Tensor–vector–scalar gravity (TeVeS),
[
] developed by
Jacob Bekenstein
Jacob David Bekenstein (; May 1, 1947 – August 16, 2015) was a Mexican-born American-Israeli theoretical physicist who made fundamental contributions to the foundation of black hole thermodynamics and to other aspects of the connections betwee ...
in 2004, is a relativistic generalization of
Mordehai Milgrom's
Modified Newtonian dynamics (MOND) paradigm.
[
]
The main features of TeVeS can be summarized as follows:
* As it is derived from the
action principle, TeVeS respects
conservation laws;
* In the
weak-field approximation of the spherically symmetric, static solution, TeVeS reproduces the MOND acceleration formula;
* TeVeS avoids the problems of earlier attempts to generalize MOND, such as
superluminal
Faster-than-light (superluminal or supercausal) travel and communication are the conjectural propagation of matter or information faster than the speed of light in vacuum (). The special theory of relativity implies that only particles with zero ...
propagation;
* As it is a relativistic theory it can accommodate
gravitational lens
A gravitational lens is matter, such as a galaxy cluster, cluster of galaxies or a point particle, that bends light from a distant source as it travels toward an observer. The amount of gravitational lensing is described by Albert Einstein's Ge ...
ing.
The theory is based on the following ingredients:
* A unit
vector field
In vector calculus and physics, a vector field is an assignment of a vector to each point in a space, most commonly Euclidean space \mathbb^n. A vector field on a plane can be visualized as a collection of arrows with given magnitudes and dire ...
;
* A dynamical
scalar field
In mathematics and physics, a scalar field is a function associating a single number to each point in a region of space – possibly physical space. The scalar may either be a pure mathematical number ( dimensionless) or a scalar physical ...
;
* A nondynamical scalar field;
* A matter
Lagrangian constructed using an alternate
metric
Metric or metrical may refer to:
Measuring
* Metric system, an internationally adopted decimal system of measurement
* An adjective indicating relation to measurement in general, or a noun describing a specific type of measurement
Mathematics
...
;
* An arbitrary dimensionless function.
These components are combined into a relativistic
Lagrangian density, which forms the basis of TeVeS theory.
Details
MOND
[ is a phenomenological modification of the Newtonian acceleration law. In ]Newtonian gravity
Newton's law of universal gravitation describes gravity as a force by stating that every particle attracts every other particle in the universe with a force that is proportional to the product of their masses and inversely proportional to the sq ...
theory, the gravitational acceleration in the spherically symmetric, static field of a point mass at distance from the source can be written as
:
where is Newton's constant
The gravitational constant is an empirical physical constant involved in the calculation of gravitational effects in Sir Isaac Newton's law of universal gravitation and in Albert Einstein's theory of general relativity. It is also known as t ...
of gravitation. The corresponding force acting on a test mass is
:
To account for the anomalous rotation curves of spiral galaxies, Milgrom proposed a modification of this force law in the form
:
where is an arbitrary function subject to the following conditions:
:
In this form, MOND is not a complete theory: for instance, it violates the law of momentum conservation
In Newtonian mechanics, momentum (: momenta or momentums; more specifically linear momentum or translational momentum) is the Multiplication, product of the mass and velocity of an object. It is a Euclidean vector, vector quantity, possessi ...
.
However, such conservation laws are automatically satisfied for physical theories that are derived using an action principle. This led Bekenstein[ to a first, nonrelativistic generalization of MOND. This theory, called AQUAL (for A QUAdratic Lagrangian) is based on the Lagrangian
:
where is the Newtonian gravitational potential, is the mass density, and is a dimensionless function.
In the case of a spherically symmetric, static gravitational field, this Lagrangian reproduces the MOND acceleration law after the substitutions and are made.
Bekenstein further found that AQUAL can be obtained as the nonrelativistic limit of a relativistic field theory. This theory is written in terms of a Lagrangian that contains, in addition to the ]Einstein–Hilbert action
The Einstein–Hilbert action in general relativity is the action that yields the Einstein field equations through the stationary-action principle. With the metric signature, the gravitational part of the action is given as
:S = \int R \sqrt ...
for the metric field , terms pertaining to a unit vector field and two scalar fields and , of which only is dynamical. The TeVeS action, therefore, can be written as
:
The terms in this action include the Einstein–Hilbert Lagrangian (using a metric signature