scholarly journals TORSION AND THE ELECTROMAGNETIC FIELD

1999 ◽  
Vol 08 (02) ◽  
pp. 141-151 ◽  
Author(s):  
V. C. DE ANDRADE ◽  
J. G. PEREIRA
Keyword(s):  
General Relativity ◽  
Electromagnetic Field ◽  
Gauge Invariance ◽  
Energy Momentum Tensor ◽  
Momentum Tensor ◽  
Local Gauge ◽  
Local Gauge Invariance

In the framework of the teleparallel equivalent of general relativity, we study the dynamics of a gravitationally coupled electromagnetic field. It is shown that the electromagnetic field is able not only to couple to torsion, but also, through its energy–momentum tensor, produce torsion. Furthermore, it is shown that the coupling of the electromagnetic field with torsion preserves the local gauge invariance of Maxwell's theory.

A note on spinor form of Lovelock differential identity

2019 ◽  
Vol 16 (09) ◽  
pp. 1950145
Author(s):  
Vladimir N. Trishin
Keyword(s):  
General Relativity ◽  
Electromagnetic Field ◽  
Maxwell Equations ◽  
Energy Momentum Tensor ◽  
Momentum Tensor ◽  
Riemann Curvature ◽  
Riemann Curvature Tensor ◽  
Differential Identity ◽  
Spinor Form ◽  
Order Identity

The paper is devoted to 2-spinor calculus methods in general relativity. New spinor form of the Lovelock differential identity is suggested. This identity is second-order identity for the Riemann curvature tensor. We provide an example that our spinorial treatment of Lovelock identity is effective for the description of solutions of Einstein–Maxwell equations. It is shown that the covariant divergence of Lipkin’s zilch tensor for the free Maxwell field vanishes on the solutions of Einstein–Maxwell equations if and only if the energy–momentum tensor of the electromagnetic field is Weyl-compatible.

Hidden local gauge invariance in the one‐dimensional Hubbard model and its equivalent coupled spin model

1990 ◽  
Vol 31 (6) ◽  
pp. 1544-1550 ◽  
Author(s):  
Huan‐Qiang Zhou ◽  
Lin‐Jie Jiang ◽  
Ping‐Feng Wu
Keyword(s):  
Hubbard Model ◽  
Gauge Invariance ◽  
Spin Model ◽  
One Dimensional ◽  
Local Gauge ◽  
Local Gauge Invariance ◽  
The One

scholarly journals Local gauge invariance implies Siegert’s hypothesis

1997 ◽  
Vol 55 (3) ◽  
pp. 1580-1582 ◽  
Author(s):  
H. W. L. Naus
Keyword(s):  
Gauge Invariance ◽  
Local Gauge ◽  
Local Gauge Invariance

scholarly journals CANONICAL APPROACH TO 2D SUPERSYMMETRIC WZNW MODEL COUPLED TO SUPERGRAVITY

2002 ◽  
Vol 17 (29) ◽  
pp. 1923-1936 ◽  
Author(s):  
OLIVERA MIŠKOVIĆ ◽  
BRANISLAV SAZDOVIĆ
Keyword(s):  
Energy Momentum Tensor ◽  
Momentum Tensor ◽  
Moody Algebra ◽  
Gauge Transformations ◽  
Local Gauge ◽  
Gauge Symmetries ◽  
Wznw Model ◽  
Canonical Approach ◽  
Explicit Expressions

Starting from the known representation of the Kac–Moody algebra in terms of the coordinates and momenta, we extend it to the representation of the super Kac–Moody and super Virasoro algebras. Then we use general canonical method to construct an action invariant under local gauge symmetries, where components of the super energy–momentum tensor L± and G± play the role of the diffeomorphisms and supersymmetry generators respectively. We obtain covariant extension of WZNW theory with respect to local supersymmetry as well as explicit expressions for gauge transformations.

Local (Gauge) Invariance

1984 ◽  
pp. 26-37 ◽  
Author(s):  
Masud Chaichian ◽  
Nikolai F. Nelipa
Keyword(s):  
Gauge Invariance ◽  
Local Gauge ◽  
Local Gauge Invariance

Superfluid Flow and Local Gauge Invariance

1980 ◽  
Vol 48 (3) ◽  
pp. 793-798 ◽  
Author(s):  
Masakazu Ichiyanagi
Keyword(s):  
Gauge Invariance ◽  
Local Gauge ◽  
Superfluid Flow ◽  
Local Gauge Invariance

scholarly journals A regular scale-dependent black hole solution

2018 ◽  
Vol 27 (03) ◽  
pp. 1850032 ◽  
Author(s):  
Ernesto Contreras ◽  
Ángel Rincón ◽  
Benjamin Koch ◽  
Pedro Bargueño
Keyword(s):  
General Relativity ◽  
Black Hole ◽  
Black Hole Solution ◽  
Energy Momentum Tensor ◽  
Energy Condition ◽  
Momentum Tensor ◽  
Scale Dependence ◽  
Weak Energy Condition ◽  
Effective Energy ◽  
Regular Black Hole

In this work, we present a regular black hole solution, in the context of scale-dependent General Relativity, satisfying the weak energy condition. The source of this solution is an anisotropic effective energy–momentum tensor which appears when the scale dependence of the theory is turned-on. In this sense, the solution can be considered as a semiclassical extension of the Schwarzschild one.

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