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相关论文: Understanding Galaxy Rotation Curves with Verlinde…

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We examine whether the radial acceleration relation (RAR) of dwarf galaxies can be explained by Verlinde's emergent gravity. This is the extension of arXiv:2206.11685v3, which examines the RAR of typical spiral galaxies, to less massive…

广义相对论与量子宇宙学 · 物理学 2024-12-24 Sanghyeon Han , Ho Seong Hwang , Youngsub Yoon

We derive a formula for the velocity distribution of an axially symmetric galaxy where the mass density is corrected using the mass formula from special relativity. We take some reasonable test mass densities and numerically compute the…

广义相对论与量子宇宙学 · 物理学 2023-02-21 Jaroslaw S. Jaracz

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…

星系天体物理 · 物理学 2022-12-21 Kyu-Hyun Chae

The approximately flat outer parts of spiral galaxy rotation curves are commonly interpreted as evidence for a discrepancy between the observed baryonic mass and the dynamical mass inferred from the measured orbital velocities. In many…

星系天体物理 · 物理学 2026-05-08 Adolfo Santa Fe Dueñas

We apply the modified acceleration law obtained from Einstein gravity coupled explaining galaxy rotation curves without exotic dark matter. Our sample of galaxies includes low surface brightness (LSB) and high surface brightness (HSB)…

天体物理学 · 物理学 2016-08-30 J. R. Brownstein , J. W. Moffat

Verlinde (2016) has recently proposed that spacetime and gravity may emerge from an underlying microscopic theory. In a de Sitter spacetime, such emergent gravity (EG) contains an additional gravitational force due to dark energy, which may…

星系天体物理 · 物理学 2017-03-22 Federico Lelli , Stacy S. McGaugh , James M. Schombert

We present a new empirical model for galaxy rotation curves that introduces a velocity correction term {\omega}, derived from observed stellar motion and anchored to Keplerian baselines. Unlike parametric halo models or modified gravity…

星系天体物理 · 物理学 2026-01-05 David C. Flynn , Jim Cannaliato

Verlinde's theory of Emergent Gravity (EG) describes gravity as an emergent phenomenon rather than a fundamental force. Applying this reasoning in de Sitter space leads to gravity behaving differently on galaxy and galaxy cluster scales;…

宇宙学与河外天体物理 · 物理学 2019-05-30 Andrius Tamosiunas , David Bacon , Kazuya Koyama , Robert C. Nichol

The log-normal distribution represents the probability of finding randomly distributed particles in a micro canonical ensemble with high entropy. To a first approximation, a modified form of this distribution with a truncated termination…

星系天体物理 · 物理学 2015-03-12 John H. Marr

We test the predictions of Emergent Gravity using matter densities of relaxed, massive clusters of galaxies using observations from optical and X-ray wavebands. We improve upon previous work in this area by including the baryon mass…

宇宙学与河外天体物理 · 物理学 2019-08-14 John A. ZuHone , Jacob R. Sims

It was recently proposed that the effects usually attributed to particle dark matter on galaxy scales are due to the displacement of dark energy by baryonic matter, a paradigm known as emergent gravity. This formalism leads to predictions…

星系天体物理 · 物理学 2017-03-22 Aurelien Hees , Benoit Famaey , Gianfranco Bertone

We show quantitatively that an exact solution of Einstein's conformal gravity can explain very well the galactic rotation curves for a sample of 104 galaxies without need for dark matter or other exotic modification of gravity. The metric…

广义相对论与量子宇宙学 · 物理学 2019-06-13 Qiang Li , Leonardo Modesto

Verlinde (2016) has proposed a new modified theory of gravity, Emergent Gravity (EG), as an alternative to dark matter. EG reproduces the Tully-Fisher relationship with no free parameters and agrees with the velocity curves of most massive,…

宇宙学与河外天体物理 · 物理学 2020-12-09 Kris Pardo

We consider the consequences of applying general relativity to the description of the dynamics of a galaxy, given the observed flattened rotation curves. The galaxy is modeled as a stationary axially symmetric pressure-free fluid. In spite…

天体物理学 · 物理学 2010-10-27 F. I. Cooperstock , S. Tieu

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

As an alternative to dark matter models we use generalized Jordan-Brans-Dicke scalar-vector-tensor (JBD-SVT) gravity model to study the behavior of the rotational velocities of test particles moving around galaxies. To do so we consider an…

广义相对论与量子宇宙学 · 物理学 2019-06-05 Hossein Ghaffarnejad , Razieh Dehghani

Current constraints on gravity are relatively weak on galactic and intergalactic scales. Screened modified gravity models can exhibit complex behaviour there without violating stringent tests of gravity within our Solar System. They might…

宇宙学与河外天体物理 · 物理学 2018-08-15 Aneesh P. Naik , Ewald Puchwein , Anne-Christine Davis , Christian Arnold

An expression for rotational velocity of a test particle around the central mass in the invariant plane is derived. For this, a line element of Schwarzschild de-Sitter space-time is used to study the effect of cosmological constant…

宇宙学与河外天体物理 · 物理学 2013-07-09 B. Aryal , R. Pandey , N. Baral , U. Khanal , W. Saurer

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

We propose to test the viability of the recently introduced $f(\mathcal{R})$ gravity model in the galactic scales. For this purpose we consider test particles moving in stable circular orbits around the galactic center. We study the…

广义相对论与量子宇宙学 · 物理学 2023-05-17 Nashiba Parbin , Umananda Dev Goswami
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