Results 121 to 130 of about 64,819 (265)
Galaxy Rotation Curves from String Theory
15 pages, 1 table, 3 figures,1 appendix, LaTex in JHEP ...
Cheung, Yeuk-Kwan E. +2 more
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Constraining String Gauge Field by Planet Perihelion Precession and Galaxy Rotation Curves [PDF]
Feng Xu
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Global monopoles in Horndeski theory
In this article, global monopole solutions will be presented for the Horndeski theory by solving linearized field equations. We obtain two different classes of solutions depending on whether the Horndeski scalar field is massless or massive.
M. Haluk Seçuk, Özgür Delice
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Modified Newtonian dynamics (MOND) was originally proposed to model galaxy rotation curves without dark matter. However, MOND presents difficulties in explaining the radial acceleration relation observed in galaxy clusters, and moreover, it does not ...
Robert Monjo
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Raising galaxy rotation curves via dressing
We present a manifestly diffeomorphism-invariant simple model of galaxy dynamics obtained by applying the Dressing Field Method (DFM) to a general-relativistic system comprising the metric and four scalar fields, phenomenologically representing the four-velocity of a cosmological fluid or dust field.
J. François, L. Ravera
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Recent measurements of the Milky Way rotation curve found a sharp decline at around 15–20 kpc from the center of the Galaxy, suggesting that the Galactic dark matter halo is much less massive than predicted by other dynamical tracers.
Xiaowei Ou +5 more
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Rotation curves and dynamical masses of MaNGA barred galaxies [PDF]
E. O. Schmidt +3 more
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Galaxy rotation curves: the effect of $\vec{j} \times\vec{B}$ force [PDF]
D. Tsiklauri
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The Nearly Universal Disk Galaxy Rotation Curve
The universal rotation curve (URC) of disk galaxies was originally proposed to predict the shape and amplitude of any rotation curve (RC) based solely on photometric data.
Raj Patel +5 more
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Perfect fluid dark matter: a viability test with galaxy rotation curves
The anomalous rotation curves of galaxies provide compelling evidence for dark matter, yet its fundamental nature and distribution remain key unresolved issues in astrophysics.
Jan Kuncewicz
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