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The 2dF Galaxy Redshift Survey (2dFGRS) has produced a three-dimensional map of the distribution of 221,000 galaxies covering 5% of the sky and reaching out to a redshift z=0.3. This is first map of the large-scale structure in the local…

天体物理学 · 物理学 2007-05-23 Matthew Colless

Based on well known photometric rules for the number of galaxies as function of the distance in Mpc we model the so called "Great Wall" which is visible on the Cosmicflows-2 catalog. The gravitational field is evaluated at the light of the…

宇宙学与河外天体物理 · 物理学 2018-02-06 Lorenzo Zaninetti

Assuming that the universe is homogenous and isotropic and applying Gauss' flux theorem for gravity, it follows that the gravitational field of the visible universe can be calculated as if the entire mass of the visible universe is located…

综合物理 · 物理学 2015-03-17 Branislav Vlahovic

Global topological defects described by real scalar field in (3,1) dimensions coupled to gravity are analyzed. We consider a class of scalar potentials with explicit dependence with distance, evading Derrick's theorem and leading to defects…

广义相对论与量子宇宙学 · 物理学 2007-05-23 D. Bazeia , C. Furtado , A. R. Gomes

Tests of gravity at the galaxy scale are in their infancy. As a first step to systematically uncovering the gravitational significance of galaxies, we map three fundamental gravitational variables -- the Newtonian potential, acceleration…

星系天体物理 · 物理学 2020-10-26 Harry Desmond , Pedro G. Ferreira , Guilhem Lavaux , Jens Jasche

Laboratory experiments on gravitation are usually performed with objects of constant density, so that the analysis of the forces concerns only the geometry of their shape. In an ideal experiment, the shapes of the constituent parts will be…

广义相对论与量子宇宙学 · 物理学 2007-05-23 John W. Barrett

The information contained in galactic rotation curves is examined under a minimal set of assumptions. If emission occurs from stable circular geodesic orbits of a static spherically symmetric field, with information propagated to us along…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Kayll Lake

The dynamical system constituted by two spherically symmetric thin shells and their own gravitational field is studied. The shells can be distinguished from each other, and they can intersect. At each intersection, they exchange energy on…

广义相对论与量子宇宙学 · 物理学 2009-11-07 P. Hajicek , I. Kouletsis

The measured rotation velocity profiles of mature spiral galaxies are successfully described with a gravitational model consisting of a thin axisymmetric disk of finte radius. The disk is assumed uniformly thin but with variable radial mass…

天体物理学 · 物理学 2008-03-06 James Q. Feng , C. F. Gallo

We report the results of a statistical analysis of the space distribution of galaxies within distances about 300 Mpc using the 2MRS catalog, which contains redshifts of 43533 galaxies of the 2MASS all-sky IR survey. Because of the unique…

宇宙学与河外天体物理 · 物理学 2016-10-26 Daniil Tekhanovich , Yurij V. Baryshev

The astronomical observations indicate that the universe expands with acceleration and it has a finite event horizon. The recent CMB observations confirm the universe is homogeneous, isotropic and asymptotically flat. The total…

综合物理 · 物理学 2014-11-18 Dimitar Valev

We consider the gravitational potential and the gravitational rotation field generated by an spherical mass distribution with exponential density, when the force between any two mass elements is not the usual Newtonian one, but some general…

天体物理学 · 物理学 2007-05-23 Carlos Rodrigo-Blanco

The 2dF Galaxy Redshift Survey (2dFGRS) of 230,000 redshifts of nearby (z~0.1) galaxies is now complete. It has allowed the 2dFGRS team and others to estimate fundamental cosmological parameters and to study galaxy intrinsic properties.…

天体物理学 · 物理学 2009-11-10 Ofer Lahav

In the weak field approximation, the nonsymmetric gravitational theory has, in addition to the Newtonian gravitational potential, a Yukawa potential produced by the exchange of a spin $1^+$ boson between fermions. If the range $r_0$ is of…

天体物理学 · 物理学 2015-06-24 J. W. Moffat

An expression for rotational velocity of a test particle around the central mass in the invariant plane is derived. For this, a line element of Schwarzschild de-Sitter space-time is used to study the effect of cosmological constant…

宇宙学与河外天体物理 · 物理学 2013-07-09 B. Aryal , R. Pandey , N. Baral , U. Khanal , W. Saurer

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

We explore the mass distribution of material associated with galaxies from the observation of gravitational weak lensing for the galaxy mass correlation function with the aid of $N$-body simulations of dark matter. The latter is employed to…

宇宙学与河外天体物理 · 物理学 2015-05-28 Shogo Masaki , Masataka Fukugita , Naoki Yoshida

According to Mach's principle inertia has its reason in the presence of all masses in the universe. Despite there is a lot of sympathy for this plausible idea, only a few quantitative frameworks have been proposed to test it. In this paper…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Alexander Unzicker

In this paper, the behavior of a spherical hole in an otherwise infinite and uniform universe is investigated. First, the Newtonian theory is developed. The concept of negative gravity, an outward gravitational force acting away from the…

广义相对论与量子宇宙学 · 物理学 2009-09-25 Gilbert N. Lewis

A galaxy group catalog is built from the sample of the 2MASS Redshift Survey almost complete to Ks=11.75 over 91% of the sky. Constraints in the construction of the groups were provided by scaling relations determined by close examination…

宇宙学与河外天体物理 · 物理学 2015-06-24 R. Brent Tully
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