A modification of the Newtonian dynamics as a possible alternative to the hidden mass hypothesis

Cited by (1,004)

Items 801–900 of 1,004

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9. The Star Formation History and Dynamics of the Ultra-diffuse Galaxy Dragonfly 44 in MOND and MOG
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10. On the absence of a universal surface density, and a maximum Newtonian acceleration in dark matter haloes: Consequences for MOND
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11. Modified inertia from extended uncertainty principle(s) and its relation to MoND
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12. Probing the radial acceleration relation and the strong equivalence principle with the Coma cluster ultra-diffuse galaxies
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13. Statistical analysis of the gravitational anomaly in Gaia wide binaries
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14. Dark matter effects in vacuum spacetime
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16. An analytic model for non-spherical lenses in covariant MOdified Newtonian Dynamics
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17. Testing modified gravity models with recent cosmological observations
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18. Galaxy rotation curves in the Grumiller's modified gravity
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19. Deep imaging of the shell elliptical galaxy NGC 3923 with MegaCam
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20. Probing the boundary between star clusters and dwarf galaxies: A MUSE view on the dynamics of Crater/Laevens I
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21. Verlinde’s emergent gravity versus MOND and the case of dwarf spheroidals
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22. Stellar accelerations and the galactic gravitational field
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23. The properties of dwarf spheroidal galaxies in the Cen A group
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24. Implications for dwarf spheroidal mass content from interloper removal
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25. Massive Elliptical Galaxies: From Cores to Halos
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26. The velocity dispersion and mass function of the outer halo globular cluster Palomar 4
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27. Long-term periodicity of sedimentary basins in response to astronomical forcing: Review and perspective
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29. Modied Gravity and Cosmology
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30. The Case for Nonlocal Modifications of Gravity
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31. Observational tests of the self-dual spacetime in loop quantum gravity
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32. Lorentz Symmetry Group, Retardation, Intergalactic Mass Depletion and Mechanisms Leading to Galactic Rotation Curves
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33. Cooling process of brown dwarfs in Palatini f(R) gravity
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34. Towards a full general relativistic approach to galaxies
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35. Fast full N-body simulations of generic modified gravity: derivative coupling models
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36. The formation of early-type galaxies through monolithic collapse of gas clouds in Milgromian gravity
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37. Novel constraints on fifth forces and ultralight dark sector with asteroidal data
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38. On the tension between the radial acceleration relation and Solar system quadrupole in modified gravity MOND
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39. Finslerian MOND versus observations of Bullet Cluster 1E 0657−558
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40. Galactic rotation curves in brane world models
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41. Testing quantised inertia on galactic scales
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42. The velocity distribution of Sloan Digital Sky Survey satellites in Modified Newtonian Dynamics
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43. Current data on the globular cluster Palomar 14 are consistent with MOND
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44. The Intrinsic Scatter of the Radial Acceleration Relation*
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45. The Origin of Galaxies and Clusters of Galaxies
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46. Probing the Mass Distributions in NGC 1407 and Its Associated Group with the X‐Ray Imaging Spectroscopic and Optical Photometric and Line‐Strength Indices Data
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47. Vector field theories in cosmology
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48. Modified gravity, dark energy and modified Newtonian dynamics
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49. Do non-relativistic neutrinos constitute the dark matter?
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50. High-energy scalarons in R2 gravity as a model for Dark Matter in galaxies
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51. The Effect of Retardation on Galactic Rotation Curves
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52. The Milky Way’s rotation curve with superfluid dark matter
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53. The Phantom of RAMSES user guide for galaxy simulations using Milgromian and Newtonian gravity
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54. The Phantom Dark Matter Halos of the Local Volume in the Context of Modified Newtonian Dynamics
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55. Rotation Curves of Galaxies and Their Dependence on Morphology and Stellar Mass
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56. DGSAT: Dwarf Galaxy Survey with Amateur Telescopes
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57. Aether scalar tensor theory: Linear stability on Minkowski space
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58. X-ray analysis of JWST’s first galaxy cluster lens SMACS J0723.3−7327
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59. The flat density profiles of massive, and relaxed galaxy clusters
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60. ENTROPIC GRAVITY, MINIMUM TEMPERATURE, AND MODIFIED NEWTONIAN DYNAMICS
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61. Scalars, vectors and tensors from metric-affine gravity
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62. The velocity field in MOND cosmology
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63. The Scale-Invariant Vacuum (SIV) Theory: A Possible Origin of Dark Matter and Dark Energy
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64. Using distant globular clusters as a test for gravitational theories
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65. Structure formation on the brane: A mimicry
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66. An f(R) gravitation for galactic environments
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67. Origin of the spectacular tidal shells of galaxy NGC 474
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68. Dark matter signatures of black holes with Yukawa potential
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69. Apparent and emergent dark matter around a Schwarzschild black hole
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70. Testing quasilinear modified Newtonian dynamics in the Solar System
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71. Fluids, superfluids and supersolids: dynamics and cosmology of self-gravitating media
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72. An elementary canonical classical and quantum dynamics for general relativity
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73. The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology
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74. A first attempt to differentiate between modified gravity and modified inertia with galaxy rotation curves
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75. The universal acceleration scale from stellar feedback
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76. Next Generation Design and Prospects for Cannex
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77. Distinguishing Dark Matter, Modified Gravity, and Modified Inertia with the Inner and Outer Parts of Galactic Rotation Curves
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78. Radial acceleration relation of galaxies with joint kinematic and weak-lensing data
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79. Inflation and accelerated expansion tensor-vector-scalar cosmological solutions
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80. Vector field and rotational curves in dark galactic halos
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81. From magnitudes and redshifts of supernovae, their light-curves, and angular sizes of galaxies to a tenable cosmology
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82. Quantum statistical modified entropic gravity as a theoretical basis for MOND
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83. General virial theorem for modified-gravity MOND
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84. Conservation, inertia, and spacetime geometry
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85. The prediction of rotation curves in gas-dominated dwarf galaxies with modified dynamics
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86. Bosonic coherent motions in the Universe
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87. Tidal streams in a MOND potential: constraints from Sagittarius
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88. Jeans Instability of Dissipative Self-Gravitating Bose–Einstein Condensates with Repulsive or Attractive Self-Interaction: Application to Dark Matter
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95. THE GALACTIC POTENTIAL AND THE ASYMMETRIC DISTRIBUTION OF HYPERVELOCITY STARS
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