Non-analytic behavior of the relativistic r-modes in slowly rotating neutron stars

An inconsistency between the theoretical analysis and numerical calculations of the relativistic \(r\)-modes puzzles the neutron star community since the Kojima's finding of the continuous part in the \(r\)-mode oscillation spectrum in 1997. In this paper, after a brief review of the Newtonian...

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Veröffentlicht in:	arXiv.org 2021-12
Hauptverfasser:	Kraav, Kirill Y, Gusakov, Mikhail E, Kantor, Elena M
Format:	Artikel
Sprache:	eng
Schlagworte:	Angular velocity Asymptotic properties Cowlings Eigenvectors Frequency ranges Inertial reference systems Mathematical analysis Neutron stars Neutrons Physics - General Relativity and Quantum Cosmology Physics - High Energy Astrophysical Phenomena Relativistic effects Resonant frequencies Stellar rotation
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