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76 Results Found

  • Article
  • Open Access
3 Citations
12,875 Views
17 Pages

12 September 2025

This paper aims to explore whether astrophysical observations, primarily galaxy rotation curves, result from covarying coupling constants (CCC) rather than from dark matter. We have shown in earlier papers that cosmological observations, such as supe...

  • Article
  • Open Access
6 Citations
4,383 Views
12 Pages

23 December 2013

Using the multiplicity of solutions for the projectable case of the covariant extension of Hořava-Lifshitz gravity, we show that an appropriate choice for the auxiliary field allows for an effective description of galaxy rotation curves. This descrip...

  • Article
  • Open Access
2 Citations
2,839 Views
14 Pages

4 March 2020

Using the classical vacuum solutions of Newtonian gravity that do not explicitly involve matter, dark matter, or the gravitational constant, subject to an averaging process, a form of gravity relevant to the flattening of galaxy rotation curves resul...

  • Article
  • Open Access
1,825 Views
11 Pages

21 September 2023

Eicheon properties are discussed. It is shown that the eicheon surface allows setting a boundary condition for the vacuum polarization and obtaining a solution describing the dark matter tail in the Milky Way Galaxy. That is, the dark matter in the M...

  • Article
  • Open Access
7 Citations
2,427 Views
19 Pages

14 September 2021

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 dimension. In our t...

  • Article
  • Open Access
18 Citations
10,071 Views
24 Pages

14 April 2014

An accurate computational method is presented for determining the mass distribution in a mature spiral galaxy from a given rotation curve by applying Newtonian dynamics for an axisymmetrically rotating thin disk of finite size with or without a centr...

  • Article
  • Open Access
16 Citations
10,435 Views
32 Pages

Dark Matter Dogma: A Study of 214 Galaxies

  • Alan Sipols and
  • Alex Pavlovich

The aim of this paper is to test the need for non-baryonic dark matter in the context of galactic rotation and the apparent difference between distributions of galactic mass and luminosity. We present a set of rotation curves and 3.6 μm surface br...

  • Article
  • Open Access
10 Citations
5,411 Views
20 Pages

15 November 2018

Spiral galaxies are spinning, internally densified objects. The Virial Theorem explains galactic rotation curves via its linkage of the rotation rate to the gravitational self-potential (Ug) and the moment of inertia of oblate spheroids. We devise a...

  • Review
  • Open Access
7 Citations
6,620 Views
15 Pages

1 February 2020

The most cited evidence for (non-baryonic) dark matter has been an apparent lack of visible mass to gravitationally support the observed orbital velocity of matter in rotating disk galaxies, yet measurement of the mass of celestial objects cannot be...

  • Article
  • Open Access
9 Citations
4,476 Views
12 Pages

On the Dwarf Galaxy Rotation Curve Diversity Problem

  • Antonino Del Popolo,
  • Morgan Le Delliou and
  • Xiguo Lee

In this paper, we show how baryonic physics can solve the problem of the striking diversity in dwarf galaxy rotation curves shapes. To this aim, we compare the distribution of galaxies of the SPARC sample, in the plane V2kpc-VRlast (V2kpc being the g...

  • Article
  • Open Access
2,789 Views
16 Pages

8 October 2022

The rotational velocity curve, which is the circular velocity profile of the stars and gas in a spiral galaxy as a function of their distance from the galactic center, plays an important role in the kinematic and dynamic investigation of spiral galax...

  • Review
  • Open Access
7 Citations
10,913 Views
38 Pages

Proposed explanations of galactic rotation curves (RC = tangential velocity vs. equatorial radius, determined from Doppler measurements) involve dramatically different assumptions. A dominant, original camp invoked huge amounts of unknown, non-baryon...

  • Feature Paper
  • Article
  • Open Access
4 Citations
3,406 Views
9 Pages

In the Newtonian limit of general relativity a force acting on a test mass in a central gravitational field is conventionally defined by the attractive Newtonian gravity (inverse square) term plus a small repulsive cosmological force, which is propor...

  • Communication
  • Open Access
7 Citations
2,085 Views
11 Pages

27 September 2021

In this paper, we further elaborate on the Bose–Einstein condensate (BEC) dark matter model extended in our previous work [Phys. Rev. D 2020, 102, 083510] by the inclusion of sixth-order (or three-particle) repulsive self-interaction term. Herei...

  • Article
  • Open Access
10 Citations
4,743 Views
27 Pages

Axial Anomaly in Galaxies and the Dark Universe

  • Janning Meinert and
  • Ralf Hofmann

Motivated by the SU(2)CMB modification of the cosmological model ΛCDM, we consider isolated fuzzy-dark-matter lumps, made of ultralight axion particles whose masses arise due to distinct SU(2) Yang–Mills scales and the Planck mass MP. In contrast to...

  • Article
  • Open Access
4 Citations
2,902 Views
9 Pages

Galaxy Rotation Curve Fitting Using Machine Learning Tools

  • Carlos R. Argüelles and
  • Santiago Collazo

16 August 2023

Galaxy rotation curve (RC) fitting is an important technique which allows the placement of constraints on different kinds of dark matter (DM) halo models. In the case of non-phenomenological DM profiles with no analytic expressions, the art of findin...

  • Article
  • Open Access
15 Citations
8,134 Views
33 Pages

26 February 2020

Spiral galaxies and their rotation curves have key characteristics of differentially spinning objects. Oblate spheroid shapes are a consequence of spin and reasonably describe galaxies, indicating that their matter is distributed in gravitationally i...

  • Review
  • Open Access
109 Citations
17,906 Views
20 Pages

We review the current status of the study of rotation curve (RC) of the Milky Way, and present a unified RC from the Galactic Center to the galacto-centric distance of about 100 kpc. The RC is used to directly calculate the distribution of the surfac...

  • Article
  • Open Access
5 Citations
6,425 Views
22 Pages

6 September 2023

Recent independent observations using several different telescope systems and analysis methods have provided evidence of parity violation between the numbers of galaxies that spin in opposite directions. On the other hand, other studies argue that no...

  • Article
  • Open Access
8 Citations
4,343 Views
25 Pages

2 June 2023

Despite over a century of research, the physics of galaxy rotation is not yet fully understood, and there is a clear discrepancy between the observed mass of galaxies and their rotational velocity. Here, we report on another observation of tension be...

  • Review
  • Open Access
91 Citations
11,291 Views
86 Pages

Dark Matters on the Scale of Galaxies

  • Ivan de Martino,
  • Sankha S. Chakrabarty,
  • Valentina Cesare,
  • Arianna Gallo,
  • Luisa Ostorero and
  • Antonaldo Diaferio

1 August 2020

The cold dark-matter model successfully explains both the emergence and evolution of cosmic structures on large scales and, when we include a cosmological constant, the properties of the homogeneous and isotropic Universe. However, the cold dark-matt...

  • Proceeding Paper
  • Open Access
1,457 Views
4 Pages

Dark Matter in the Milky Way as the F-Type of Vacuum Polarization

  • Sergey L. Cherkas and
  • Vladimir L. Kalashnikov

Dark matter in the Milky Way is explained by the F-type of vacuum polarization, which could represent dark radiation. A nonsingular solution for dark radiation exists in the presence of eicheon (i.e., black hole in old terminology) in the galaxy&rsqu...

  • Article
  • Open Access
1,733 Views
14 Pages

The Schwarzschild–de Sitter Metric of Nonlocal dS Gravity

  • Ivan Dimitrijevic,
  • Branko Dragovich,
  • Zoran Rakic and
  • Jelena Stankovic

1 May 2024

It is already known that a simple nonlocal de Sitter gravity model, which we denote as dS gravity, contains an exact vacuum cosmological solution that mimics dark energy and dark matter and is in very good agreement with the standard model of cosmolo...

  • Proceeding Paper
  • Open Access
1 Citations
2,812 Views
6 Pages

In a recent paper, we have a shown that the flattening of galactic rotation curves can be explained by retardation. However, this relies on a temporal change of galactic mass. In our previous work, we kept only second order terms of the retardation t...

  • Communication
  • Open Access
642 Views
7 Pages

21 March 2025

A recent study using weak gravitational lensing revealed that the rotation curves of some isolated galaxies are found at a very large distance from their galactic centres. This may provide strong evidence supporting Modified Newtonian Dynamics (MOND)...

  • Article
  • Open Access
7 Citations
5,180 Views
14 Pages

When dealing with galactic dynamics, or more specifically, with galactic rotation curves, one basic assumption is always taken: the frame of reference relative to which the rotational velocities are given is assumed to be inertial. In other words, fi...

  • Article
  • Open Access
2,921 Views
10 Pages

Testing Noncommutativity-Like Model as a Galactic Density Profile

  • Juan Jordi Ancona-Flores,
  • Alberto Hernández-Almada and
  • Miguel Angel García-Aspeitia

Noncommutative-like model (NC-like) is an interesting alternative inspired by string theory to understand and describe the velocity rotation curves of galaxies without the inclusion of dark matter particles. In a natural way, a Gaussian density profi...

  • Article
  • Open Access
1 Citations
1,416 Views
19 Pages

As an alternative gravitational theory to General Relativity (GR), Conformal Gravity (CG) can be verified through astronomical observations. Currently, Mannheim and Kazanas have provided vacuum solutions for cosmological and local gravitational syste...

  • Article
  • Open Access
2 Citations
1,391 Views
9 Pages

17 November 2024

Gravity and electromagnetic interactions are the only fundamental physical interactions (outside the nuclear domain). In this work, we shall concentrate on Hamiltonians containing gravitational interaction, which according to general relativity must...

  • Feature Paper
  • Article
  • Open Access
12 Citations
4,549 Views
13 Pages

Dark Matter as a Non-Relativistic Bose–Einstein Condensate with Massive Gravitons

  • Emma Kun,
  • Zoltán Keresztes,
  • Saurya Das and
  • László Á. Gergely

17 October 2018

We confront a non-relativistic Bose–Einstein Condensate (BEC) model of light bosons interacting gravitationally either through a Newtonian or a Yukawa potential with the observed rotational curves of 12 dwarf galaxies. The baryonic component is...

  • Review
  • Open Access
5 Citations
4,034 Views
45 Pages

13 September 2021

Dark matter (DM) is one of the biggest mystery in the Universe. In this review, we start reporting the evidences for this elusive component and discussing about the proposed particle candidates and scenarios for such phenomenon. Then, we focus on rec...

  • Feature Paper
  • Conference Report
  • Open Access
5 Citations
3,575 Views
8 Pages

Galactic Structures from Gravitational Radii

  • Salvatore Capozziello,
  • Duško Borka,
  • Vesna Borka Jovanović and
  • Predrag Jovanović

7 February 2018

We demonstrate that the existence of a Noether symmetry in f ( R ) theories of gravity gives rise to an additional gravitational radius, besides the standard Schwarzschild one, determining the dynamics at galactic scales. By this feature, it...

  • Feature Paper
  • Article
  • Open Access
9 Citations
6,586 Views
16 Pages

7 November 2017

[-5]The applications of Newtonian dynamics in galactic scales have shown that the inverse square law is incompatible with the amount of visible mass in the form of stars and molecular clouds. This manifests as the rotational curves of galaxies being...

  • Article
  • Open Access
2 Citations
2,702 Views
15 Pages

Retarded Gravity in Disk Galaxies

  • Yuval Glass,
  • Tomer Zimmerman and
  • Asher Yahalom

26 March 2024

Disk galaxies have a typical dimension of a few tens of kiloparsecs. It follows from the theory of general relativity that any signal originating from the galactic center will be noticed at the outskirts of the galaxy only tens of thousands of years...

  • Article
  • Open Access
1 Citations
1,723 Views
14 Pages

PossibleExistence of Dark-Matter-Admixed Pulsar in the Disk Region of the Milky Way Galaxy

  • Nilofar Rahman,
  • Masum Murshid,
  • Sajahan Molla and
  • Mehedi Kalam

7 December 2022

In our previous study, (Eur Phys J Plus 135:362, 2020 & Eur Phys J Plus 135:637, 2020), we have discussed the possible existence of the dark-matter-admixed pulsars, located in dwarf as well as in massive spiral galaxies (based on Singular Isother...

  • Article
  • Open Access
7 Citations
1,784 Views
38 Pages

Geometric Origin of the Galaxies’ Dark Side

  • Leonardo Modesto,
  • Tian Zhou and
  • Qiang Li

29 December 2023

We show that Einstein’s conformal gravity can explain, simply, and on the geometric ground, galactic rotation curves, without the need to introduce any modification in both the gravitational as well as in the matter sector of the theory. The ge...

  • Article
  • Open Access
638 Views
18 Pages

24 November 2025

We resume our analysis of Newtonian Fractional-Dimension Gravity (NFDG), an alternative gravitational model that does not require the dark matter (DM) paradigm. We add three more galaxies (NGC 6946, NGC 3198, NGC 2841) to the catalog of those studied...

  • Article
  • Open Access
4 Citations
2,325 Views
19 Pages

Dark Matter in Fractional Gravity III: Dwarf Galaxies Kinematics

  • Francesco Benetti,
  • Andrea Lapi,
  • Giovanni Gandolfi,
  • Minahil Adil Butt,
  • Yacer Boumechta,
  • Balakrishna S. Haridasu and
  • Carlo Baccigalupi

8 November 2023

Recently, we put forward a framework where the dark matter (DM) component within virialized halos is subject to a non-local interaction originated by fractional gravity (FG) effects. In previous works, we demonstrated that such a framework can substa...

  • Article
  • Open Access
7 Citations
2,503 Views
15 Pages

We apply Newtonian fractional-dimension gravity (NFDG), an alternative gravitational model, to some notable cases of galaxies with little or no dark matter. In the case of the ultra-diffuse galaxy AGC 114905, we show that NFDG methods can effectively...

  • Article
  • Open Access
19 Citations
4,466 Views
25 Pages

15 October 2020

We derive an effective gravitational potential, induced by the quantum wavefunction of a physical vacuum of a self-gravitating configuration, while the vacuum itself is viewed as the superfluid described by the logarithmic quantum wave equation. We d...

  • Article
  • Open Access
3,108 Views
6 Pages

18 October 2017

Monitoring of the lens system JVAS B0218+357 with the Fermi Gamma-ray Space Telescope measured a different time delay to that derived from radio observations. We have re-analysed three months of archival Very Large Array data to produce variability c...

  • Article
  • Open Access
2 Citations
1,605 Views
28 Pages

6 September 2024

The baryonic mass–velocity relation provides an important test of different galaxy dynamics models such as Lambda–cold dark matter (ΛCDM) and alternatives like Modified Newtonian Dynamics (MOND). Novel nonlinear density wave theory...

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