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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 M at distance r from the source can be written as :a = -\frac, where G 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 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 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 :=-\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 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 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 of the TeVeS theory and that predicted and measured by the
Gravity Probe B Gravity Probe B (GP-B) was a satellite-based experiment whose objective was to test two previously-unverified predictions of general relativity: the geodetic effect and frame-dragging. This was to be accomplished by measuring, very precisely, t ...
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 Astronomical interferometer, 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, wh ...
leads to K=-30 + \frac. So the coupling constants read: :K= 3(\pm\sqrt-5), \qquad k = 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 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 ...
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 2 eV)
neutrino A neutrino ( ; denoted by the Greek letter ) is an elementary particle that interacts via the weak interaction and gravity. The neutrino is so named because it is electrically neutral and because its rest mass is so small ('' -ino'') that i ...
s. 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 General relativity, also known as the general theory of relativity, and as Einstein's theory of gravity, is the differential geometry, geometric theory of gravitation published by Albert Einstein in 1915 and is the current description of grav ...
(GR) on large scales (a hundred billion times the size of the
Solar System The Solar SystemCapitalization of the name varies. The International Astronomical Union, the authoritative body regarding astronomical nomenclature, specifies capitalizing the names of all individual astronomical objects but uses mixed "Sola ...
) for the first time has been measured with data from the
Sloan Digital Sky Survey The Sloan Digital Sky Survey or SDSS is a major multi-spectral imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States. The project began in 2000 a ...
to be E_G=0.392\pm (~16%) consistent with GR, GR plus
Lambda CDM The Lambda-CDM, Lambda cold dark matter, or ΛCDM model is a mathematical model of the Big Bang theory with three major components: # a cosmological constant, denoted by lambda (Λ), associated with dark energy; # the postulated cold dark matte ...
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 Gauge ( ) may refer to: Measurement * Gauge (instrument), any of a variety of measuring instruments * Gauge (firearms) * Wire gauge, a measure of the size of a wire ** American wire gauge, a common measure of nonferrous wire diameter, especia ...
* Modified Newtonian dynamics *
Nonsymmetric gravitational theory In theoretical physics, the nonsymmetric gravitational theory (NGT) of John Moffat is a classical theory of gravitation that tries to explain the observation of the flat rotation curves of galaxies. In general relativity, the gravitational fiel ...
* 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 outer space, space exploration, astronomy, skywatching and entertainment, with editorial teams based in the United States and United Kingdom. Launched on July 20, 1999, the website offers live coverag ...
) {{DEFAULTSORT:Tensor-Vector-Scalar Gravity Theories of gravity Astrophysics