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Related papers: Chameleon Gravity as an Alternative to Dark Matter

200 papers

If dark energy --- which drives the accelerated expansion of the universe --- consists of a light scalar field, it might be detectable as a "fifth force" between normal-matter objects, in potential conflict with precision tests of gravity.…

Atomic Physics · Physics 2015-08-24 Paul Hamilton , Matt Jaffe , Philipp Haslinger , Quinn Simmons , Holger Müller , Justin Khoury

The recent paper by Lee and Lee (2004) may strongly leave the impression that astronomers have established that the rotation curves of spiral galaxies are flat. We show that the old paradigm of Flat Rotation Curves lacks, today, any…

Astrophysics · Physics 2008-11-26 P. Salucci , G. Gentile

One possibility to explain the current accelerated expansion of the universe may be related with the presence of cosmologically evolving scalar whose mass depends on the local matter density (chameleon cosmology). We point out that matter…

High Energy Physics - Theory · Physics 2009-09-17 Shin'ichi Nojiri , Sergei D. Odintsov

We have investigated a brane world model in which the gravitational field in the bulk is described both by a metric tensor and a minimally coupled scalar field. This scalar field is taken to be a chameleon with an appropriate potential…

General Relativity and Quantum Cosmology · Physics 2017-12-12 Y. Bisabr , F. Ahmadi

Chameleon, environmentally dependent dilaton, and symmetron gravity are three models of modified gravity in which the effects of the additional scalar degree of freedom are screened in dense environments. They have been extensively studied…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-18 Anne-Christine Davis , Ruth Gregory , Rahul Jha , Jessica Muir

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…

General Relativity and Quantum Cosmology · Physics 2020-07-20 Vipin Kumar Sharma , Bal Krishna Yadav , Murli Manohar Verma

We investigate the case of a homogeneous tachyon field coupled to gravity in a spatially flat Friedman-Robertson-Walker spacetime. Assuming the field evolution to be exponentially decaying with time we solve the field equations and show…

Astrophysics · Physics 2009-11-11 A. Das , Shashikant Gupta , Tarun Deep Saini , Sayan Kar

We investigate whether a dark matter with substantial amounts of pressure, comparable in magnitude to the energy density, could be a viable candidate for the constituent of dark matter halos. We find that galaxy halos models, consistent…

Astrophysics · Physics 2009-11-07 Somnath Bharadwaj , Sayan Kar

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…

Cosmology and Nongalactic Astrophysics · Physics 2011-11-28 A. Carati

In this paper, we attempt to resolve the dark matter problem in f(T) gravity. Specifically, from our model we successfully obtain the flat rotation curves of galaxies containing dark matter. Further, we obtain the density profile of dark…

General Relativity and Quantum Cosmology · Physics 2012-09-29 Mubasher Jamil , D. Momeni , Ratbay Myrzakulov

A scalar field is a favorite candidate for the particle responsible for dark energy. However, few theoretical means exist that can simultaneously explain the observed acceleration of the Universe and evade tests of gravity. The chameleon…

High Energy Physics - Experiment · Physics 2019-08-15 Jason H. Steffen

[abridged] We explore the possibility that the dark matter (DM) component in galaxies may originate fractional gravity. In such a framework, the standard law of inertia continues to hold, but the gravitational potential associated to a…

Astrophysics of Galaxies · Physics 2023-06-07 Francesco Benetti , Andrea Lapi , Giovanni Gandolfi , Paolo Salucci , Luigi Danese

The missing gravity in galaxies requires dark matter, or alternatively a modification of gravity or inertia. These theoretical possibilities of fundamental importance may be distinguished by the statistical relation between the observed…

Astrophysics of Galaxies · Physics 2022-12-21 Kyu-Hyun Chae

We investigate the possibility that the galactic dark matter exists in an scenario where the phantom field is responsible for the dark energy. We obtain the statically and spherically approximate solution for this kind of the galaxy system…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-20 Ming-Hsun Li , Kwei-Chou Yang

We examine the amplitude of the rotation velocity that can be attributed to the dark matter halos of disk galaxies, focusing on well measured intermediate radii. The data for 60 galaxies spanning a large range of mass and Hubble types,…

Astrophysics · Physics 2010-11-05 S. S. McGaugh , W. J. G. de Blok , J. M. Schombert , R. Kuzio de Naray , J. H. Kim

A dark matter halo model is developed postulating a new state of matter, entities which have internal spin-like terms. Their motion in an external Schwarzschild metric is discussed. The internal spin motion contributes to the centrifugal…

General Physics · Physics 2017-05-25 H. L. Helfer

It is shown that the cosmological constant links the roots both of General Relativity and Newtonian gravity via the general function satisfying Newton's theorem according to which the gravitating sphere acts as a point mass situated in its…

General Relativity and Quantum Cosmology · Physics 2019-01-10 V. G. Gurzadyan

We consider static spherically symmetric solutions of a general scalar field theory with non-standard kinetic energy coupled to gravity with a view to explain dark matter halos as a coherent state of the scalar field. Consistent solutions…

High Energy Physics - Theory · Physics 2008-06-04 Ratindranath Akhoury , Christopher S. Gauthier

The cold dark matter halo mass function is much steeper than the galaxy stellar mass function on galactic and subgalactic scales. This difference is usually reconciled by assuming that the galaxy formation efficiency drops sharply with…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 Ismael Ferrero , Mario G. Abadi , Julio F. Navarro , Laura V. Sales , Sebastian Gurovich

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…

General Relativity and Quantum Cosmology · Physics 2009-03-26 Yousef Sobouti
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