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Scalar–tensor–vector gravity (STVG) is a modified theory of
gravity In physics, gravity (), also known as gravitation or a gravitational interaction, is a fundamental interaction, a mutual attraction between all massive particles. On Earth, gravity takes a slightly different meaning: the observed force b ...
developed by John Moffat, a researcher at the Perimeter Institute for Theoretical Physics in
Waterloo, Ontario Waterloo is a city in the Canadian province of Ontario. It is one of three cities in the Regional Municipality of Waterloo (formerly Waterloo County, Ontario, Waterloo County). Waterloo is situated about west-southwest of Toronto, but it is n ...
. The theory is also often referred to by the acronym MOG (''MO''dified ''G''ravity).


Overview

Scalar–tensor–vector gravity theory, also known as MOdified Gravity (MOG), is based on an action principle and postulates the existence of a
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 ...
, while elevating the three constants of the theory to
scalar fields Scalar may refer to: *Scalar (mathematics), an element of a field, which is used to define a vector space, usually the field of real numbers *Scalar (physics), a physical quantity that can be described by a single element of a number field such a ...
. In the weak-field approximation, STVG produces a Yukawa-like modification of the gravitational force due to a point source. Intuitively, this result can be described as follows: far from a source gravity is stronger than the Newtonian prediction, but at shorter distances, it is counteracted by a repulsive
fifth force In physics, a fifth force refers to a hypothetical fundamental interaction (also known as fundamental force) beyond the four known interactions in nature: gravitational, electromagnetic, strong nuclear, and weak nuclear forces. Some speculativ ...
due to the vector field. STVG has been used successfully to explain galaxy rotation curves, the mass profiles of galaxy clusters, gravitational lensing in the Bullet Cluster, and cosmological observations without the need for
dark matter In astronomy, dark matter is an invisible and hypothetical form of matter that does not interact with light or other electromagnetic radiation. Dark matter is implied by gravity, gravitational effects that cannot be explained by general relat ...
. On a smaller scale, in the Solar System, STVG predicts no observable deviation from general relativity. The theory may also offer an explanation for the origin of
inertia Inertia is the natural tendency of objects in motion to stay in motion and objects at rest to stay at rest, unless a force causes the velocity to change. It is one of the fundamental principles in classical physics, and described by Isaac Newto ...
.


Mathematical details

STVG is formulated using the action principle. In the following discussion, a
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 ...
signature of ,-,-,-/math> will be used; the speed of light is set to c=1, and we are using the following definition for the
Ricci tensor In differential geometry, the Ricci curvature tensor, named after Gregorio Ricci-Curbastro, is a geometric object which is determined by a choice of Riemannian or pseudo-Riemannian metric on a manifold. It can be considered, broadly, as a measure ...
: :R_=\partial_\gamma\Gamma^\gamma_-\partial_\beta\Gamma^\gamma_+\Gamma^\gamma_\Gamma^\delta_-\Gamma^\gamma_\Gamma^\delta_. We begin with the Einstein–Hilbert Lagrangian: :_G=-\frac(R+2\Lambda)\sqrt, where R is the trace of the Ricci tensor, G is the gravitational constant, g is the determinant of the metric tensor g_, while \Lambda is the cosmological constant. We introduce the Maxwell-Proca Lagrangian for the STVG covector field \phi_\alpha: :\mathcal_\phi=-\frac\omega\left fracB^B_-\frac\mu^2\phi_\alpha\phi^\alpha+V_\phi(\phi)\rightsqrt, where B_=\partial_\alpha\phi_\beta-\partial_\beta\phi_\alpha = (\mathrm\phi)_ is the field strength of \phi_\alpha (given by the
exterior derivative On a differentiable manifold, the exterior derivative extends the concept of the differential of a function to differential forms of higher degree. The exterior derivative was first described in its current form by Élie Cartan in 1899. The re ...
), \mu is the mass of the vector field, \omega characterizes the strength of the coupling between the fifth force and matter, and V_\phi is a self-interaction potential. The three constants of the theory, G, \mu, and \omega, are promoted to scalar fields by introducing associated kinetic and potential terms in the Lagrangian density: :_S=-\frac\left fracg^\left(\frac+\frac-\partial_\alpha\omega\partial_\beta\omega\right)+\frac+\frac+V_\omega(\omega)\rightsqrt, where V_G, V_\mu, and V_\omega are the self-interaction potentials associated with the scalar fields. The STVG action integral takes the form :S=\int~\mathrm x, where _M is the ordinary matter Lagrangian density.


Spherically symmetric, static vacuum solution

The
field equations A classical field theory is a physical theory that predicts how one or more fields in physics interact with matter through field equations, without considering effects of quantization; theories that incorporate quantum mechanics are called qua ...
of STVG can be developed from the action integral using the
variational principle A variational principle is a mathematical procedure that renders a physical problem solvable by the calculus of variations, which concerns finding functions that optimize the values of quantities that depend on those functions. For example, the pr ...
. First a test particle Lagrangian is postulated in the form :_\mathrm=-m+\alpha\omega q_5\phi_\mu u^\mu, where m is the test particle mass, \alpha is a factor representing the nonlinearity of the theory, q_5 is the test particle's fifth-force charge, and u^\mu=dx^\mu/ds is its four-velocity. Assuming that the fifth-force charge is proportional to mass, i.e., q_5=\kappa m, the value of \kappa=\sqrt is determined and the following equation of motion is obtained in the spherically symmetric, static gravitational field of a point mass of mass M: :\ddot=-\frac\left +\alpha-\alpha(1+\mu r)e^\right where G_N 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. Further study of the field equations allows a determination of \alpha and \mu for a point gravitational source of mass M in the form :\mu=\frac, :\alpha=\frac\frac, where G_\infty\simeq 20G_N is determined from cosmological observations, while for the constants D and E galaxy rotation curves yield the following values: :D\simeq 25^2\cdot\,10 M_\odot^\mathrm^, :E\simeq 50^2\cdot\,10 M_\odot^, where M_\odot is the mass of the
Sun The Sun is the star at the centre of the Solar System. It is a massive, nearly perfect sphere of hot plasma, heated to incandescence by nuclear fusion reactions in its core, radiating the energy from its surface mainly as visible light a ...
. These results form the basis of a series of calculations that are used to confront the theory with observation.


Agreement with observations

STVG/MOG has been applied successfully to a range of astronomical, astrophysical, and cosmological phenomena. On the scale of the Solar System, the theory predicts no deviation from the results of Newton and Einstein. This is also true for star clusters containing no more than a few million solar masses. The theory accounts for the rotation curves of spiral galaxies, correctly reproducing the Tully–Fisher law. STVG is in good agreement with the mass profiles of galaxy clusters. STVG can also account for key cosmological observations, including: * The acoustic peaks in the
cosmic microwave background The cosmic microwave background (CMB, CMBR), or relic radiation, is microwave radiation that fills all space in the observable universe. With a standard optical telescope, the background space between stars and galaxies is almost completely dar ...
radiation; * The accelerating expansion of the universe that is apparent from
type Ia supernova A Type Ia supernova (read: "type one-A") is a type of supernova that occurs in binary systems (two stars orbiting one another) in which one of the stars is a white dwarf. The other star can be anything from a giant star to an even smaller white ...
observations; * The
matter power spectrum The matter power spectrum describes the density contrast of the universe (the difference between the local density and the mean density) as a function of scale. It is the Fourier transform of the matter correlation function. On large scales, ...
of the universe that is observed in the form of galaxy-galaxy correlations.


Problems and criticism

A 2017 article on Forbes by Ethan Siegel states that the Bullet Cluster still "proves dark matter exists, but not for the reason most physicists think". There he argues in favor of dark matter over non-local gravity theories, such as STVG/MOG. Observations show that in "undisturbed"
galaxy clusters A galaxy cluster, or a cluster of galaxies, is a structure that consists of anywhere from hundreds to thousands of galaxies that are bound together by gravity, with typical masses ranging from 1014 to 1015 solar masses. Clusters consist of galax ...
the reconstructed mass from
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 ...
is located where matter is distributed, and a separation of matter from gravitation only seems to appear after a collision or interaction has taken place. According to Ethan Siegel: "Adding dark matter makes this work, but non-local gravity would make differing before-and-after predictions that can't both match up, simultaneously, with what we observe."


See also

* 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 ...
* Tensor–vector–scalar gravity * '' Reinventing Gravity''


References

{{DEFAULTSORT:Scalar-Tensor-Vector Gravity Theories of gravity Astrophysics