collaborators

5 papers

astro-ph.HE2025

Fundamental modes of rotating neutron stars with various degrees of differential rotation in dynamical spacetimes

Anson Ka Long Yip, Patrick Chi-Kit Cheong, Tjonnie Guang Feng Li

Violent astrophysical events, including core-collapse supernovae and binary neutron star mergers, can result in rotating neutron stars with diverse degrees of differential rotation…

astro-ph.HE2025

Magnetic effects on fundamental modes in rotating neutron stars with a purely toroidal magnetic field

Anson Ka Long Yip, Tjonnie Guang Feng Li

Electromagnetic and gravitational-wave signals from neutron stars are shaped by rapid rotation and strong magnetic fields. Determining these properties is essential to interpret su…

astro-ph.HE2025

Gravitational wave signatures from the phase-transition-induced collapse of a magnetized neutron star

Anson Ka Long Yip, Patrick Chi-Kit Cheong, Tjonnie Guang Feng Li

Strong magnetic fields make neutron stars potential sources of detectable electromagnetic and gravitational-wave signals. Hence, inferring these magnetic fields is critical to unde…

astro-ph.HE2025

Impact of rotation on magnetic field stability and orientation in isolated neutron stars

Fabrizio Venturi Piñas, Anson Ka Long Yip, Patrick Chi-Kit Cheong +1

Neutron stars are the most compact horizonless objects in the Universe, exhibiting the strongest known magnetic fields. They are potential sources of coincident gravitational waves…

astro-ph.HE2025

General-relativistic resistive-magnetohydrodynamics simulations of self-consistent magnetized rotating neutron stars

Patrick Chi-Kit Cheong, Antonios Tsokaros, Milton Ruiz +4

We present the first general-relativistic resistive magnetohydrodynamics simulations of self-consistent, rotating neutron stars with mixed poloidal and toroidal magnetic fields. Sp…