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

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Items 201–300 of 1,004

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20. New constraints on modified Newtonian dynamics from galaxy clusters
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25. Evolution of spiral galaxies in modified gravity
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27. PALATINI FORMULATION OF MODIFIED GRAVITY WITH A NON-MINIMAL CURVATURE-MATTER COUPLING
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31. Rotational velocity curves in the Milky Way as a test of modified gravity
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32. Classical tests for Weyl gravity: Deflection of light and time delay
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34. Dark Matter in the Galactic Dwarf Spheroidal Satellites
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35. ANDROMEDA DWARFS IN LIGHT OF MOND. II. TESTING PRIOR PREDICTIONS
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36. keV NEUTRINO MODEL BUILDING
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37. Black hole thermodynamics in MOdified Gravity (MOG)
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38. THE REAL PROBLEM WITH MOND
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39. The shape of the dark matter halo in the early-type galaxy NGC 2974
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40. General Theory of Relativity: Will It Survive the Next Decade?
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41. THE MOND LIMIT FROM SPACETIME SCALE INVARIANCE
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42. Reconciling the Diversity and Uniformity of Galactic Rotation Curves with Self-Interacting Dark Matter
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43. Problems for Modified Newtonian Dynamics in Clusters and the Lyα Forest?
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44. Can higher order curvature theories explain rotation curves of galaxies?
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45. Testing Modified Gravity with Globular Cluster Velocity Dispersions
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46. Dwarf spheroidals in MOND
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47. Quantum Gravity at Astrophysical Distances?
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48. Are Galactic Rotation Curves Really Flat? ∗
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51. Dark matter superfluidity and galactic dynamics
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52. Scaling laws in the distribution of galaxies
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53. THE GLOBULAR CLUSTER NGC 2419: A CRUCIBLE FOR THEORIES OF GRAVITY
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54. The DiskMass Survey. VII. The distribution of luminous and dark matter in spiral galaxies
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55. Gravitational polarization and the phenomenology of MOND
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56. The Ursa Major Cluster of Galaxies. II. Bimodality of the Distribution of Central Surface Brightnesses
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57. The Modified Dynamics as a vacuum effect
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58. The mass discrepancy acceleration relation in a ΛCDM context
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59. Quantum physics in space
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61. First Clear Signature of an Extended Dark Matter Halo in the Draco Dwarf Spheroidal
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62. The Beginning and Evolution of the Universe
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64. The MOND limit from space-time scale invariance
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65. MOND effects in the inner Solar system
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66. The Methodology of Scientific Research Programs
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67. Milky Way potentials in cold dark matter and MOdified Newtonian Dynamics. Is the Large Magellanic Cloud on a bound orbit?
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68. DARK MATTER AND DARK ENERGY AS EFFECTS OF MODIFIED GRAVITY
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69. Quasi-linear formulation of MOND
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70. Model of dark matter and dark energy based on gravitational polarization
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71. The Nature of UCDs: Internal Dynamics from an Expanded Sample and Homogeneous Database ⋆
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72. Proper Motions of Dwarf Spheroidal Galaxies fromHubble Space TelescopeImaging. III. Measurement for Ursa Minor
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73. Do we have any hope of detecting scattering between dark energy and baryons through cosmology?
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74. The Bullet Cluster 1E0657-558 evidence shows Modified Gravity in the absence of Dark Matter
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75. A massive stellar bulge in a regularly rotating galaxy 1.2 billion years after the Big Bang.
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76. A Tully-Fisher Relation for S0 Galaxies
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77. The mean mass density of the Universe
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78. TheXMMCluster Survey: testing chameleon gravity using the profiles of clusters
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79. Virial theorem and the dynamics of clusters of galaxies in the brane world models
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80. Towards a fully consistent parametrization of modified gravity
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82. Dark Matters on the Scale of Galaxies
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84. Proper Motions of Dwarf Spheroidal Galaxies fromHubble Space TelescopeImaging. II. Measurement for Carina
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86. Modified Newton's gravity in Finsler space as a possible alternative to dark matter hypothesis
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87. Brief Review on Scalar Field Dark Matter Models
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93. Nonlocal metric formulations of modified Newtonian dynamics with sufficient lensing
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100. The Halos of Satellite Galaxies: the Companion of the Massive Elliptical Lens SL2S J08544−0121⋆
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