Tests of gravitational symmetries with radio pulsars
arXiv:1604.03662 · doi:10.1007/s11433-016-0087-6
Abstract
Symmetries play important roles in modern theories of physical laws. In this paper, we review several experimental tests of important symmetries associated with the gravitational interaction, including the universality of free fall for self-gravitating bodies, time-shift symmetry in the gravitational constant, local position invariance and local Lorentz invariance of gravity, and spacetime translational symmetries. Recent experimental explorations for post-Newtonian gravity are discussed, of which, those from pulsar astronomy are highlighted. All of these tests, of very different aspects of gravity theories, at very different length scales, favor to very high precision the predictions of the strong equivalence principle (SEP) and, in particular, general relativity which embodies SEP completely. As the founding principles of gravity, these symmetries are motivated to be promoted to even stricter tests in future.
23 pages, 9 figures. Invited review article, minor modifications to match published version
References in corpus (28)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- The Confrontation between General Relativity and Experiment
- A Massive Pulsar in a Compact Relativistic Binary
- Quantum Gravity at a Lifshitz Point
- Tests of general relativity from timing the double pulsar
- Gravity Probe B: Final Results of a Space Experiment to Test General Relativity
- The relativistic pulsar-white dwarf binary PSR J1738+0333 II. The most stringent test of scalar-tensor gravity
- High-precision timing of 42 millisecond pulsars with the European Pulsar Timing Array
- Signals for Lorentz Violation in Post-Newtonian Gravity
- Models of non-relativistic quantum gravity: the good, the bad and the healthy
- Matter-gravity couplings and Lorentz violation
- Atom Interferometry tests of the isotropy of post-Newtonian gravity
- Neutron-star mergers in scalar-tensor theories of gravity
- What Do We Know About Lorentz Invariance?
- Gravitational-radiation losses from the pulsar-white-dwarf binary PSR J1141-6545
- Testing for Lorentz Violation: Constraints on Standard-Model Extension Parameters via Lunar Laser Ranging
- Short-range gravity and Lorentz violation
- Tests of local Lorentz invariance violation of gravity in the standard model extension with pulsars
- New tests of local Lorentz invariance of gravity with small-eccentricity binary pulsars
- Search for Lorentz violation in short-range gravity
- Pulsars and Gravity
- New pulsar limit on local Lorentz invariance violation of gravity in the standard-model extension
- Lorentz violation in the gravity sector: The t puzzle
- Phenomenology of theories of gravity without Lorentz invariance: the preferred frame case
- Search for Lorentz invariance violation through tests of the gravitational inverse square law at short-ranges
- Testing the strong equivalence principle with the triple pulsar PSR J0337+1715
- A characteristic observable signature of preferred frame effects in relativistic binary pulsars
- Testing Lorentz violation with binary pulsars: constraints on standard model extension
Cited by in corpus (42)
- Fundamental Physics with the Square Kilometre Array
- Testing the universality of free fall by tracking a pulsar in a stellar triple system
- Tests of Gravitational Symmetries with Pulsar Binary J1713+0747
- Constraining nonperturbative strong-field effects in scalar-tensor gravity by combining pulsar timing and laser-interferometer gravitational-wave detectors
- The Science of the Einstein Telescope
- Closing a spontaneous-scalarization window with binary pulsars
- Combined search for anisotropic birefringence in the gravitational-wave transient catalog GWTC-1
- PSR J2222--0137. I. Improved physical parameters for the system
- An effective action model of dynamically scalarizing binary neutron stars
- New Graviton Mass Bound from Binary Pulsars
- New limits on the Lorentz/CPT symmetry through fifty gravitational-wave events
- Reduced-order surrogate models for scalar-tensor gravity in the strong field and applications to binary pulsars and GW170817
- Strong-field effects in massive scalar-tensor gravity for slowly spinning neutron stars and application to X-ray pulsar pulse profiles
- Cosmological perturbations in Gauss-Bonnet quasi-dilaton massive gravity
- Testing velocity-dependent CPT-violating gravitational forces with radio pulsars
- Neutron stars as extreme laboratories for gravity tests
- Scalarized neutron stars in massive scalar-tensor gravity: X-ray pulsars and tidal deformability
- Testing the universality of free fall towards dark matter with radio pulsars
- Neutron stars in massive scalar-Gauss-Bonnet gravity: Spherical structure and time-independent perturbations
- Testing the Gravitational Weak Equivalence Principle in the Standard-Model Extension with Binary Pulsars
- Degeneracy in Studying the Supranuclear Equation of State and Modified Gravity with Neutron Stars
- Bounding the mass of graviton in a dynamic regime with binary pulsars
- Probing dipole radiation from binary neutron stars with ground-based laser-interferometer and atom-interferometer gravitational-wave observatories
- Numerical simulations of black hole-neutron star mergers in scalar-tensor gravity
- Prospects for Constraining the Yukawa Gravity with Pulsars around Sagittarius A*
- Extended reduced-order surrogate models for scalar-tensor gravity in the strong field and applications to binary pulsars and gravitational waves
- Strong Matter: Rethinking Philosophically
- Neutron Star Structure in the Minimal Gravitational Standard-Model Extension and the Implication to Continuous Gravitational Waves
- Newtonian approximation and possible time-varying in nonlocal gravities
- Simultaneous bounds on the gravitational dipole radiation and varying gravitational constant from compact binary inspirals
- Precession of spheroids under Lorentz violation and observational consequences for neutron stars
- Stringent Tests of Gravity with Highly Relativistic Binary Pulsars in the Era of LISA and SKA
- Lorentz-violating matter-gravity couplings in small-eccentricity binary pulsars
- Tests of conservation laws in post-Newtonian gravity with binary pulsars
- Lorentz-violating scalar Hamiltonian and equivalence principle in a static metric
- Radio Pulsars as a Laboratory for Strong-field Gravity Tests
- Scalar Dark Energy Models and Scalar-Tensor Gravity: Theoretical Explanations for the Accelerated Expansion of Present Universe
- Moment of Inertia for Axisymmetric Neutron Stars in the Standard-Model Extension
- Testing for gravitational preferred directions with galaxy and lensing surveys
- Pulsar tests of the graviton mass
- Tests of Classical Gravity with Radio Pulsars
- An independent test on the local position invariance of gravity with the triple pulsar PSR J0337+1715