Abstract
A null fluid with radial “pressure” is proposed as a source generating Vaidya spacetime. The fluid is anisotropic with no transversal pressures and p = ρ/3 as its equation of state, where p is the isotropic pressure and ρ is the energy density. The radial energy flux is directed inward when \(\dot{m} > 0\) and the total energy flow crossing a surface of constant r resembles the Brown–York quasilocal energy (QLE). A modified Vaidya metric removes the singularity at the origin, and the corresponding QLE is investigated in terms of both r and the mass m(v) of the object.
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.