@Article{CiCP-22-863,
author = {Federico Cipolletta, Christian Cherubini, Simonetta Filippi, Jorge A. Rueda and Remo Ruffini},
title = {Equilibrium Configurations of Classical Polytropic Stars with a Multi-Parametric Differential Rotation Law: A Numerical Analysis},
journal = {Communications in Computational Physics},
year = {2017},
volume = {22},
number = {3},
pages = {863--888},
abstract = {<p style="text-align: justify;">In this paper we analyze in detail the equilibrium configurations of classical
polytropic stars with a multi-parametric differential rotation law of the literature using
the standard numerical method introduced by Eriguchi and Mueller. Specifically we
numerically investigate the parameters&#39; space associated with the velocity field characterizing
both equilibrium and non-equilibrium configurations for which the stability
condition is violated or the mass-shedding criterion is verified.</p>},
issn = {1991-7120},
doi = {https://doi.org/10.4208/cicp.OA-2017-0007},
url = {http://global-sci.org/intro/article_detail/cicp/9985.html}
}