015-06-22 Christiane Frigerio Martins , Jose' Ademir Sales Lima , Pietro Chimenti

A new force is proposed in order to explain galactic rotation curves. CPT is chosen as the underlying symmetry of the new force because it is a universal spacetime symmetry. Local CPT transformations are presented for the Dirac field…

综合物理 · 物理学 2013-08-30 Kurt Koltko

I describe a new approach (developed in collaboration with D.E. Holz) to calculating the statistical distributions for magnification, shear, and rotation of images of cosmological sources due to gravitational lensing by mass inhomogeneities…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Robert M. Wald

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 measurements of gas velocity in the outer parts of high redshift galaxies suggest that steeply falling rotation curves may be common, or even universal, in these galaxies, in contrast to the near universal flat, non-declining…

星系天体物理 · 物理学 2024-07-24 Alistair H. Nelson , Peter R. Williams

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 theory of distributions in non-Riemannian spaces is used to obtain exact static thin domain wall solutions of Einstein-Cartan equations of gravity. Curvature $ \delta $-singularities are found while Cartan torsion is given by Heaviside…

广义相对论与量子宇宙学 · 物理学 2015-06-25 L. C. Garcia de Andrade

A Riemannian geometry of noncommutative n-dimensional surfaces is developed as a first step towards the construction of a consistent noncommutative gravitational theory. Historically, as well, Riemannian geometry was recognized to be the…

高能物理 - 理论 · 物理学 2008-11-26 M. Chaichian , A. Tureanu , R. B. Zhang , X. Zhang

Concordance cosmology points to a Universe of zero mean curvature, due to the inflation mechanism which occurred soon after the Big Bang, while along a relatively small number of lower redshift light paths where lensing events are observed,…

天体物理学 · 物理学 2014-11-18 Richard Lieu

Infall of cold dark matter on a galaxy may result in caustic rings where the particle density is enhanced. They may be searched for as features in the galactic rotation curves. Previous studies suggested the evidence for these caustic rings…

宇宙学与河外天体物理 · 物理学 2023-03-03 D. Davydov , S. Troitsky

We review the topic of rotation curves of spiral galaxies emphasizing the standard interpretation as evidence for the existence of dark matter halos. Galaxies other than spirals and late-type dwarfs may also possess great amounts of dark…

天体物理学 · 物理学 2007-05-23 Eduardo Battaner , Estrella Florido

Dark matter, a conjectured substance not directly observable but which has tremendous mass, was proposed to explain why galaxies hold together and rotate faster at their edges than predicted by Newton's Inverse Square (1/r2) Law of Gravity.…

星系天体物理 · 物理学 2013-05-30 Martin Wen-Yu Lo