Constraining Relativistic Generalizations of Modified Newtonian Dynamics with Gravitational Waves
Paul M. Chesler and Abraham Loeb
Index: 10.1103/PhysRevLett.119.031102
Full Text: HTML
Abstract
In the weak-field limit of general relativity, gravitational waves obey linear equations and propagate at the speed of light. These properties of general relativity are supported by the observation of ultrahigh-energy cosmic rays as well as by LIGO’s recent detection of gravitation waves. We argue that two existing relativistic generalizations of modified Newtonian dynamics, namely, the generalized Einstein-aether theory and bimetric modified Newtonian dynamics, display fatal inconsistencies with these observations.
Latest Articles:
Hippocampal Spike-Timing Correlations Lead to Hexagonal Grid Fields
2017-07-19
[10.1103/PhysRevLett.119.038101]
Nonuniform Currents and Spins of Relativistic Electron Vortices in a Magnetic Field
2017-07-18
[10.1103/PhysRevLett.119.030401]
Neural Decoder for Topological Codes
2017-07-18
[10.1103/PhysRevLett.119.030501]
Natural Covariant Planck Scale Cutoffs and the Cosmic Microwave Background Spectrum
2017-07-18
[10.1103/PhysRevLett.119.031301]
J/ψProduction and Polarization within a Jet
2017-07-18
[10.1103/PhysRevLett.119.032001]