Abstract
It is shown that Rosen's bimetric theory of gravitation also has a Schwarzschild-type singularity. The radius of the singularity-the gravitational radius-is defined by the secondary massM1. Simultaneously it is shown that only those configurations are stable, which are located in the range of central densities corresponding to the increasing branch of theM1 =M1(ρc) curve.
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.
