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...
Main Authors: | , , |
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Format: | Article |
Language: | English |
Published: |
MDPI AG
2022-10-01
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Series: | Universe |
Subjects: | |
Online Access: | https://www.mdpi.com/2218-1997/8/10/542 |