activity
20182026
most citedTwo-flavor color superconducting quark stars may not exist

13 citations · 35 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2026

Multiwavelength Analysis of PSR J0437-4715 with Pulse Profile Modeling

Liqiang Qi, Juan Zhang, Weiwei Xu +6

We present a multi-wavelength analysis of the nearby millisecond pulsar PSR J0437--4715, combining Hubble Space Telescope (HST) far-ultraviolet, ROSAT soft X-ray, and XMM-Newton X-…

astro-ph.HE2025

A Microphysical Probe of Neutron Star Interiors: Constraining the Equation of State with Glitch Dynamics

Zhonghao Tu, Ang Li

Glitches in neutron stars originate from the sudden transfer of angular momentum between superfluid components and the observable crust. By modeling this glitch dynamics--including…

astro-ph.HE2025

Timing results of 22 years for PSR J0922+0638

Peng Liu, Mingyang Wang, Jianping Yuan +4

We conducted a timing analysis of PSR J0922+0638 (B0919+06) using data from the Nanshan 26 m radio telescope and the MeerKAT telescope, spanning from January 2001 to March 2023. Du…

nucl-th2025

Unified QMF equation of state for neutron star matter: Static and dynamic properties

Zhonghao Tu, Xiangdong Sun, Shuochong Han +2

We construct a set of unified equations of state based on the quark mean field (QMF) model, calibrated to different values of nuclear symmetry energy slope at the saturation densit…

nucl-th2025★ 3 cited

Delayed Thermal Relaxation of Rapidly Cooling Neutron Stars: Nucleon Superfluidity and Non-nucleon Particles

Zhonghao Tu, Ang Li

The thermal relaxation time of neutron stars, typically defined by a sudden drop in surface temperature, is usually on the order of 10 to 100 years. In this study, we investigate n…

nucl-th2024★ 4 cited

Exploring nuclear force with pulsar glitch observation

Zhong-Hao Tu, Ang Li

We connect nuclear forces to one of the most notable irregular behaviors observed in pulsars, already detected in approximately 6\% known pulsars, with increasingly accurate data e…

astro-ph.HE2024★ 8 cited

Thermal x-ray studies of neutron stars and the equation of state

Zhiqiang Miao, Liqiang Qi, Juan Zhang +2

The understanding of neutron star equation of state hinges on a comprehensive analysis of multi-messenger, multi-wavelength data. The recent scrutiny of PSR J0030+0451 data by NICE…

astro-ph.HE2023★ 7 cited

On the spin period distribution of millisecond pulsars

Xiao-Jin Liu, Zhi-Qiang You, Zu-Cheng Chen +3

Spin period distribution provides important clues to understand the formation of millisecond pulsars (MSPs). To uncover the intrinsic period distribution, we analyze three samples…

nucl-th2023★ 13 cited

Two-flavor color superconducting quark stars may not exist

Wen-Li Yuan, Ang Li

Large uncertainties in the determinations of the equation of state of dense stellar matter allow the intriguing possibility that the bulk quark matter in beta equilibrium might be…

astro-ph.HE2018

Internal Plateau in Short GRBs and Quark Stars

A. Li

I summarize our recent calculations on quark stars (QSs), for the purpose of explaining some short gamma-ray bursts characterized by internal plateau in their early X-ray afterglow…