Gravitational waves from glitch-induced -mode oscillations in quark and neutron stars
OH Wilson, WCG Ho - Physical Review D, 2024 - APS
Matter in compact stars is dense enough that transient events within the star could have
sufficiently high energies to produce detectable gravitational waves (GWs). These GWs …
sufficiently high energies to produce detectable gravitational waves (GWs). These GWs …
Gravitational waves from glitch-induced f-mode oscillations in quark and neutron stars
OH Wilson, WCG Ho - arXiv preprint arXiv:2403.09489, 2024 - arxiv.org
Matter in compact stars is dense enough that transient events within the star could have
sufficiently high energies to produce detectable gravitational waves (GWs). These GWs …
sufficiently high energies to produce detectable gravitational waves (GWs). These GWs …
Gravitational waves from glitch-induced f-mode oscillations in quark and neutron stars
OH Wilson, WCG Ho - Physical Review D, 2024 - ui.adsabs.harvard.edu
Matter in compact stars is dense enough that transient events within the star could have
sufficiently high energies to produce detectable gravitational waves (GWs). These GWs …
sufficiently high energies to produce detectable gravitational waves (GWs). These GWs …
Gravitational waves from glitch-induced f-mode oscillations in quark and neutron stars
OH Wilson, WCG Ho - arXiv e-prints, 2024 - ui.adsabs.harvard.edu
Matter in compact stars is dense enough that transient events within the star could have
sufficiently high energies to produce detectable gravitational waves (GWs). These GWs …
sufficiently high energies to produce detectable gravitational waves (GWs). These GWs …