Importance of perturbed gravitational potentials in differentially rotating Newtonian stars
Importance of perturbed gravitational potentials in differentially rotating Newtonian stars
It is usually believed that the Cowling approximation can give satisfactory solutions if the stars %are highly compressible have soft equations of state and/or if the strongly general relativistic stars are treated in the case of rigid rotation. Since, however, there have been no systematic studies about the accuracy of …