Abstract

We construct the kinetic potentials that appear on the generalized Clebsch representation for the velocity field of a perfect fluid with a politropic state equation that describes the matter distribution in a Newtonian homogeneous isotropic universe. We also specify the constants of motion with respect to the HS group.

Full Text
Published version (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