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相关论文: Is flat rotation curve a sign of cosmic expansion?

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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

A solution for the problem of understanding observed rotation curves in galaxies without the introduction of dark matter halos is presented. This solution has been obtained upon considering the distribution of masses in the expanding…

广义相对论与量子宇宙学 · 物理学 2009-09-25 J. L. Rosales

We study the possibility that galactic rotation curves can be explained by a gravitational potential that contains a linear term as well as a Newtonian one. This hypothesis, suggested by conformal gravity, does allow good fits to the…

天体物理学 · 物理学 2007-05-23 Carl E. Carlson , Eric J. Lowenstein

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

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

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. In…

广义相对论与量子宇宙学 · 物理学 2009-11-10 S. Capozziello , V. F. Cardone , S. Carloni , A. Troisi

An interpretation of the formation of halo in accelerators based on quantum-like theory by a diffraction model is given in terms of the transversal beam motion. Physical implications of the longitudinal dynamics are also examined.

加速器物理 · 物理学 2009-10-31 Sameen Ahmed Khan , Modesto Pusterla

Flat galaxy rotation curves and the accelerating Universe both imply the existence of a critical acceleration, which is of the same order of magnitude in both the cases, in spite of the galactic and cosmic length scales being vastly…

广义相对论与量子宇宙学 · 物理学 2012-07-16 Priti Mishra , Tejinder P. Singh

The "cosmic triangle" is introduced as a way of representing the past, present, and future status of the universe. Our current location within the cosmic triangle is determined by the answers to three questions: How much matter is in the…

天体物理学 · 物理学 2009-09-15 N. Bahcall , J. P. Ostriker , S. Perlmutter , P. J. Steinhardt

In this paper we identify a new regularity in the systematics of galactic rotation curves, namely we find that at the last detected points in galaxies of widely varying luminosity, the centripetal acceleration is found to have the…

天体物理学 · 物理学 2009-10-28 Philip D. Mannheim

Assuming a suitable rotation of the Universe as a whole, we can attribute the rotation of galaxies to it. Using Lagrangian Mechanics we then can find the equations governing the rotation of a galaxy. We find in this way the azimuthal…

综合物理 · 物理学 2012-05-30 Evangelos Chaliasos

The flattening of spiral-galaxy rotation curves is unnatural in view of the expectations from Kepler's third law and a central mass. It is interesting, however, that the radius-independence velocity is what one expects in one less…

星系天体物理 · 物理学 2021-09-22 Felipe J. Llanes-Estrada

Rotation curves of spiral galaxies are the major tool for determining the distribution of mass in spiral galaxies. They provide fundamental information for understanding the dynamics, evolution and formation of spiral galaxies. We describe…

天体物理学 · 物理学 2019-02-25 Yoshiaki Sofue , Vera Rubin

It has been proposed that the flat rotation curves observed at large radii in disk galaxies can be interpreted as an effect of General Relativity (GR) instead of the presence of dark matter (DM) halos in Newtonian gravity. In Ciotti (2022)…

星系天体物理 · 物理学 2024-11-07 Luca Ciotti

The rotation curves of 20 spiral galaxies are examined in the light of a toy model (Soares 1992) which has as the main feature the assignment of a high M/L ratio (=30; Ho=50 km/s/Mpc) to the visible matter. The observed rotation of all…

天体物理学 · 物理学 2009-09-25 D. S. L. Soares

We use the rotation curves of more than 100 disk galaxies to examine whether the structure of their surrounding dark halos is consistent with the universal density profile proposed by Navarro, Frenk & White (NFW profiles). Rotation curve…

天体物理学 · 物理学 2007-05-23 Julio F. Navarro

Recent experimental results find strong indications that the universe is flat, while other experimental results from supernovae Ia observations have been interpreted to show that, not only that there is an accelerating expansion of the…

天体物理学 · 物理学 2012-08-27 George A. Baker,

The Horava - Lifshitz (HL) theory has recently attracted a lot of interest as a viable solution to some quantum gravity related problems and the presence of an effective cosmological constant able to drive the cosmic speed up. We show here…

宇宙学与河外天体物理 · 物理学 2015-05-18 V. F. Cardone , N. Radicella , M. L. Ruggiero , M. Capone

We present new mathematical alternatives for explaining rotation curves of spiral galaxies in the MOND context. For given total masses, it is shown that various mathematical alternatives to MOND, while predicting flat rotation curves for…

天体物理学 · 物理学 2007-05-23 Sandro S. e Costa , R. Opher

Circular velocities of stars and gas in galaxies generally do not decline in accordance with widely expected Keplerian fall-off in velocities further from the galactic nucleus. Two main groups of theories were proposed to explain the…

星系天体物理 · 物理学 2014-06-11 Konstantin Pavlovich , Alex Pavlovich , Alan Sipols
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