SPHEROIDAL AND TORSIONAL MODES OF QUASISTATIC SHEAR OSCILLATIONS IN THE SOLID GLOBE MODELS OF NUCLEAR PHYSICS AND PULSAR ASTROPHYSICS
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Publication:3500354
DOI10.1142/S0217751X07036634zbMath1200.85007arXiv0704.1732OpenAlexW3105508531MaRDI QIDQ3500354
Dima Podgainy, Irina Molodtsova, Serban Misicu, Sergey Bastrukov, Hsiang-Kuang Chang
Publication date: 3 June 2008
Published in: International Journal of Modern Physics A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/0704.1732
nonradial pulsations of neutron starsnuclear giant resonancesspheroidal and torsional modes of quasistatic shear vibrationsviscoelastic solid globe models
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On Hoyle-Narlikar-Wheeler mechanism of vibration energy powered magneto-dipole emission of neutron stars ⋮ RADIATIVE ACTIVITY OF MAGNETIC WHITE DWARF UNDERGOING LORENTZ-FORCE-DRIVEN TORSIONAL VIBRATIONS ⋮ SELF-GRAVITATING ASTROPHYSICAL MASS WITH SINGULAR CENTRAL DENSITY VIBRATING IN FUNDAMENTAL MODE ⋮ Alfvén node-free vibrations of white dwarf in the model of solid star with toroidal magnetic field ⋮ Frequency spectrum of toroidal Alfvén mode in a neutron star with Ferraro's form of nonhomogeneous poloidal magnetic field
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