Gauge vector–tensor gravity (GVT) is a relativistic generalization of Mordehai Milgrom's Modified Newtonian dynamics (MOND) paradigm where gauge fields cause the MOND behavior. The former covariant realizations of MOND such as the Bekenestein's Tensor–vector–scalar gravity and the Moffat's Scalar–tensor–vector gravity attribute MONDian behavior to some scalar fields. GVT is the first example wherein the MONDian behavior is mapped to the gauge vector fields. The main features of GVT can be summarized as follows:
Contents
- Details
- Action
- Coupling to the matter
- Regimes of the GVT theory
- Strong and Newtonian regimes
- MOND regime
- Post MONDian regime
- References
Its dynamical degrees of freedom are:
Details
The physical geometry, as seen by particles, represents the Finsler geometry–Randers type:
This implies that the orbit of a particle with mass
The geometrical quantities are Riemannian. GVT, thus, is a bi-geometric gravity.
Action
The metric's action coincides to that of the Einstein–Hilbert gravity:
where
and
where L has the following MOND asymptotic behaviors
and
Coupling to the matter
Metric couples to the energy-momentum tensor. The matter current is the source field of both gauge fields. The matter current is
where
Regimes of the GVT theory
GVT accommodates the Newtonian and MOND regime of gravity; but it admits the post-MONDian regime.
Strong and Newtonian regimes
The strong and Newtonian regime of the theory is defined to be where holds:
The consistency between the gravitoelectromagnetism approximation to the GVT theory and that predicted and measured by the Einstein–Hilbert gravity demands that
which results to
MOND regime
The MOND regime of the theory is defined to be
So the action for the
So the GVT theory is capable of reproducing the flat rotational velocity curves of galaxies. The current observations do not fix
Post-MONDian regime
The post-MONDian regime of the theory is defined where both of the actions of the