Cosmological consequences of a rolling homogeneous scalar field

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Items 201–300 of 1,006

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2. Thermodynamics of dark energy interacting with dark matter and radiation
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3. Effective gravitational couplings for cosmological perturbations in the most general scalar–tensor theories with second-order field equations
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4. Constraints on the sum of the neutrino masses in dynamical dark energy models with w(z)≥−1 are tighter than those obtained in ΛCDM
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5. Statefinder diagnostic for coupled quintessence
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6. Cosmography and constraints on the equation of state of the Universe in various parametrizations
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7. THEORETICAL MODELS OF DARK ENERGY
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8. Searching for an Oscillating Massive Scalar Field as a Dark Matter Candidate Using Atomic Hyperfine Frequency Comparisons
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9. Interacting holographic phantom
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10. A Review on the Scalar Field/Bose-Einstein Condensate Dark Matter Model
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11. Extended holographic dark energy
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12. Fate of bound systems in phantom and quintessence cosmologies
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13. Cosmological observations in scalar-tensor quintessence
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14. Could supermassive black holes be quintessential primordial black holes?
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15. Phase-space analysis of teleparallel dark energy
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16. Quintom models with an equation of state crossing − 1
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17. Dark synergy: Gravitational lensing and the CMB
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18. Dark matter and background light
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19. Dimming Supernovae without Cosmic Acceleration
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20. Modified theories of gravity: Why, how and what?
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21. Median Statistics,H0, and the Accelerating Universe
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22. Spherical symmetry in f(R)-gravity
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23. Thawing quintessence with a nearly flat potential
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24. Rock ‘n’ roll solutions to the Hubble tension
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25. The clustering of galaxies in the SDSS-III DR9 Baryon Oscillation Spectroscopic Survey: testing deviations from Λ and general relativity using anisotropic clustering of galaxies
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26. HydrodynamicalN-body simulations of coupled dark energy cosmologies
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27. Relic gravity waves from braneworld inflation
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28. Electroweak baryogenesis and the expansion rate of the Universe
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29. Dark energy in Horndeski theories after GW170817: A review
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30. Early dark energy cosmologies
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31. Reconciling CMB and structure growth measurements with dark energy interactions
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32. The dynamics of quintessence, the quintessence of dynamics
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33. Cosmological dynamics of the tachyon with an inverse power-law potential
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34. Cosmology with a stiff matter era
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35. Effective field theory of dark energy: A review
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36. Dynamical vacuum energy, holographic quintom, and the reconstruction of scalar-field dark energy
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37. Dark Energy in Light of Multi-Messenger Gravitational-Wave Astronomy
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38. Latest supernova data in the framework of the generalized Chaplygin gas model
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39. Extended dark energy analysis using DESI DR2 BAO measurements
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40. Transition redshift: new kinematic constraints from supernovae
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41. Quantum tests of the Einstein Equivalence Principle with the STE–QUEST space mission
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42. Is the dark matter a solid?
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44. Cosmological solutions of f(T) gravity
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45. Hubble expansion and structure formation in time varying vacuum models
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46. New cosmological tracker solution for quintessence
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47. Cosmological constraints on Bose-Einstein-condensed scalar field dark matter
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48. Dark coupling
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49. Cosmology with Interaction between Phantom Dark Energy and Dark Matter and the Coincidence Problem
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50. Cosmological constant problem and quintessence
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51. Crossing the phantom divide barrier with scalar tensor theories
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52. hi_class: Horndeski in the Cosmic Linear Anisotropy Solving System
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53. Relating gravitational wave constraints from primordial nucleosynthesis, pulsar timing, laser interferometers, and the CMB: Implications for the early universe
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54. Bulk–brane interaction and holographic dark energy
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55. Renormalization group improved gravitational actions: A Brans-Dicke approach
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56. Quintessence and scalar dark matter in the Universe
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57. Early-universe constraints on dark energy
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58. Reconstructing holographic quintessence
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59. Kinematic constraints to the transition redshift from supernovae type Ia union data
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60. Generalized Chaplygin gas as a unified scenario of dark matter/energy: Observational constraints
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61. Inflation and preheating in nonoscillatory models
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62. A new view ofk-essence
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63. Steep inflation: Ending braneworld inflation by gravitational particle production
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64. Dynamical dark energy: Current constraints and forecasts
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65. Searching for C P T Violation with Cosmic Microwave Background Data from WMAP and BOOMERANG
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66. Cosmographic bounds on the cosmological deceleration-acceleration transition redshift in f(R) gravity
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67. Field-theoretical formulations of MOND-like gravity
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68. Neutrino Mass Ordering from Oscillations and Beyond: 2018 Status and Future Prospects
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69. Generalized second law of thermodynamics in quintom dominated universe
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70. Expansion around the vacuum equation of state: Sudden future singularities and asymptotic behavior
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71. Effective equation of state for dark energy: Mimicking quintessence and phantom energy through a variable Λ
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72. Solving the Coincidence Problem: Tracking Oscillating Energy
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73. Future supernovae data and quintessence models
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74. Model independent approach to the dark energy equation of state
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75. An alternative f(R, T) gravity theory and the dark energy problem
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76. Recent developments in bimetric theory
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77. Does Hubble tension signal a breakdown in FLRW cosmology?
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78. Recent developments in bimetric theory
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79. H0 tension, phantom dark energy, and cosmological parameter degeneracies
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80. Cosmological Parameters from the 2003 Flight of BOOMERANG
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81. 8 How to determine an effective potential for a variable cosmological term
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82. Gravity Resonance Spectroscopy Constrains Dark Energy and Dark Matter Scenarios
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83. On the Growth of Perturbations as a Test of Dark Energy and Gravity
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84. Inflation, braneworlds and quintessence
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85. New varying speed of light theories
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86. Interacting holographic dark energy model and generalized second law of thermodynamics in a non-flat universe
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87. Interacting Holographic Phantom
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88. Measuring the Speed of Sound of Quintessence
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89. Generalized phantom energy
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90. Nonlocal quantum gravity: A review
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91. Cosmological constraints on the dark energy equation of state and its evolution
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92. Experimental Tests of General Relativity
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93. Generalized Galileon cosmology
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94. The acceleration of the universe and the physics behind it
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95. A single scalar field model of dark energy with equation of state crossing −1
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96. Cosmological effects of a class of fluid dark energy models
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97. Holographic tachyon model of dark energy
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98. T HE C OSMIC M ICROWAVE B ACKGROUND AND P ARTICLE P HYSICS
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99. String or M theory axion as a quintessence
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100. Dark energy cosmology with generalized linear equation of state
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