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Logarithmic superfluid theory of physical vacuum suggests that gravity has a multiple-scale structure; where one can recognize sub-Newtonian, Newtonian, logarithmic, linear and quadratic (de Sitter) terms in the induced spacetime metric and…

综合物理 · 物理学 2023-10-12 Konstantin G. Zloshchastiev

We study the possibility that galactic rotation curves can be explained by a gravitational potential that contains a linear term as well as a Newtonian one. This hypothesis, suggested by conformal gravity, does allow good fits to the…

天体物理学 · 物理学 2007-05-23 Carl E. Carlson , Eric J. Lowenstein

Taking the flat rotation curve as input and treating the matter content in the galactic halo region as perfect fluid, we obtain space time metric at the galactic halo region in the framework of general relativity. We find that the resultant…

广义相对论与量子宇宙学 · 物理学 2010-11-26 F. Rahaman , K. K. Nandi , A. Bhadra , M. Kalam , K. Chakraborty

The logarithmic superfluid theory of physical vacuum predicts that gravity is an induced phenomenon, which has a multiple-scale structure. At astronomical scales, as the distance from a gravitating center increases, gravitational potential…

广义相对论与量子宇宙学 · 物理学 2022-01-13 Konstantin G. Zloshchastiev

The missing of a Keplerian fall-off in the observed galaxy rotation curves represents classical evidence for the existence of dark matter on galactic scales. There has been some recent activity concerning the potential of modelling galactic…

广义相对论与量子宇宙学 · 物理学 2010-02-17 Aleksandar Rakic , Dominik J. Schwarz

The anomalous rotation curves of galaxies provide compelling evidence for dark matter, yet its fundamental nature and distribution remain key unresolved issues in astrophysics. In this work, we investigate a dark matter model derived from…

广义相对论与量子宇宙学 · 物理学 2025-09-17 Jan Kuncewicz

We prove the existence of general relativistic perfect fluid black hole solutions, and demonstrate the phenomenon for the $P=w\rho$ class of equations of state. While admitting a local time-like Killing vector on the event horizon itself,…

广义相对论与量子宇宙学 · 物理学 2012-11-28 Aharon Davidson , Shimon Rubin , Yosef Verbin

Recently, in a series of papers, we established the existence and found a general solution for the simultaneously rotating and twisting locally rotationally symmetric spacetimes in general relativity, which can model inhomogeneous and…

广义相对论与量子宇宙学 · 物理学 2017-09-25 Sayuri Singh , Amare Abebe , Rituparno Goswami , Sunil D. Maharaj

We review some recent work by Mannheim and O'Brien on the systematics of galactic rotation curves in the conformal gravity theory. In this work the conformal theory was applied to a comprehensive, high quality sample of spiral galaxies…

宇宙学与河外天体物理 · 物理学 2015-06-12 Philip D. Mannheim , James G. O'Brien

Ho\v{r}ava--Lifshitz gravity has covariance only under the foliation-preserving diffeomorphism. This implies that the quantities on the constant-time hypersurfaces should be regular. In the original theory, the projectability condition,…

广义相对论与量子宇宙学 · 物理学 2013-12-18 Naoki Tsukamoto , Tomohiro Harada

It has recently been suggested that observed galaxy rotation curves can be accounted for by general relativity without recourse to dark-matter halos. Good fits have been produced to observed galatic rotation curves using this model. We show…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Dylan Menzies , Grant J. Mathews

The paths of stars in galaxies have circular velocity independent of their distance from the centre of the galaxy. Newtonian mechanics with a logarithmic potential has such paths. In relativity these paths can be taken to be geodesics and…

天体物理学 · 物理学 2011-04-04 Mark D. Roberts

In a previous paper we presented a typical set of galactic rotation curves associated with the linear gravitational potential of the conformal invariant fourth order theory of gravity which has recently been advanced by Mannheim and Kazanas…

天体物理学 · 物理学 2009-09-25 PHILIP D. MANNHEIM

We have found exact constant solutions for the cosmological density parameter using a generalization of general relativity that incorporates a cosmic time-variation of the velocity of light in vacuum and the Newtonian gravitation constant.…

天体物理学 · 物理学 2009-10-31 Luis P. Chimento , Alejandro S. Jakubi

We present new numerical algorithms for the coupled Einstein-perfect fluid system in axisymmetry. Our framework uses a foliation based on a family of light cones, emanating from a regular center, and terminating at future null infinity.…

广义相对论与量子宇宙学 · 物理学 2009-11-07 Florian Siebel , Jose A. Font , Ewald Mueller , Philippos Papadopoulos

A solution for the problem of understanding observed rotation curves in galaxies without the introduction of dark matter halos is presented. This solution has been obtained upon considering the distribution of masses in the expanding…

广义相对论与量子宇宙学 · 物理学 2009-09-25 J. L. Rosales

In the present article we find a new class of solutions of Einstein's field equations. It describes stationary, cylindrically symmetric spacetimes with closed timelike geodesics everywhere outside the symmetry axis. These spacetimes contain…

广义相对论与量子宇宙学 · 物理学 2010-04-20 Oyvind Gron , Steinar Johannesen

Spacetime foam manifests itself in a variety of ways. It has some attributes of a turbulent fluid. It is the source of the holographic principle. Cosmologically it may play a role in explaining why the energy density has the critical value,…

广义相对论与量子宇宙学 · 物理学 2011-02-24 Y. Jack Ng

The relativistic treatment of galaxies modelled as a rotating disk surrounded by a magnetised material halo is considered. The galactic halo is modelled by a magnetised mass-energy distribution described by the energy-momentum tensor of a…

广义相对论与量子宇宙学 · 物理学 2014-12-19 Antonio C. Gutiérrez-Piñeres , Abraão Capistrano

While many observations support the validity of Einstein's general relativity as the theory of gravity, there are yet many that suggest the presence of new physics. In order to explain the high-redshift supernovae Ia observations together…

天体物理学 · 物理学 2008-11-26 R. G. Vishwakarma
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