Título

Helmholtz Theorems, Gauge Transformations, General Covariance and the Empirical Meaning of Gauge Conditions

Autor

Andrew Chubykalo

Nivel de Acceso

Acceso Abierto

Resumen o descripción

It is well known that the use of Helmholtz decomposition theorem for static vector fields C : R3 → R3 ,

when applied to the time dependent vector fields E : R4 → R3 , B : R4 → R3 which represent the

electromagnetic field, allows us to obtain instantaneous-like solutions all along R3 . For this reason,

some people thought (see e.g. [1] and references therein) that the Helmholtz theorem cannot

be applied to time dependent vector fields and some modification is wanted in order to get the retarded

solutions. However, the use of the Helmholtz theorem for static vector fields is correct even

for time dependent vector fields (see, e.g. [2]), so a relation between the solutions was required, in

such a way that a retarded solution can be transformed in an instantaneous one, and conversely.

On this paper we want to suggest, following most of the time the mathematical formalism of Woodside

in [3], that: 1) there are many Helmholtz decompositions, all equally consistent, 2) each one is

naturally related to a space-time structure, 3) when we use the Helmholtz decomposition for the

electromagnetic potentials it is equivalent to a gauge transformation, 4) there is a natural methodological

criterion for choosing the gauge according to the structure postulated for a global spacetime,

5) the Helmholtz decomposition is the manifestation at the level of the fields that a gauge is

involved. So, when we relate the retarded solution to the instantaneous one what we do is to change

the gauge and the space-time. And, if the Helmholtz decompositions are related to a space-time

structure, and are equivalent to gauge transformations, each gauge transformation is natural for a

specific space-time. In this way, a Helmholtz decomposition for Euclidean space is equivalent to

the Coulomb gauge and a Helmholtz decomposition for the Minkowski space is equivalent to the

Lorenz gauge. This leads us to consider that the theories defined by different gauges may be mathematically

equivalent, because they can be related by means of a gauge transformation, but they

are not empirically equivalent, because they have quite different observational consequences due

to the different space-time structure involved.

Producción Científica de la Universidad Autónoma de Zacatecas UAZ

Fecha de publicación

mayo de 2016

Tipo de publicación

Artículo

Recurso de información

Formato

application/pdf

Idioma

Inglés

Audiencia

Público en general

Repositorio Orígen

Repositorio Institucional Caxcán

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