Speaker
Mr
Samuel I. Santos
(ITA)
Description
The theory of classical Proca
elds in curved spacetimes without torsion is presented.
In particular, the wave equation for a Proca potential is deduced. A two-component
spinor version of the theory is subsequently exhibited on the basis of the use of certain
calculational techniques that are already available in the literature concerning the spinor
formalisms of Infeld and van der Waerden. Then, it will be shown that no couplings
between Proca
elds and photons coming from curvatures ultimately occur in the spinor
wave equations for the theory. However, the procedures for deriving such wave equations
produce a new coupling term which involves an Infeld-van der Waerden affine potential
and a Proca potential. Additionally, these procedures suggest the implementation of a
subsidiary condition that carries the covariant divergence of a Proca potential and the
skew part of a potential coupling term. One of the motivations for elaborating the work
comes from the absence from the literature of the theory to be described here. The present
work will hereby presumably
ll in the gap related to the absence from the literature of
any detailed formulation of the theory of Proca
elds in General Relativity.
Author
Mr
Samuel I. Santos
(ITA)
Co-author
Prof.
Jorge G. Cardoso
(UDESC)