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相关论文: Comment about the Letter entitled ``Scalar fields …

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In this manuscript the authors present a detailed answer to the comment in order to avoid misunderstandings in the future.

广义相对论与量子宇宙学 · 物理学 2007-05-23 F. S. Guzman , T. Matos

In this work we study rotation curves of spiral galaxies using a model of dark matter based on a scalar-tensor theory of gravity. We show how to estimate the scalar field dark matter parameters using a sample of observed rotation curves.

星系天体物理 · 物理学 2012-10-26 Mario A. Rodriguez-Meza

We discuss scenarios in which the galactic dark matter in spiral galaxies is described by a long range coherent field which settles in a stationary configuration that might account for the features of the galactic rotation curves. The…

广义相对论与量子宇宙学 · 物理学 2010-11-19 Ulises Nucamendi , Marcelo Salgado , Daniel Sudarsky

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…

天体物理学 · 物理学 2008-11-26 P. Salucci , G. Gentile

An exact, axially symmetric solution to the Einstein-Klein-Gordon field equations is employed to model the dark matter in spiral galaxies. The extended rotation curves from a previous analysis are used to fit the model and a very good…

天体物理学 · 物理学 2007-05-23 F. S. Guzman , T. Matos , H. Villegas-Brena

We review the topic of rotation curves of spiral galaxies emphasizing the standard interpretation as evidence for the existence of dark matter halos. Galaxies other than spirals and late-type dwarfs may also possess great amounts of dark…

天体物理学 · 物理学 2007-05-23 Eduardo Battaner , Estrella Florido

We present a model for the dark matter in spiral galaxies, which is a result of a static and axial symmetric exact solution of the Einstein-Dilaton theory. We suposse that dark matter is a scalar field endowed with a scalar potential. We…

广义相对论与量子宇宙学 · 物理学 2010-04-06 F. Siddhartha Guzman , Tonatiuh Matos

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

As a candidate for dark matter in galaxies, we study an SU(3) triplet of complex scalar fields which are non-minimally coupled to gravity. In the spherically symmetric static spacetime where the flat rotational velocity curves of stars in…

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

Based on dynamical constraints about the Hubble sequence evolution, observational data and a number of "conspiracies", we propose that the dark matter around spiral galaxies is in the form of cold gas, essentially in molecular form and…

天体物理学 · 物理学 2011-05-23 D. Pfenniger , F. Combes , L. Martinet

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

We suggest a new explanation of flatness of galaxies rotation curves without invoking dark matter. For this purpose a new gravitational tensor field is introduced in addition to the metric tensor.

高能物理 - 唯象学 · 物理学 2023-12-25 S. A. Larin

Beginning with a geometric motivation for dark matter going back to the axioms of general relativity, we show how scalar field dark matter, which naturally forms dark matter density waves due to its wave nature, may cause the observed…

综合物理 · 物理学 2012-12-27 Hubert L. Bray

The dark matter hypothesis, which is not called into question here, explains why typical rotation curves of spiral galaxies do not follow a Keplerian profile. It is however not sufficient in itself to explain why the whole matter…

星系天体物理 · 物理学 2019-06-13 Vincent Deledicque

In this note we comment on a recent attempt by P. Burikham, T. Harko, K. Pimsamarn and S. Shahidi [Phys. Rev. D {\bf 107}, 064008 (2023)] to explain the galactic rotation curves as the result of the motion of time-like test particles in the…

广义相对论与量子宇宙学 · 物理学 2023-08-16 Israel Quiros

We present decompositions of the rotation curves of distant spiral galaxies into contributions due to their bulges, disks, and putative dark haloes. In order to set constraints on the ambiguities of the decompositions we interpret the…

天体物理学 · 物理学 2007-05-23 B. Fuchs , C. Moellenhoff , J. Heidt

We study a spherically symmetric fluctuation of scalar dark matter in the cosmos and show that it could be the dark matter in galaxies, provided that the scalar field has an exponential potential whose overall sign is negative and whose…

天体物理学 · 物理学 2008-11-26 T. Matos , F. S. Guzman , D. Nunez

We investigate the possibility to explain theoretically the galaxy rotation curves by a gravitational potential in total absence of dark matter. To this aim an analytic fourth-order theory of gravity, nonminimally coupled with a massive…

广义相对论与量子宇宙学 · 物理学 2015-06-15 A. Stabile , S. Capozziello

There should be two ways to describe the flat rotation curves of galaxies and cluster of galaxies. Either one can introduce a dark matter component for the matter filling the halo, or by modifying the gravity theory and give the flat…

广义相对论与量子宇宙学 · 物理学 2014-04-02 F. Shojai , A. Shojai

Recent observations have revealed the structural properties of the dark and luminous mass distribution in spirals. These results led to the vision of a new and amazing scenario. The investigation of single and coadded objects has shown that…

星系天体物理 · 物理学 2015-04-13 Paolo Salucci , Mariafelicia De Laurentis
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