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相关论文: Revisiting galactic rotation curves given a noncom…

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Observational cosmology is entering an era in which high precision will be required in both measurement and data analysis. Accuracy, however, can only be achieved with a thorough understanding of potential sources of contamination from…

宇宙学与河外天体物理 · 物理学 2015-11-19 Assaf Ben-David , Sebastian von Hausegger , Andrew D. Jackson

In recent years Quantum Superstrings and Quantum Gravity approaches have come to rely on non differenciable spacetime manifolds. These throw up a noncommutative spacetime geometry and we consider the origin of mass and a related…

综合物理 · 物理学 2007-05-23 B. G. Sidharth

We study a family of parametric statistical models based on gamma distributions, which do give realistic descriptions for other stochastic porous media. Gamma distributions contain as a special case the exponential distributions, which…

天体物理学 · 物理学 2016-08-30 C. T. J. Dodson

We investigate the radial behavior of galactic rotation curves by a Fourth Order Gravity adding also the Dark Matter component. The Fourth Order Gravity is a Lagrangian containing the Ricci scalar, the Ricci and Riemann tensor, but the…

广义相对论与量子宇宙学 · 物理学 2015-05-28 A. Stabile , G. Scelza

A new method is developed which permits the reconstruction of the surface-density distribution in the galactic disk of finite radius from an arbitrary smooth distribution of the angular velocity via two simple quadratures. The existence of…

天体物理学 · 物理学 2009-11-07 N. R. Sibgatullin , A. A. Garcia , V. S. Manko

We consider a proposed alternative to quantum gravity, in which the spacetime metric is treated as classical, even while matter fields remain quantum. Consistency of the theory necessarily requires that the metric evolve stochastically.…

广义相对论与量子宇宙学 · 物理学 2024-07-23 Jonathan Oppenheim , Andrea Russo

We use the rotation curves of more than 100 disk galaxies to examine whether the structure of their surrounding dark halos is consistent with the universal density profile proposed by Navarro, Frenk & White (NFW profiles). Rotation curve…

天体物理学 · 物理学 2007-05-23 Julio F. Navarro

The rotation dynamics of spiral galaxies is modeled using a sum of two mass distributions: a spherical bulge and a thin disk. The density functions representing these mass distributions are calculated from the total angular momentum of the…

星系天体物理 · 物理学 2012-10-09 Louis Marmet

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

We note that galaxy-galaxy lensing by non-spherical galaxy halos produces a net anti-correlation between the shear of background galaxies and the ellipticity of foreground galaxies. This anti-correlation would contaminate the tomographic…

天体物理学 · 物理学 2009-11-11 Sarah Bridle , Filipe B. Abdalla

Noncommutative-like model (NC-like) is an interesting alternative inspired by string theory to understand and describe the velocity rotation curves of galaxies without the inclusion of dark matter particles. In a natural way, a Gaussian…

星系天体物理 · 物理学 2021-03-08 Juan J. Ancona-Flores , A. Hernandez-Almada , Miguel A. Garcia-Aspeitia

Circular velocities of stars and gas in galaxies generally do not decline in accordance with widely expected Keplerian fall-off in velocities further from the galactic nucleus. Two main groups of theories were proposed to explain the…

星系天体物理 · 物理学 2014-06-11 Konstantin Pavlovich , Alex Pavlovich , Alan Sipols

Gaussian random fields pervade all areas of science. However, it is often the departures from Gaussianity that carry the crucial signature of the nonlinear mechanisms at the heart of diverse phenomena, ranging from structure formation in…

统计力学 · 物理学 2015-06-05 T. H. Beuman , A. M. Turner , V. Vitelli

The presence of non--Gaussian features in the Cosmic Microwave Background (CMB) radiation maps represents one of the most long--awaited clues in the search for the actual structure of the primordial radiation, still needing confirmation.…

天体物理学 · 物理学 2009-10-22 Alejandro Gangui

Context. The cusp-core discrepancy is one of the major problems in astrophysics. It results from comparing the observed mass distribution of galaxies with the predictions of Cold Dark Matter simulations. The latter predict a cuspy density…

宇宙学与河外天体物理 · 物理学 2015-05-13 J. van Eymeren , C. Trachternach , B. S. Koribalski , R. -J. Dettmar

The rotation curves of low surface brightness galaxies provide a unique data set with which to test alternative theories of gravitation over a large dynamic range in size, mass, surface density, and acceleration. Many clearly fail,…

天体物理学 · 物理学 2015-06-24 Stacy McGaugh , Erwin de Blok

The Sphere Covering Inequality was introduced in \cite{GM} (\emph{Invent. Math.}, 2018) as a sharp geometric inequality that provides a lower bound for the total area of two distinct surfaces of Gaussian curvature 1. These surfaces are…

偏微分方程分析 · 数学 2025-10-22 Changfeng Gui , Amir Moradifam

Studies of weak gravitational lensing by large-scale structures require the measurement of the distortions introduced to the shapes of distant galaxies at the few percent level by anisotropic light deflection along the line of sight. To…

天体物理学 · 物理学 2009-11-07 Andrew W. Blain

We review some applications of noncommutative geometry to the study of transverse geometry of Riemannian foliations and discuss open problems.

微分几何 · 数学 2007-05-23 Yuri Kordyukov

In this paper, a Riemannian geometry of noncommutative super surfaces is developed which generalizes [4] to the super case. The notions of metric and connections on such noncommutative super surfaces are introduced and it is shown that the…

微分几何 · 数学 2022-12-29 Yong Wang , Tong Wu