REVIEW 8 cited by
Scalar-Tensor-Vector Gravity Theory
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
abstract
A covariant scalar-tensor-vector gravity theory is developed which allows the gravitational constant $G$, a vector field coupling $\omega$ and the vector field mass $\mu$ to vary with space and time. The equations of motion for a test particle lead to a modified gravitational acceleration law that can fit galaxy rotation curves and cluster data without non-baryonic dark matter. The theory is consistent with solar system observational tests. The linear evolutions of the metric, vector field and scalar field perturbations and their consequences for the observations of the cosmic microwave background are investigated.
Forward citations
Cited by 8 Pith papers
-
Compact binary systems in Einstein-{\AE}ther gravity. II. Radiation reaction to 2.5 post-Newtonian order
The paper derives radiative equations of motion for Einstein-Aether compact binaries to 2.5PN order and reports energy-loss rates that contradict earlier flux-based calculations, with the dipole rate depending only on...
-
Parametrized beyond-Teukolsky framework in the time domain
First time-domain implementation of the parametrized beyond-Teukolsky framework, validated against frequency-domain benchmarks for low multipoles and yielding new amplitude, phase, quadratic-coefficient, and tail-onse...
-
Breathing Black Hole Shadows in Modified Gravity (MOG)
In MOG gravity, gravitational waves would make a black hole's shadow breathe in area and then wobble translationally after a time delay, signatures absent in general relativity.
-
D-dimensional black holes in extended Gauss-Bonnet gravity
Charged and rotating anti-de Sitter black hole solutions are constructed in extended Gauss-Bonnet gravity for dimensions three, four, five and higher.
-
Regular Rotating Black Hole: Probing the boundaries of the Radiative Signatures and Jet Power
MOG regular rotating black holes are compatible with most X-ray binary data only for beta below about 0.38 to 0.4, and are excluded for the near-extremal source GRS 1915+105.
-
Eikonal Quality-Factor Parameterization of Model-Conditional Static Black-Hole Thermodynamics
A quasinormal frequency ratio can invert a one-parameter black-hole family, and RN and static MOG are exactly isospectral for neutral test scalars with different Wald entropies.
-
Connection Between the Shadow Radius and Quasinormal Frequencies for Black Holes in STVG with Perfect Fluid Dark Matter
In STVG with PFDM, eikonal QNM real frequencies equal multipole number over shadow radius, so shadow size and ringdown are dual photon-sphere observables.
-
Signatures of modified gravity from the gravitational Aharonov-Bohm effect
For a Kaluza-Klein modified gravitational potential, the gravitational Aharonov-Bohm phase produces energy-level shifts that are dominated by an assumed constant correction to Newton's constant, while the claimed new ...
Discussion (0). Continue with ORCID to comment.