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In this work the phenomenology of models possessing a non-minimal coupling between matter and geometry is discussed, with a particular focus on the possibility of describing the flattening of the galactic rotation curves as a dynamically…

星系天体物理 · 物理学 2015-05-18 Orfeu Bertolami , Jorge Páramos

The existence of the flat rotation curves of galaxies is still perplexing. The dark matter paradigm was proposed long ago to solve this conundrum; however, this proposal is still under debate. In this paper, we search for universal…

星系天体物理 · 物理学 2022-10-25 G. Pascoli

Noether symmetry of F(R) theory of gravity in vacuum or in matter dominated era yields three-half power law of R. We show that this particular curvature invariant term is very special in the context of isotropic and homogeneous cosmological…

宇宙学与河外天体物理 · 物理学 2013-02-18 Kaushik Sarkar , Nayem Sk. , Soumendranath Ruz , Subhra Debnath , Abhik Kumar Sanyal

We discuss the f(R) gravity model in which the origin of dark energy is identified as a modification of gravity. The Noether symmetry with gauge term is investigated for the f(R) cosmological model. By utilization of the Noether Gauge…

综合物理 · 物理学 2012-01-16 Ibrar Hussain , Mubasher Jamil , F. M. Mahomed

The simplest gauge gravitation theory in Riemann-Cartan space-time leading to the solution of the problem of cosmological singularity and dark energy problem is investigated with purpose to solve the dark matter problem. It is shown that…

广义相对论与量子宇宙学 · 物理学 2017-05-09 A. V. Minkevich

We study spherically symmetric solutions in a covariant massive gravity model, which is a candidate for a ghost-free non-linear completion of the Fierz-Pauli theory. There is a branch of solutions that exhibits the Vainshtein mechanism,…

高能物理 - 理论 · 物理学 2011-11-04 Kazuya Koyama , Gustavo Niz , Gianmassimo Tasinato

In bigravity, when taking into account the potential existence of matter fields minimally coupled to the second gravitation sector, the dynamics of our Universe depends on some matter that cannot be observed in a direct way. In this paper,…

广义相对论与量子宇宙学 · 物理学 2018-03-02 Mariam Bouhmadi-López , Salvatore Capozziello , Prado Martín-Moruno

A very general class of axially-symmetric metrics in general relativity (GR) that includes rotations is used to discuss the dynamics of rotationally-supported galaxies. The exact vacuum solutions of the Einstein equations for this extended…

广义相对论与量子宇宙学 · 物理学 2023-02-15 Yogendra Srivastava , Giorgio Immirzi , John Swain , Orland Panella , Simone Pacetti

Flat or almost flat rotation curves of spiral galaxies can be explained by logarithmic gravitational potentials. The field equations of GR admit of spacetime metrics with such behaviors. The scenario can be interpreted either as an…

广义相对论与量子宇宙学 · 物理学 2009-03-26 Yousef Sobouti

We use Noether symmetry approach to find spherically symmetric static solutions of the non-minimally coupled electromagnetic fields to gravity. We construct the point-like Lagrangian under the spherical symmetry assumption. Then we…

广义相对论与量子宇宙学 · 物理学 2020-07-28 Özcan Sert , Fatma Çeliktaş

An attempt has been made to explore the galactic dynamics via the rotational velocity beyond the Einstein's geometric theory of gravity. It is inspired from the geometric relation obtained in the power law $f(R)$ gravity model in vacuum. We…

广义相对论与量子宇宙学 · 物理学 2020-07-20 Vipin Kumar Sharma , Bal Krishna Yadav , Murli Manohar Verma

The solutions for the field equations of $f(R)$ gravity are investigated in static cylindrically symmetric space-time. Conserved quantities of the system, as well as unknown functions, can be determined with the help of the Noether symmetry…

广义相对论与量子宇宙学 · 物理学 2021-09-21 Işıl Başaran Öz , Kazuharu Bamba

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

A solution to Einstein's field equations via the Friedman equations is shown to produce a cosmological model that is in exact agreement with the measurements made by the dark energy astronomers. All the essential physical parameters are…

综合物理 · 物理学 2012-06-26 James G. Gilson

Allowing the energy of a gravitational field to serve partially as its own source allows gravitating bodies to exhibit stronger fields, as if they were more massive. Depending on degree of compaction of the body, the field could be one to…

天体物理学 · 物理学 2013-01-29 Yousef Sobouti

The discrepancy between the visible mass in galaxies or galaxy clusters, and that inferred from their dynamics is well known. The prevailing solution to this problem is dark matter. Here we show that a different approach, one that conforms…

星系天体物理 · 物理学 2020-06-24 Alexandre Deur , Corey Sargent , Balša Terzić

Modifications to Newtonian dynamics at low accelerations have long been proposed as an alternative to dark matter to explain galaxy rotation curves. More recently, similar corrections have been invoked to interpret anomalies in…

星系天体物理 · 物理学 2026-03-19 Riccardo Scarpa , Renato Falomo , Aldo Treves

Several rare coincidences of scales in standard particle physics are needed to explain (i) why neutrinos have mass, (ii) why the negative pressure of the cosmological dark energy (DE) coincides with the positive pressure of random motion of…

广义相对论与量子宇宙学 · 物理学 2008-06-11 HongSheng Zhao

The nonsymmetric gravitational theory predicts an acceleration law that modifies the Newtonian law of attraction between particles. For weak fields a fit to the flat rotation curves of galaxies is obtained in terms of the mass…

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

We search for spherically symmetric solutions of f(R) theories of gravity via the Noether Symmetry Approach. A general formalism in the metric framework is developed considering a point-like f(R)-Lagrangian where spherical symmetry is…

广义相对论与量子宇宙学 · 物理学 2008-11-26 S. Capozziello , A. Stabile , A. Troisi