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相关论文: Is Galaxy Dark Matter a Property of Spacetime?

200 篇论文

Observations show that for disk galaxies the fourth power of the circular velocity of stars around the core of the galaxy is proportional to the luminosity L. This is known as the Tully-Fisher law. Since L is proportional to the mass M of…

天体物理学 · 物理学 2007-05-23 Silvia Behar , Moshe Carmeli

We give an estimate of the gravitational field of force exerted on a test particle by the far galaxies, in the frame of the weak field approximation. In virtue of Hubble's law, the action of the far matter turns out to be non negligible,…

天体物理学 · 物理学 2011-11-10 A. Carati , S. L. Cacciatori , L. Galgani

This article deals with the problem of the motion of stars in galaxies. By using the Newton's theory combined with a gravitational time dilatation for the weak gravitational field, it is possible to give a solution without using the dark…

宇宙学与河外天体物理 · 物理学 2010-07-22 Emmanuel Moulay

Gravitational force manifested in its affect on rotational velocity is what indicates the presence of dark matter in individual galaxies. Newtonian mechanics is generally used to derive the relationship between rotational velocity and…

综合物理 · 物理学 2007-05-23 D. M. Snyder

We continue the study of the tensor-four-scalars theory which is a modification of general relativity. We include normal matter by applying the displace, cut, and reflect method to our previous vacuum solutions with dark halo. The resulting…

广义相对论与量子宇宙学 · 物理学 2012-05-22 Günter Scharf

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

The self-consistent spatial distribution of particles of Galactic dark matter is derived including their own gravitational potential, as also that of the visible matter of the Galaxy. In order to reproduce the observed rotation curve of the…

天体物理学 · 物理学 2009-10-28 R. Cowsik , Charu Ratnam , P. Bhattacharjee

For the past forty years the search for dark matter has been one of the primary foci of astrophysics, although there has yet to be any direct evidence for its existence (Porter et al. 2011). Indirect evidence for the existence of dark…

宇宙学与河外天体物理 · 物理学 2015-06-11 F. Elliott Koch , Angus H. Wright

In this paper we study a stellar dynamic model for the stars' rotational-dynamics, with a distribution of its own mass, rotating around its center with a higher density, like spiral galaxies happen, by means of a classical calculus of the…

天体物理学 · 物理学 2019-09-10 E. Lopez-Sandoval

We derive the first analytical formula for the density of "Dark Matter" (DM) at all length scales, thus also for the rotation curves of stars in galaxies, for the baryonic Tully-Fisher relation and for planetary systems, from Einstein's…

广义相对论与量子宇宙学 · 物理学 2025-03-14 Peter H. Handel , Klara E. Splett

There is strong evidence that the mass in the Universe is dominated by dark matter, which exerts gravitational attraction but whose exact nature is unknown. In particular, all galaxies are believed to be embedded in massive haloes of dark…

天体物理学 · 物理学 2008-11-26 A. Dekel , F. Stoehr , G. A. Mamon , T. J. Cox , G. S. Novak , J. R. Primack

The motion of massive test particles in dark matter is studied. It is shown that if the energy density of the dark matter making up a galactic halo has a large $r$ behavior of $1/r^2$, then contrary to intuition the motion of these test…

高能物理 - 唯象学 · 物理学 2008-02-03 Achilles D. Speliotopoulos

During the last century many observations have been made to peep into the dark matter in the universe and many astonishing behaviors of Galaxy clusters have been found which do not fit to any theories formulated before. However, Optical…

宇宙学与河外天体物理 · 物理学 2022-11-08 R. Debnath , A. Negi , S. AC , K. S. Kamath , S. Rauniyar

Dark matter is estimated to make up ~84% of all normal/baryonic matter, but cannot be directly imaged. Despite the fact that dark matter cannot be directly observed yet, its influence on the motion of stars and gas in spiral galaxies have…

The present work is devoted to study the dynamical evolution of the galaxies in scalar-GaussBonnet gravity in relationship with the MOND paradigm. This study is useful for giving meaning to the presence of a new gravitational constant. The…

广义相对论与量子宇宙学 · 物理学 2022-01-19 M. Bousder

The evidence of the phenomenon for which, in galaxies, the gravitating mass is distributed differently than the luminous mass, increases as new data become available. Furthermore, this discrepancy is well structured and it depends on the…

星系天体物理 · 物理学 2019-03-11 Paolo Salucci

We show that a new force, which appeared in a five-dimensional generalization of general relativity, implies precisely the flat circular velocity curves of luminous matter observed in the outer parts of spiral galaxies. A cosmological…

天体物理学 · 物理学 2007-05-23 R. L. Ingraham , L. A. Cummings

The paper is devoted to an explanation of the accelerated rate of expansion of the Universe. Usually the acceleration of the Universe, which is described by FRW metric, is due to dark energy. It is shown that this effect may be considered…

广义相对论与量子宇宙学 · 物理学 2013-03-14 S. C. Ulhoa

We show that in cosmology the gravitational action of the far away matter has quite relevant effects, if retardation of the forces and discreteness of matter (with its spatial correlation) are taken into account. The expansion rate is found…

宇宙学与河外天体物理 · 物理学 2009-08-03 A. Carati , S. L. Cacciatori , L. Galgani

Dark matter, believed to be present in many galaxies, is interpreted as a hydrodynamical system in interaction with the gravitational field and nothing else. An equation of state determines the mass distribution and the associated…

宇宙学与河外天体物理 · 物理学 2011-06-14 Christian Fronsdal , Thomas J. Wilcox
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