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相关论文: Large Numbers, Galactic Rotation and Orbits

200 篇论文

The local curvature of the space produced by the Sun causes not only the perihelion precession of Mercury's elliptical orbit, but also the variations of the whole orbit, in comparison with those predicted by the Newtonian theory of…

广义相对论与量子宇宙学 · 物理学 2019-07-17 Q. H. Liu , Q. Li , T. G. Liu , X . Wang

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

It is shown that F(R)-modified gravitational theories lead to curvature oscillations in astrophysical systems with rising energy density. The frequency and the amplitude of such oscillations could be very high and would lead to noticeable…

广义相对论与量子宇宙学 · 物理学 2015-06-12 E. V. Arbuzova , A. D. Dolgov , L. Reverberi

{Comparison of mass density profiles of galaxies of varying sizes based on some gravity theories from observed galaxy rotation curves and assessing the need for dark matter.} We present an analysis of the rotation curves of five galaxies of…

天体物理学 · 物理学 2011-08-23 Rahul Datta , Dilip G. Banhatti

A passing gravitational wave causes a deflection in the apparent astrometric positions of distant stars. The effect of the speed of the gravitational wave on this astrometric shift is discussed. A stochastic background of gravitational…

广义相对论与量子宇宙学 · 物理学 2020-01-29 Deyan P. Mihaylov , Christopher J. Moore , Jonathan Gair , Anthony Lasenby , Gerard Gilmore

We estimate the possible variations of the gravitational constant G in the framework of a generalized (Bergmann-Wagoner-Nordtvedt) scalar-tensor theory of gravity on the basis of the field equations, without using their special solutions.…

广义相对论与量子宇宙学 · 物理学 2007-05-23 K. A. Bronnikov , V. N. Melnikov , Mario Novello

In the paper we discussed the observational aspects of rotation in the Universe on different scales. We show dependence between the angular momentum of the structures and their size. The presented observational situation is that the…

宇宙学与河外天体物理 · 物理学 2015-05-27 Wlodzimierz Godlowski

We consider implications of the microscopic dynamics of spacetime for the evolution of cosmological models. We argue that quantum geometry effects may lead to stochastic fluctuations of the gravitational constant, which is thus considered…

广义相对论与量子宇宙学 · 物理学 2022-09-15 Marco de Cesare , Fedele Lizzi , Mairi Sakellariadou

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 energy inferred from the observed negative deceleration parameter introduces a small mass of the graviton, that satisfies the Higuchi stability condition. It implies an infra-red modification of gravitation that produces Milgrom's…

综合物理 · 物理学 2015-01-28 Maurice H. P. M. van Putten

Matter and dark matter in galaxies represent two main components linked by the gravitational interaction. Collisions of galaxies may create an offset between the centers of mass of these components. Ignoring internal dynamics of particles…

星系天体物理 · 物理学 2026-05-27 V. V. Flambaum , I. B. Samsonov

There is growing evidence that the majority of the energy density of the universe is not baryonic or dark matter, rather it resides in an exotic component with negative pressure. The nature of this `quintessence' influences our view of the…

天体物理学 · 物理学 2011-03-10 Geraint F. Lewis , Rodrigo A. Ibata

We present an analysis of a devised sample of Rotation Curves (RCs), aimed at checking the consequences of a modified f(R) gravity on galactic scales. Originally motivated by the the dark energy mystery, this theory may serve as a…

天体物理学 · 物理学 2008-11-26 Christiane Frigerio Martins , Paolo Salucci

This pedagogical review addresses several issues related to statistical description of gravitating systems in both static and expanding backgrounds, focusing on the latter. After briefly reviewing the results for the static background, I…

天体物理学 · 物理学 2007-05-23 T. Padmanabhan

A gauge-invariant, linear cosmological perturbation theory of an almost homogeneous and isotropic universe with dynamically evolving Newton constant G and cosmological constant $\Lambda$ is presented. The equations governing the evolution…

广义相对论与量子宇宙学 · 物理学 2011-04-22 Adriano Contillo

The late time acceleration of the Universe has challenged contemporary cosmology since its discovery. General Relativity explains this phenomenon by introducing the cosmological constant, named the standard cosmological model…

广义相对论与量子宇宙学 · 物理学 2024-01-02 Simran Arora

[Abridged] Star and planet formation are the complex outcomes of gravitational collapse and angular momentum transport mediated by protostellar and protoplanetary disks. In this review we focus on the role of gravitational instability in…

太阳与恒星天体物理 · 物理学 2016-10-05 Kaitlin M. Kratter , Giuseppe Lodato

In this paper we present the discussion on the salient points of the computational analysis that are at the basis of the paper \emph{Rotation Curves of Galaxies by Fourth Order Gravity} \citep{StSc}. In fact in this paper any galactic…

星系天体物理 · 物理学 2015-04-14 G. Scelza , A. Stabile

We consider a modification of General Relativity motivated by the treatment of anisotropies in Continuum Mechanics. The Newtonian limit of the theory is formulated and applied to galactic rotation curves. By assuming that the additional…

广义相对论与量子宇宙学 · 物理学 2018-06-25 Christian G. Boehmer , Nicola Tamanini , Matthew Wright

We investigate the cosmological behavior in a universe governed by time asymmetric extensions of general relativity, which is a novel modified gravity based on the addition of new, time-asymmetric, terms on the Hamiltonian framework, in a…

广义相对论与量子宇宙学 · 物理学 2015-11-11 Genly Leon , Emmanuel N. Saridakis