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¹Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
²Center for Gravitation and Cosmology, College of Physical Science and Technology, Yangzhou University, Yangzhou 225009, China
³Department of Physics and Illinois Center for Advanced Studies of the Universe, University of Illinois Urbana-Champaign, Urbana, Illinois 61801, USA
⁴Center of Gravitational Physics and Quantum Information, Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto, 606-8502, Japan

^*Contact author: yong.gao@aei.mpg.de

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Articles Citing

Nonradial oscillations of stratified neutron stars with solid crusts: Mode characterization and tidal resonances in coalescing binaries

Detecting Tidal Resonances in Binary Neutron Stars

Magnetorotational instabilities in solids: Application to neutron-star crusts

Rethinking resonance detectability during binary neutron star inspiral: Accurate mismatch computations for low-lying dynamical tides

Difference between quark stars and neutron stars in universal relations and their effect on gravitational waves

Dynamical tidal response of neutron stars as a probe of dense-matter properties

Spacetime quasinormal mode oscillations of anisotropic neutron stars

Relativistic mode sums for neutron-star tidal response

Universal relations with dynamical tides

Properties and microscopic structures of dense stellar matter in relativistic mean field models

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