HOME

TheInfoList



OR:

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: * 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 propagation; * As it is a relativistic theory it can accommodate gravitational lensing. The theory is based on the following ingredients: * A unit vector field; * A dynamical
scalar field In mathematics and physics, a scalar field is a function associating a single number to every point in a space – possibly physical space. The scalar may either be a pure mathematical number (dimensionless) or a scalar physical quantity ...
; * A nondynamical scalar field; * A matter Lagrangian constructed using an alternate metric; * An arbitrary dimensionless function. These components are combined into a relativistic
Lagrangian density Lagrangian may refer to: Mathematics * Lagrangian function, used to solve constrained minimization problems in optimization theory; see Lagrange multiplier ** Lagrangian relaxation, the method of approximating a difficult constrained problem with ...
, which forms the basis of TeVeS theory.


Details

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 at distance r from the source can be written as :a = -\frac, where G is Newton's constant of gravitation. The corresponding force acting on a test mass m is :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 (\frac \right )ma, where \mu(x) is an arbitrary function subject to the following conditions: :\mu(x)= \begin 1 & , x, \gg 1 \\ x & , x, \ll 1 \end 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 :=-\fracf\left(\frac\right)-\rho\Phi, where \Phi is the Newtonian gravitational potential, \rho is the mass density, and f(y) is a dimensionless function. In the case of a spherically symmetric, static gravitational field, this Lagrangian reproduces the MOND acceleration law after the substitutions a=-\nabla\Phi and \mu(\sqrt)=df(y)/dy 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 (also referred to as 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 a ...
for the metric field g_, terms pertaining to a unit vector field u^\alpha and two scalar fields \sigma and \phi, of which only \phi is dynamical. The TeVeS action, therefore, can be written as :S_\mathrm=\int\left(_g+_s+_v\right)d^4x. The terms in this action include the Einstein–Hilbert Lagrangian (using a metric signature ,-,-,-/math> and setting the speed of light, c=1): :_g=-\fracR\sqrt, where R is the Ricci scalar and g is the determinant of the metric tensor. The scalar field Lagrangian is :_s=-\frac\left sigma^2h^\partial_\alpha\phi\partial_\beta\phi+\frac\frac\sigma^4F \left (kG\sigma^2 \right)\rightsqrt, where h^=g^-u^\alpha u^\beta, l is a constant length, k is the dimensionless parameter and F an unspecified dimensionless function; while the vector field Lagrangian is :_v=-\frac\left ^g^ \left (B_B_ \right )+2\frac \left (g^u_\mu u_\nu-1 \right )\rightsqrt where B_=\partial_\alpha u_\beta-\partial_\beta u_\alpha, while K is a dimensionless parameter. k and K are respectively called the scalar and vector coupling constants of the theory. The consistency between the
Gravitoelectromagnetism Gravitoelectromagnetism, abbreviated GEM, refers to a set of formal analogies between the equations for electromagnetism and relativistic gravitation; specifically: between Maxwell's field equations and an approximation, valid under certain ...
of the TeVeS theory and that predicted and measured by the Gravity Probe B leads to K=\frac, and requiring consistency between the near horizon geometry of a black hole in TeVeS and that of the Einstein theory, as observed by the
Event Horizon Telescope The Event Horizon Telescope (EHT) is a large telescope array consisting of a global network of radio telescopes. The EHT project combines data from several very-long-baseline interferometry (VLBI) stations around Earth, which form a combined arr ...
leads to K=-30 + \frac. So the coupling constants read: :K= 3(\pm\sqrt-5), \kappa = 6\pi (\pm \sqrt-5) The function F in TeVeS is unspecified. TeVeS also introduces a "physical metric" in the form :^=e^g^-2u^\alpha u^\beta\sinh(2\phi). The action of ordinary matter is defined using the physical metric: :S_m=\int \left (_,f^\alpha,f^\alpha_,\ldots \right)\sqrtd^4x, where covariant derivatives with respect to _ are denoted by , . 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.


Problems and criticisms

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 E_G probing general relativity (GR) on large scales (a hundred billion times the size of the solar system) for the first time has been measured with data from the Sloan Digital Sky Survey to be E_G=0.392\pm (~16%) consistent with GR, GR plus Lambda CDM and the extended form of GR known as f(R) theory, but ruling out a particular TeVeS model predicting E_G=0.22. This estimate should improve to ~1% with the next generation of sky surveys and may put tighter constraints on the parameter space of all modified gravity theories. TeVeS appears inconsistent with recent measurements made by LIGO of gravitational waves.


See also

* Gauge vector–tensor gravity * Modified Newtonian dynamics * Nonsymmetric gravitational theory * Scalar–tensor–vector gravity


References


Further reading

* *
Dark Matter Observed
( SLAC Today)
Einstein's Theory 'Improved'?
( PPARC)
Einstein Was Right: General Relativity Confirmed
' TeVeS, however, made predictions that fell outside the observational error limits', (
Space.com Space.com is an online publication focused on space exploration, astronomy, skywatching and entertainment, with editorial teams based in the United States and United Kingdom. The website offers live coverage of space missions, astronomical discov ...
) {{DEFAULTSORT:Tensor-Vector-Scalar Gravity Theories of gravity Theoretical physics Astrophysics