A potential-based method constructs stationary, differentially rotating, non-barotropic neutron stars in general relativity, with dynamical evolutions supporting that they are equilibrium configurations.
Analytic construction of baroclinic tori by non-linear summation
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abstract
In this paper analytical method for constructing baroclinic flow is presented. Presented method allows the construction of baroclinic tori with significant vertical shear, which are stable by the Solberg--H{\o}iland criteria. The presented method can be useful in the investigations of the influence of background structure on vertical-shear- and entropy-driven instabilities.
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Rotating neutron stars with non-barotropic thermal profile
A potential-based method constructs stationary, differentially rotating, non-barotropic neutron stars in general relativity, with dynamical evolutions supporting that they are equilibrium configurations.