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It is still a challenging problem to the theoretical physicists to know the exact nature of the galactic dark matter which causes the galactic rotational velocity to be more or less a constant. We have proposed that the dark matter as an…

广义相对论与量子宇宙学 · 物理学 2015-06-05 Farook Rahaman , Ritabrata Biswas , Hafiza Ismat Fatima , Nasarul Islam

We consider the application of quantum corrections computed using renormalization group arguments in the astrophysical domain and show that, for the most natural interpretation of the renormalization group scale parameter, a gravitational…

宇宙学与河外天体物理 · 物理学 2014-11-20 Davi C. Rodrigues , Patricio S. Letelier , Ilya L. Shapiro

Multi-fractional theories with integer-order derivatives are models of gravitational and matter fields living in spacetimes with variable Hausdorff and spectral dimension, originally proposed as descriptions of geometries arising in quantum…

广义相对论与量子宇宙学 · 物理学 2022-08-09 Gianluca Calcagni , Gabriele U. Varieschi

We analyse the evolution of the rotational type cosmological perturbation in a gravity with general quadratic order gravitational coupling terms. The result is expressed independently of the generalized nature of the gravity theory, and is…

广义相对论与量子宇宙学 · 物理学 2010-11-19 J. Hwang , H. Noh

When dealing with galactic dynamics, or more specifically, with galactic rotation curves, one basic assumption is always taken: the frame of reference relative to which the rotational velocities are given is assumed to be inertial. In other…

星系天体物理 · 物理学 2021-05-25 Roy Gomel , Tomer Zimmerman

The existence of "dark matter", inferred from the observed rotation curves of galaxies, is a hypothesis which is widely regarded as problematic. This paper proposes an alternative hypothesis based on the space-time geometry near a rotating…

综合物理 · 物理学 2020-02-27 Colin Rourke

In a recent paper, we have a shown that the flattening of galactic rotation curves can be explained by retardation. However, this will rely on a temporal change of galactic mass. In our previous work, we kept only second order terms of the…

综合物理 · 物理学 2021-08-19 Asher Yahalom

Generally, the dynamics of test particles around galaxies, as well as the corresponding mass deficit, is explained by postulating the existence of a hypothetical dark matter. In fact, the behavior of the rotation curves shows the existence…

广义相对论与量子宇宙学 · 物理学 2013-11-13 Salvatore Capozziello , Tiberiu Harko , Tomi S. Koivisto , Francisco S. N. Lobo , Gonzalo J. Olmo

Higher order curvature gravity has recently received a lot of attention due to the fact that it gives rise to cosmological models which seem capable of solving dark energy and quintessence issues without using "ad hoc" scalar fields. Such…

天体物理学 · 物理学 2014-10-13 S. Capozziello , V. F. Cardone , S. Carloni , A. Troisi

The postulate of universal Weyl conformal symmetry for all elementary physical fields introduces nonclassical gravitational effects in both conformal gravitation(CG) and the conformal Higgs model (CHM). The resulting theory is found to…

广义相对论与量子宇宙学 · 物理学 2023-12-27 R. K. Nesbet

We consider the consequences of applying general relativity to the description of the dynamics of a galaxy, given the observed flattened rotation curves. The galaxy is modeled as a stationary axially symmetric pressure-free fluid. In spite…

天体物理学 · 物理学 2010-10-27 F. I. Cooperstock , S. Tieu

Rotation curves of spiral galaxies are known with reasonable precision for a large number of galaxies with similar morphologies. The data implies that non-Keplerian fall--off is seen. This implies that (i) large amounts of dark matter must…

天体物理学 · 物理学 2011-05-23 C. Rodrigo-Blanco , J. Pérez-Mercader

The geometrical nature of gravity emerges from the universality dictated by the equivalence principle. In the usual formulation of General Relativity, the geometrisation of the gravitational interaction is performed in terms of the…

高能物理 - 理论 · 物理学 2019-03-19 Jose Beltran Jimenez , Lavinia Heisenberg , Tomi S. Koivisto

The Quadratic Gravitational Lagrangian with torsion provides us with a richer number of solutions than the Einstein-Hilbert Lagrangian does. With proper interpretation, these solutions, together, seem to give good explanations of the form…

综合物理 · 物理学 2012-05-14 Yi Yang , Wai Bong Yeung

A Born-Infeld theory has been proposed in order to explain both dark matter and dark energy. We show that the approximation used to deduce the flat rotation curves in this model breaks down at large distances in a spherically symmetric…

高能物理 - 理论 · 物理学 2008-04-15 Musongela Lubo

We present a simple, closed form expression for the potential of an axisymmetric disk of stars interacting through gravitational potentials of the form $V(r)=-\beta /r+\gamma r/2$, the potential associated with fundamental sources in the…

天体物理学 · 物理学 2007-05-23 Philip D. Mannheim

Astronomical data have shown that the galaxy rotation curves are mostly flat in the far distance of the galactic cores, which reveals the insufficiency of our knowledges about how gravity works in these regimes. In this paper we introduce a…

广义相对论与量子宇宙学 · 物理学 2023-05-31 H. Shabani , P. H. R. S. Moraes

We derive a simple, closed form expression for the potential of a thin exponential disk of stars interacting through gravitational potentials of the form $V(r)=-\beta /r+\gamma r/2$, the potential associated with fundamental sources in the…

高能物理 - 唯象学 · 物理学 2009-10-22 Philip D. Mannheim

Conformal Weyl Gravity (CWG) predicts galactic rotation curves without invoking dark matter. This makes CWG an interesting candidate theory as an alternative to GR. This removal of the necessity of dark matter arises because the exact…

广义相对论与量子宇宙学 · 物理学 2014-04-01 Deandra Cutajar , Kristian Zarb Adami

Gravitation is described in the context of a dilatonic theory that is conformally related to general relativity. All dimensionless ratios of fundamental dimensional quantities, e.g. particle masses and the Planck mass, as well as the…

宇宙学与河外天体物理 · 物理学 2017-04-21 Meir Shimon