中文
相关论文

相关论文: Rotation curves of galaxies in GR

200 篇论文

We present a method to investigate relativistic effects arising from large masses. The method is non-perturbative and employs a mean-field approximation and gravitational lensing. Using this method and a basic model of disk galaxy, we find…

星系天体物理 · 物理学 2021-03-17 Alexandre Deur

Two classes of stationary axisymmetric solutions of Einstein's equations for isolated differentially rotating matter sources are presented. The asymptotic regime is extracted, with attention to quasilocal gravitational energy, shear and…

广义相对论与量子宇宙学 · 物理学 2025-06-12 Marco Galoppo , David L. Wiltshire

We use the concept of the spiral rotation curves universality to investigate the luminous and dark matter properties of the dwarf disc galaxies in the local volume (size $\sim11$ Mpc). Our sample includes 36 objects with rotation curves…

星系天体物理 · 物理学 2017-01-09 Ekaterina V. Karukes , Paolo Salucci

We investigate effects of massive graviton on the rotation curves of the Milky Way, spiral galaxies and Low Surface Brightness~(LSB) galaxies. Using a simple de Rham, Gabadadze, and Tolley (dRGT) massive gravity model, we find static…

广义相对论与量子宇宙学 · 物理学 2018-09-19 Sirachak Panpanich , Piyabut Burikham

A better understanding of the formation of mass structures in the universe can be obtained by determining the amount and distribution of dark and luminous matter in spiral galaxies. To investigate such matters a sample of 12 galaxies, most…

星系天体物理 · 物理学 2015-06-23 Roelof Bottema , Jose Luis G. Pestana

Non-baryonic Dark Matter (DM) appears in galaxies and other cosmic structures when and only when the acceleration of gravity, as computed considering only baryons, goes below a well defined value a0=1.2e-8 cm/s/s. This might indicate a…

天体物理学 · 物理学 2009-11-11 Riccardo Scarpa , Gianni Marconi , Roberto Gilmozzi

We focus on a modified version of Horava - Lifschitz theory and, in particular, we consider the impact of its weak - field static spherically symmetric limit on the galaxy dynamics. In a previous paper, we used the modified gravitational…

宇宙学与河外天体物理 · 物理学 2015-06-04 Vincenzo F. Cardone , Monica Capone , Ninfa Radicella , Matteo L. Ruggiero

Equations of motion, in cylindrical co-ordinates, for the observed rotation of gases within the gravitational potential of spiral galaxies have been derived from Carmeli's Cosmological General Relativity theory. A Tully-Fisher type relation…

天体物理学 · 物理学 2007-05-23 John G. Hartnett

The rotation curves of 20 spiral galaxies are examined in the light of a toy model (Soares 1992) which has as the main feature the assignment of a high M/L ratio (=30; Ho=50 km/s/Mpc) to the visible matter. The observed rotation of all…

天体物理学 · 物理学 2009-09-25 D. S. L. Soares

It is shown that the cosmological constant links the roots both of General Relativity and Newtonian gravity via the general function satisfying Newton's theorem according to which the gravitating sphere acts as a point mass situated in its…

广义相对论与量子宇宙学 · 物理学 2019-01-10 V. G. Gurzadyan

Dark matter is the generally accepted paradigm in astrophysics and cosmology as a solution to the higher rate of rotation in galaxies, among many other reasons. But since there are still some problems encountered by the standard dark matter…

星系天体物理 · 物理学 2021-02-24 Hanna A. Sabat , Raed Z. Bani-Abdoh , Marwan S. Mousa

An impact model of gravity designed to emulate Newton's law of gravitation is applied to the radial acceleration of disk galaxies. Based on this model (Wilhelm et al. 2013), the rotation velocity curves can be understood without the need to…

星系天体物理 · 物理学 2017-09-11 K. Wilhelm , B. N. Dwivedi

In the framework of the unimodular metagravity, with the scalar graviton/graviscalar dark matter, a regular anomalous one-parameter solution to the static spherically symmetric metagravity equations in empty space is found. The solution…

广义相对论与量子宇宙学 · 物理学 2010-10-19 Yu. F. Pirogov

We use the galaxy rotation curves in the SPARC database to compare 9 different dark matter and modified gravity models on an equal footing, paying special attention to the stellar mass-to-light ratios. We compare three non-interacting dark…

星系天体物理 · 物理学 2021-11-24 Nicolas Loizeau , Glennys R. Farrar

Gravitational decoherence (GD) refers to the effects of gravity in actuating the classical appearance of a quantum system. Because the underlying processes involve issues in general relativity (GR), quantum field theory (QFT) and quantum…

广义相对论与量子宇宙学 · 物理学 2024-06-19 Charis Anastopoulos , Bei-Lok Hu

The existence of the flat rotation curves of galaxies is still perplexing. The dark matter paradigm was proposed long ago to solve this conundrum; however, this proposal is still under debate. In this paper, we search for universal…

星系天体物理 · 物理学 2022-10-25 G. Pascoli

Galactic rotation curves exhibit diverse behavior in the inner regions, while obeying an organizing principle, i.e., they can be approximately described by a radial acceleration relation or the Modified Newtonian Dynamics phenomenology. We…

星系天体物理 · 物理学 2019-08-14 Tao Ren , Anna Kwa , Manoj Kaplinghat , Hai-Bo Yu

Starting with the conceptual foundation of general relativity (GR) - equivalence principle, space-time geometry and special relativity, I train cross hairs on two characteristic predictions of GR - black holes and gravitational waves. These…

广义相对论与量子宇宙学 · 物理学 2015-09-23 Patrick Das Gupta

Recent observations have revealed the structural properties of the dark and luminous mass distribution in spirals. These results led to the vision of a new and amazing scenario. The investigation of single and coadded objects has shown that…

星系天体物理 · 物理学 2015-04-13 Paolo Salucci , Mariafelicia De Laurentis

We analyze the dynamics of a single spiral galaxy from a general relativistic viewpoint. We employ the known family of stationary axially-symmetric solutions to Einstein gravity coupled with dust in order to model the halo external to the…

广义相对论与量子宇宙学 · 物理学 2022-07-13 Davide Astesiano , Sergio L. Cacciatori , Federico Re