The Teleparallel Equivalent of General Relativity: Comparison
Please note this is a comparison between Version 3 by José Maluf and Version 2 by José Maluf.

The teleparallel equivalent of general relativity (TEGR) is an alternative geometrical formulation of the relativistic theory of gravitation. A brief description of the  TEGR is presented. The building blocks of the theory and few main achievements are discussed.

• Teleparallelism
• TEGR
• Gravitational Energy-Momentum
• f(T) theories

The teleparallel equivalent of general relativity (TEGR) is an alternative geometrical

formulation of Einstein's general relativity[1][2]. The TEGR is formulated in terms of

the tetrad field and of the corresponding torsion tensor, which is the antisymmetric

part of the Weitzenböck connection, in contrast with Einstein's formulation of general

relativity, which is constructed out of the metric tensor and of the Riemann-Christoffel

curvature tensor. The field equations for the tetrad field in the TEGR are completely

equivalent to Einstein's equations for the metric tensor. A theory constructed out of

the tetrad field, such as the TEGR, allows the establishment of third rank tensors

(the torsion tensor, for instance), and these tensors allow, in turn, the definitions

of vector densities and total divergences. These mathematical quantities are suitable

for the construction of surface integrals, that are eventually identified with the

energy, momentum and 4-angular momentum of the gravitational field. In the metric

formulation of general relativity it is not easy to establish non-trivial third rank

tensors that yield well defined total divergences of vector fields. Thus, in the TEGR

it is possible to define the energy-momentum and 4-angular momentum of the

gravitational field. Morever, the definitions of the latter quantities satisfy the algebra of

the Poincare group in the phase space of the theory[2][1]. In particular[1], in the TEGR it

is possible to establish the definition of the centre of mass moment of the gravitational

field. The gravitational centre of mass density is a quantity that describes the regions

in space where the gravitational field is more intense, i.e., where geodesic particles

acquire stronger gravitational accelerations, compared with the geodesic motion in the

flat space-time.

In the TEGR the concept of frame, determined by the tetrad fields, is of great importance.

Observers are adapted to frames in space-time, and the frames are subject to inertial

and gravitational accelerations, in general. Inertial accelerations are those that cause

the deviation of the motion of free particles, for instance, from the geodesic behaviour.

As an example, a static frame is subject to inertial accelerations.

In the geometrical framework of teleparallelism, it is possible to establish the notion

of distant parallelism. This feature justifies the name of the geometrical formulation.

In order to understand the distant parallelism, one has first to fix a particular frame.

In a space–time endowed with a set of tetrad fields, two vectors at distant points in

a particular frame are called parallel if they have identical components with respect

to the local tetrads at the points considered. It is possible to show[2]  that the

Weitzenböck connection plays a major role in the establishment of the condition of

absolute parallelism in space-time.

All physical features and results that one obtains in the context of Einstein's general

relativity are also described in the TEGR. The latter approach to the relativistic theory

of gravitation further allows the consideration of additional concepts and definitions,

specially regarding the energy-momentum and 4-angular momentum of the gravitational field.

Among these applications, we mention the evaluation of the gravitational energy contained

within the external event horizon of a Kerr black hole (see[2]  and references therein). More

recently, the definition of the gravitational centre of mass moment has been applied to the

analysis of (non-linear) plane-fronted gravitational waves[3] [3].

Teleparallel theories of gravity are also considered and applied in the investigation of

cosmological models[4]. The f(T) models of relativistic gravitation  may provide a theoretical

interpretation of the late-time universe acceleration, dispensing in this way the cosmological

constant, and may easily accommodate with the regular thermal expanding history, including

the radiation and cold dark matter dominated phases.

### References

1. J. W. Maluf; The Teleparallel Equivalent of General Relativity and the Gravitational Centre of Mass. Universe 2016, 2, 19, 10.3390/universe2030019.
2. J. W. Maluf; The teleparallel equivalent of general relativity. Annalen der Phyzik 2013, 525, 339, 10.1002/andp.201200272.
3. J. W. Maluf, J. F. da Rocha-Neto, S. C. Ulhoa and F. L. Carneiro; The work energy-relation for particles on geodesics in the pp-wave sapce-times. JCAP 2019, 2019, JCAP03(2019)028, 10.1088/1475-7516/2019/03/028.
4. Yi-Fu Cai; Salvatore Capozziello; Mariafelicia De Laurentis; Emmanuel N Saridakis; f(T) teleparallel gravity and cosmology. Reports on Progress in Physics 2016, 79, 106901, 10.1088/0034-4885/79/10/106901.
More