activity
20242026
collaborators

7 papers

astro-ph.HE2026

Exploring Superfluid Angular Momentum Reservoir Effect on Pulsar Glitches and Forecasting Next Glitches of the Crab Pulsar

Pei-Xin Zhu, Xiao-Ping Zheng, Quan Cheng +2

Pulsar glitches are generally viewed as stochastic events driven by sudden angular momentum transfer from the neutron star's superfluid interior to its crust. Except two peculiar p…

astro-ph.HE2026

Superfluid Angular Momentum Reservoir Effect in Pulsar Glitches and Crab Pulsar Glitch Time Prediction

Pei-Xin Zhu, Xiao-Ping Zheng, Quan Cheng +2

Pulsar glitches are usually regarded as stochastic, independent events triggered by sudden angular momentum transfer from the neutron star's superfluid interior to its crust. Howev…

astro-ph.HE2025

Could the stochastic gravitational wave background from newborn magnetars be detected by the advanced LIGO and Einstein Telescope?

Yu-Long Yan, Quan Cheng, Xiao-Ping Zheng +1

Newborn magnetars are important gravitational wave sources due to their ultra-strong magnetic fields and fast spins, and the entire population in the Universe may significantly con…

astro-ph.HE2025

Revealing the internal magnetic field configuration of magnetars via their associated periodic signals

Jie Shu, Quan Cheng, Xiao-Ping Zheng

The magnetic deformation of magnetars is affected by their internal magnetic fields, which are generally difficult to be measured directly through observations. In this work, the p…

astro-ph.HE2024

Investigating the neutron star physics through observations of several young pulsars in the dipole-field re-emergence scenario

Yu-Long Yan, Quan Cheng, Xiao-Ping Zheng

The observed timing data, magnetic tilt angle , and age of young pulsars could be used to probe some important issues about neutron star (NS) physics, e.g., the NS internal mag…

astro-ph.HE2024

Constraints on the internal physics of neutron stars from the observational data of several young pulsars: the role of a power-law decaying dipole magnetic field

Yu-Long Yan, Quan Cheng, Xiao-Ping Zheng

The observational data (e.g., the timing data and magnetic tilt angles ) of young pulsars can be used to probe some critical issues about the internal physics of neutron stars…