General Relativistic Stability and Gravitational Wave Content of Rotating Triaxial Neutron Stars

General Relativistic Stability and Gravitational Wave Content of Rotating Triaxial Neutron Stars

Triaxial neutron stars can be sources of continuous gravitational radiation detectable by ground-based interferometers. The amplitude of the emitted gravitational wave can be greatly affected by the state of the hydrodynamical fluid flow inside the neutron star. In this work, we examine the most tri...

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Bibliographic Details
Main Authors: Yufeng Luo, Antonios Tsokaros, Roland Haas, Kōji Uryū
Format: Article
Language:English
Published: MDPI AG 2024-03-01
Series:Symmetry
Subjects:
neutron stars
stability
gravitational waves
Online Access:https://www.mdpi.com/2073-8994/16/3/343

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