Abstract
Formulates an exact form of the virial theorem for a relativistic charged thermodynamic perfect fluid in curved spacetime in time-orthogonal coordinates and diagonal metric tensor. Its Newtonian limit leads to a generalisation of Chandrasekhar's tensor virial theorem in hydromagnetics. The author applies the exact form of the virial theorem in curved spacetime, to obtain equilibrium configurations in two cases.
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.
