Hestenes' Tetrad and Spin Connections

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

10.1007/s10773-005-4688-8

Defining a spin connection is necessary for formulating Dirac's bispinor equation in a curved space-time. Hestenes has shown that a bispinor field is equivalent to an orthonormal tetrad of vector fields together with a complex scalar field. In this paper, we show that using Hestenes' tetrad for the spin connection in a Riemannian space-time leads to a Yang-Mills formulation of the Dirac Lagrangian in which the bispinor field is mapped to a set of Yang-Mills gauge potentials and a complex scalar field. This result was previously proved for a Minkowski space-time using Fierz identities. As an application we derive several different non-Riemannian spin connections found in the literature directly from an arbitrary linear connection acting on Hestenes' tetrad and scalar fields. We also derive spin connections for which Dirac's bispinor equation is form invariant. Previous work has not considered form invariance of the Dirac equation as a criterion for defining a general spin connection.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Hestenes' Tetrad and Spin Connections does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Hestenes' Tetrad and Spin Connections, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hestenes' Tetrad and Spin Connections will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-126116

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.