Tensor–vector–scalar gravity (TeVeS), developed by Jacob Bekenstein 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:
The theory is based on the following ingredients:
These components are combined into a relativistic Lagrangian density, which forms the basis of TeVeS theory.
MOND is a phenomenological modification of the Newtonian acceleration law. In Newtonian gravity theory, the gravitational acceleration in the spherically symmetric, static field of a point mass
M
r
a=-
GM | |
r2 |
,
where
G
m
F=ma.
To account for the anomalous rotation curves of spiral galaxies, Milgrom proposed a modification of this force law in the form
F=\mu\left(
a | |
a0 |
\right)ma,
where
\mu(x)
\mu(x)=\begin{cases}1&|x|\gg1\ x&|x|\ll1\end{cases}
In this form, MOND is not a complete theory: for instance, it violates the law of momentum conservation.
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
{lL}=- |
| f\left( | ||||||
8\piG |
|\nabla\Phi|2 | ||||||
|
\right)-\rho\Phi,
where
\Phi
\rho
f(y)
In the case of a spherically symmetric, static gravitational field, this Lagrangian reproduces the MOND acceleration law after the substitutions
a=-\nabla\Phi
\mu(\sqrt{y})=df(y)/dy
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 for the metric field
g\mu\nu
u\alpha
\sigma
\phi
\phi
STeVeS=\int\left({lL}g+{lL}s+{lL}
4x. | |
v\right)d |
The terms in this action include the Einstein–Hilbert Lagrangian (using a metric signature
[+,-,-,-]
c=1
{lL} | ||||
|
R\sqrt{-g},
where
R
g
The scalar field Lagrangian is
{lL} | ||||
|
\left[\sigma2h\alpha\beta\partial\alpha\phi\partial
|
G | |
l2 |
\sigma4F\left(kG\sigma2\right)\right]\sqrt{-g},
where
h\alpha\beta=g\alpha\beta-u\alphau\beta,l
k
F
{lL} | ||||
|
\left[g\alpha\betag\mu\nu\left(B\alpha\muB\beta\nu\right)+2
λ | |
K |
\left(g\mu\nuu\muu\nu-1\right)\right]\sqrt{-g}
where
B\alpha\beta=\partial\alphau\beta-\partial\betau\alpha,
K
k
K
K= | k |
2\pi |
K=-30+
72\pi | |
k |
.
K=3(\pm\sqrt{29}-5), k=6\pi(\pm\sqrt{29}-5)
The function
F
TeVeS also introduces a "physical metric" in the form
{\hatg}\mu\nu=e2\phig\mu\nu-2u\alphau\beta\sinh(2\phi).
The action of ordinary matter is defined using the physical metric:
Sm=\int{lL}\left({\hatg}\mu\nu,f\alpha,f
\alpha | |
|\mu |
,\ldots\right)\sqrt{-{\hatg}}d4x,
where covariant derivatives with respect to
{\hatg}\mu\nu
|.
TeVeS solves problems associated with earlier attempts to generalize MOND, such as superluminal propagation. In his paper, Bekenstein also investigated the consequences of TeVeS in relation to gravitational lensing and cosmology.
In addition to its ability to account for the flat rotation curves of galaxies (which is what MOND was originally designed to address), TeVeS is claimed to be consistent with a range of other phenomena, such as gravitational lensing and cosmological observations. However, Seifert shows that with Bekenstein's proposed parameters, a TeVeS star is highly unstable, on the scale of approximately 106 seconds (two weeks). The ability of the theory to simultaneously account for galactic dynamics and lensing is also challenged. A possible resolution may be in the form of massive (around 2eV) neutrinos.
A study in August 2006 reported an observation of a pair of colliding galaxy clusters, the Bullet Cluster, whose behavior, it was reported, was not compatible with any current modified gravity theory.
A quantity
EG
EG=0.392\pm{0.065}
f(R)
EG=0.22
TeVeS appears inconsistent with recent measurements made by LIGO of gravitational waves.