Abstract
The authors exhibit the Lagrangian and Hamiltonian for the post-Newtonian N-body equations of motion in the non-symmetric gravitation theory. This Lagrangian may be deduced in the standard way from a straightforward generalisation of a variational principle and calculational procedure used in metric theories. This procedure also correctly reproduces the equations of motion for a test particle in a static spherically symmetric field.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: 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.
