Abstract

We describe the equation of motion of two charged spherical shells with tangential pressure in the field of a central Reissner–Nordstrom (RN) source. We solve the problem of determining the motion of the two shells after the intersection by solving the related Einstein–Maxwell equations and by imposing a physical continuity condition on the shells' velocities. In addition, we consider four applications: post-Newtonian and ultrarelativistic approximations, a test-shell case, and the ejection mechanism of one shell. This work is a direct generalization of Barkov–Belinski–Bisnovati–Kogan paper.

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 call

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.