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

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Items 701–800 of 1,004

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29. The formation of cosmic structure with modified Newtonian dynamics
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45. Ultra-diffuse cluster galaxies as key to the MOND cluster conundrum
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46. Cosmological variation of the MOND constant: Secular effects on galactic systems
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50. Applications of Fractional Calculus to Newtonian Mechanics
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52. Alternatives to Einstein’s General Relativity Theory
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53. The MUSE-Faint survey
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55. Modified gravity models and the central cusp of dark matter haloes in galaxies
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56. Do non-relativistic neutrinos constitute the dark matter?
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57. The escape velocity curve of the Milky Way in modified Newtonian dynamics
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58. Aether unleashed
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59. Exponential potential versus dark matter
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60. Constraining the Gravitational Potential from the Projected Morphology of Extragalactic Tidal Streams
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62. Nonlocal metric realizations of MOND
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63. Testing Newtonian gravity in the low acceleration regime with globular clusters: the case ofω Centauri revisited
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64. Compact stars with a small electric charge: the limiting radius to mass relation and the maximum mass for incompressible matter
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70. Testing Gravity in the Outer Solar System: Results from Trans‐Neptunian Objects
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71. Evidence for Galaxy Dynamics Tracing Background Cosmology Below the de Sitter Scale of Acceleration
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72. Test of modified Newtonian dynamics with recent Boomerang data
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73. MOND and the Universal Rotation Curve: Similar Phenomenologies
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75. Measuring Spacetime: From the Big Bang to Black Holes
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78. Gravity, antimatter and the Dirac-Milne universe
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80. Is there a fundamental acceleration scale in galaxies?
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82. Models of a modified-inertia formulation of MOND
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83. Wide Binaries from GAIA EDR3: preference for GR over MOND?
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86. Investigation of dark matter and modified Newtonian dynamics in early-type galaxies through globular cluster systems
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93. Masses, Tidal Radii, and Escape Speeds in Dwarf Spheroidal Galaxies under MOND and Dark Halos Compared
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94. Constraints on alternative models to dark energy
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