Abstract
An approach to classical neutrino fields in Einstein-Cartan theory is described using a generalised method of spin-coefficients, and some corrections to a previous paper are pointed out. It is also pointed out that this approach is particularly suitable for the generation of new exact solutions from known solutions in general relativity, and an example is given.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.