中文
相关论文

相关论文: Rotation Curves of Spiral Galaxies and Large Scale…

200 篇论文

We investigate the possibility to explain theoretically the galaxy rotation curves by a gravitational potential in total absence of dark matter. To this aim an analytic fourth-order theory of gravity, nonminimally coupled with a massive…

广义相对论与量子宇宙学 · 物理学 2015-06-15 A. Stabile , S. Capozziello

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

The data of velocity rotation curve in spiral galaxies, almost for galaxies which have close central surface brightness, collapse onto a universal scaling function. Since scaling functions are the signature of emergence in complex systems…

星系天体物理 · 物理学 2012-01-17 Reza Torabi

We show quantitatively that an exact solution of Einstein's conformal gravity can explain very well the galactic rotation curves for a sample of 104 galaxies without need for dark matter or other exotic modification of gravity. The metric…

广义相对论与量子宇宙学 · 物理学 2019-06-13 Qiang Li , Leonardo Modesto

Rotation curves of spiral galaxies are the major tool for determining the distribution of mass in spiral galaxies. They provide fundamental information for understanding the dynamics, evolution and formation of spiral galaxies. We describe…

天体物理学 · 物理学 2019-02-25 Yoshiaki Sofue , Vera Rubin

The recent paper by Lee and Lee (2004) may strongly leave the impression that astronomers have established that the rotation curves of spiral galaxies are flat. We show that the old paradigm of Flat Rotation Curves lacks, today, any…

天体物理学 · 物理学 2008-11-26 P. Salucci , G. Gentile

The dark matter hypothesis, which is not called into question here, explains why typical rotation curves of spiral galaxies do not follow a Keplerian profile. It is however not sufficient in itself to explain why the whole matter…

星系天体物理 · 物理学 2019-06-13 Vincent Deledicque

We study a generalized Einstein theory with the following two criteria:{\it i}) on the solar scale, it must be consistent with the classical tests of general relativity, {\it ii}) on the galactic scale, the gravitational potential is a sum…

天体物理学 · 物理学 2010-11-01 Masakatsu Kenmoku , Yuko Okamoto , Kazuyasu Shigemoto

Galactic rotation curve is a powerful indicator of the state of the gravitational field within a galaxy. The flatness of these curves indicates the presence of dark matter in galaxies and their clusters. In this paper, we focus on the…

广义相对论与量子宇宙学 · 物理学 2023-11-28 Gayatri Mohan , Umananda Dev Goswami

We have investigated the stellar light distribution and the rotation curves of high-luminosity spiral galaxies in the local Universe. The sample contains 30 high-quality extended H alpha and HI rotation curves. The stellar disk scale-length…

宇宙学与河外天体物理 · 物理学 2011-10-11 I. A. Yegorova , A. Babic , P. Salucci , K. Spekkens , A. Pizzella

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

The dark matter accretion theory (around a central body) of the author on the basis of his 5-dimensional Projective Unified Field Theory (PUFT) is applied to the orbital motion of stars around the center of the Galaxy. The departure of the…

广义相对论与量子宇宙学 · 物理学 2009-11-07 E. Schmutzer

We present, in closed analytic form, a general stationary, slowly rotating black hole, which is solution to a large class of alternative theories of gravity in four dimensions. In these theories, the Einstein-Hilbert action is supplemented…

广义相对论与量子宇宙学 · 物理学 2011-10-27 Paolo Pani , Caio F. B. Macedo , Luis C. B. Crispino , Vitor Cardoso

We present an exact solution of the averaged Einstein's field equations in the presence of two real scalar fields and a component of dust with spherical symmetry. We suggest that the space-time found provides the characteristics required by…

广义相对论与量子宇宙学 · 物理学 2009-11-07 T. Matos , F. S. Guzman

The observed flat rotation curves of galaxies require either the presence of dark matter in Newtonian gravitational potentials or a significant modification to the theory of gravity at galactic scales. Detecting relativistic Doppler shifts…

星系天体物理 · 物理学 2012-02-15 Alan Cooney , Dimitrios Psaltis , Dennis Zaritsky

We show that in the Einstein-Cartan gravity it is possible to obtain a relation between Hubble's expansion and the global rotation (vorticity) of the Universe. Gravitational coupling can be reduced to dimensionless quantity of order unity,…

天体物理学 · 物理学 2008-11-26 D. Palle

In this paper we study consistent solutions of spherically symmetric space in metric f(R) gravity theory. Here we inversely obtain a generic action from metric solutions that describe flat rotation curves in spiral galaxies without dark…

广义相对论与量子宇宙学 · 物理学 2021-05-11 Solmaz Asgari , Reza Saffari

The spacetime satisfying the flat curve condition for galaxies is shown to be the zero mass limit of the dilaton blackhole with an exponential potential. We derive the geodesic equations and by studying rotational curves and light…

广义相对论与量子宇宙学 · 物理学 2019-03-06 Yen-Kheng Lim

Based on an exact solution of the Einstein field equations, it is proposed in this note that the dark-matter hypothesis could have led to the prediction of flat galactic rotation curves long before the discovery thereof by assuming that on…

广义相对论与量子宇宙学 · 物理学 2016-06-14 Peter K. F. Kuhfittig

The Galaxy rotation curve is usually assumed to be flat. However, some galaxies have rotation curves that are lower than the flat rotation curve. In our Galaxy the Keplerian rotation of interstellar clouds in the galactic longitude l=135…

星系天体物理 · 物理学 2020-01-08 Piotr Gnaciński
‹ 上一页 1 2 3 10 下一页 ›