Nonanalytic Relativistic <i>r</i>-Modes of Slowly Rotating Nonbarotropic Neutron Stars

We show that the <i>r</i>-modes of slowly rotating nonbarotropic neutron stars are described by nonanalytic functions of stellar angular velocity, which makes the perturbation techniques, used so far in the <i>r</i>-mode theoretical studies, inapplicable. In contrast to those...

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Bibliographic Details
Main Authors: Kirill Y. Kraav, Mikhail E. Gusakov, Elena M. Kantor
Format: Article
Language:English
Published: MDPI AG 2022-10-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/8/10/542