The Abell Cluster A586 and the Detection of the Equivalence Principle

Abstract

We discuss the current bounds on the Equivalence Principle, in particular from structure formation and, reexamine in this context, the recent claim on the evidence of the interaction between dark matter and dark energy in the Abell Cluster A586 and the ensued violation of the Equivalence Principle.

9 pages, 2 Figures. GRG format

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Cited by in corpus (56)

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• Observational constraint on interacting Tsallis holographic dark energy in logarithmic Brans-Dicke theory
• Signature of the interaction between dark energy and dark matter in observations
• Cosmological Constraints on the Sign-Changeable Interactions
• Mimicking dark matter in galaxy clusters through a non-minimal gravitational coupling with matter
• Mimicking dark matter through a non-minimal gravitational coupling with matter
• Cosmological Evolution of Quintessence and Phantom with a New Type of Interaction in Dark Sector
• Observational constraints on holographic tachyonic dark energy in interaction with dark matter
• A Consistent View of Interacting Dark Energy from Multiple CMB Probes
• Interacting new agegraphic tachyon, K-essence and dilaton scalar field models of dark energy in non-flat universe
• The imprint of the interaction between dark sectors in galaxy clusters
• Transient cosmic acceleration from interacting fluids
• Holographic dark energy in Brans-Dicke theory with log correction
• The generalized second law in irreversible thermodynamics for the interacting dark energy in a non-flat FRW universe enclosed by the apparent horizon
• The effect of Dark Matter and Dark Energy interactions on the peculiar velocity field and the kinetic Sunyaev-Zel'dovich effect
• Revisiting the Cosmological Constraints on the Interacting Dark Energy Models
• Quintessence with Yukawa Interaction
• Two-scalar-field model for the interaction of dark energy and dark matter
• A Model for Dark Energy decay
• Breaking parameter degeneracy in interacting dark energy models from observations
• Reconstructing interacting new agegraphic polytropic gas model in non-flat FRW universe
• Neutron Stars and Dark Matter
• Interacting entropy-corrected new agegraphic dark energy in non-flat universe
• Deep connection between f(R) gravity and the interacting dark sector model
• The signature of the scattering between dark sectors in large scale cosmic microwave background anisotropies
• On the change of old neutron star masses with galactocentric distance
• The cosmological constant problem: a user's guide
• The Layzer-Irvine equation in theories with non-minimal coupling between matter and curvature
• Phase Space Analysis and Thermodynamics of Interacting Umami Chaplygin gas in FRW Universe
• Indistinguishability of Warm Dark Matter, Modified Gravity, and Coupled Cold Dark Matter
• QCD modified ghost scalar field dark energy models
• Testing the interaction of dark energy to dark matter through the analysis of virial relaxation of clusters Abell Clusters A586 and A1689 using realistic density profiles
• The generalized second law for the interacting new agegraphic dark energy in a non-flat FRW universe enclosed by the apparent horizon
• Non-virialised clusters for detection of Dark Energy-Dark Matter interaction
• Interacting Quintessence in a New Scalar-Torsion Gravity
• Neutron star mass in dark matter clumps
• Interacting entropy-corrected holographic scalar field models in non-flat universe
• Cosmological evolution of quintessence with a sign-changing interaction in dark sector
• New observational constraints on interacting dark energy using galaxy clusters virial equilibrium states
• Entropy-corrected new agegraphic dark energy in Horava-Lifshitz cosmology
• Holographic field theory models of dark energy in interaction with dark matter
• Gamma-Ray Bursts and Dark Energy - Dark Matter interaction
• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia
• Interacting dark energy collapse with matter components separation
• Using simulated Tianqin gravitational wave data and electromagnetic wave data to study the coincidence problem and Hubble tension problem
• Phenomenological models of Universe with varying $G$ and $\Lambda$
• The role of Dark Matter interaction in galaxy clusters
• Bounds from multi-messenger astronomy on the Super Heavy Dark Matter
• Interacting dark fluid in the universe bounded by event horizon : A non-equilibrium prescription
• Constraining Violations of the Weak Equivalence Principle in the Dark Sector
• Revisiting Agegraphic Dark Energy in Brans-Dicke Cosmology
• Testing the Dark Universe through the Layzer-Irvine Equation