Abstract
The Einstein field equations for a perfect fluid distribution representing slowly-rotating fluid spheres are investigated. By imposing restrictions on the matter rotation ω(r, t) which is related to the dragging of inertial frames, and a uniform rotation which is a function of time, the general solutions for Ω(r, t) are obtained for all cosmological models. In the case of closed models the solutions for Ω(r, t) may represent realistic astrophysical situations only when the radial distance is greater than −1 and less than +1.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
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
