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相关论文: Large Numbers, Galactic Rotation and Orbits

200 篇论文

We consider two cosmologies which give an inverse time dependance for the gravitational constant G, and show that we can recover the correct value of the perhelion precession and anomalous inward radial accelerations, amongst other things.

天体物理学 · 物理学 2007-05-23 B. G. Sidharth

The correct perihelion precession was recently deduced within the frame work of a time varying Gravitational constant G. Here, we deduce also the observed gravitational bending of light and flattening of galactic rotational curves.

综合物理 · 物理学 2007-05-23 B. G. Sidharth

On the basis of a recent cosmological model, the puzzle of galactic rotational velocities at their edges is explained without invoking dark matter. A rationale for the existence of structures like galaxies and superclusters is also…

天体物理学 · 物理学 2007-05-23 B. G. Sidharth

It was recently shown that in cosmology the gravitational action of faraway matter has quite relevant effects, if retardation of the forces and discreteness of matter (with its spatial correlation) are taken into account. Indeed, far matter…

宇宙学与河外天体物理 · 物理学 2011-11-28 A. Carati

The amount of dark matter in the Milky Way and beyond is examined by taking into account the possible running of the gravitational constant $G$ as a function of distance scale. If the running of $G$, as suggested by the Asymptotically-Free…

天体物理学 · 物理学 2010-11-30 A. Bottino , C. W. Kim , J. Song

The gravitational action of the smooth energy-matter components filling in the universe can affect the orbit of a planetary system. Changes are related to the acceleration of the cosmological scale size R. In a universe with significant…

天体物理学 · 物理学 2008-11-26 M. Sereno , Ph. Jetzer

This paper describes how the non-gravitational contribution to Galactic Velocity Rotation Curves can be explained in terms of a negative Cosmological Constant ($\Lambda$). It will be shown that the Cosmological Constant leads to a velocity…

天体物理学 · 物理学 2007-05-23 S. B. Whitehouse , G. V. Kraniotis

This paper discusses the observed at rotation curves of galaxies in the context of noncommutative geometry. The energy density of such a geometry is diffused throughout a region due to the uncertainty encoded in the coordinate commutator.…

广义相对论与量子宇宙学 · 物理学 2016-11-25 F. Rahaman , Peter K. F. Kuhfittig , K. Chakraborty , A. A. Usmani , Saibal Ray

In this paper it is shown that dynamics based on a variation of the gravitational constant $G$ with time solves several puzzling and anomalous features observed, for example the rotation curves of galaxies (attributed to as yet undetected…

综合物理 · 物理学 2009-12-28 B G Sidharth , B S Lakshmi

Galaxies are huge physical systems having dimensions of many tens of thousands of light years. Thus any change at the galactic center will be noticed at the rim only tens of thousands of years later. Those retardation effects seems to be…

综合物理 · 物理学 2025-05-27 Asher Yahalom

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

This paper investigates the influence of nonlinear dissipative forces, specifically Gravitational Friction (GF), on the precession of celestial bodies within the framework of general relativity. We derive a modified line element by…

广义相对论与量子宇宙学 · 物理学 2024-12-02 Raju S. Khatiwada , C. Ortiz , Basanta R. Giri

Conformal gravity theory can explain observed flat rotation curves of galaxies without invoking hypothetical dark matter. Within this theory, we obtain a generic formula for the sizes of galaxies exploiting the stability criterion of…

广义相对论与量子宇宙学 · 物理学 2012-08-28 Kamal K. Nandi , Arunava Bhadra

In the paper are studied the deformations of the planetary orbits caused by the time dependent gravitational potential in the universe. It is shown that the orbits are not axially symmetric and the time dependent potential does not cause…

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

Einstein gravity coupled to a massive skew symmetric field F_{\mu\nu\lambda} leads to an acceleration law that modifies the Newtonian law of attraction between particles. We use a framework of non-perturbative renormalization group…

天体物理学 · 物理学 2009-11-10 J. W. Moffat

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

It has been suggested that antiscreening effects due to the running of the gravitational constant G might provide a partial solution to the dark matter mystery. It has also been hypothesized that renormalization group scaling…

广义相对论与量子宇宙学 · 物理学 2015-08-31 Tom T. S. Chang

A modified gravitational theory explains early universe and late time cosmology, galaxy and galaxy cluster dynamics. The modified gravity (MOG) theory extends general relativity (GR) by three extra degrees of freedom: a scalar field $G$,…

广义相对论与量子宇宙学 · 物理学 2020-10-30 J. W. Moffat

Cosmologies with running cosmological term (Lambda) and gravitational Newton's coupling (G) may naturally be expected if the evolution of the universe can ultimately be derived from the first principles of Quantum Field Theory or String…

宇宙学与河外天体物理 · 物理学 2015-05-14 Javier Grande , Joan Sola , Julio C. Fabris , Ilya L. Shapiro

Galaxies are gigantic physical systems having a typical size of many tens of thousands of light years. Thus any change at the center of the galaxy will affect the rim only tens of millennia later. Those retardation effects seems to be…

综合物理 · 物理学 2021-08-21 Asher Yahalom
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