activity
20092024
most citedRapid cooling of neutron star in Cassiopeia A and r-mode damping in the core

26 citations · 130 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2024★ 1 cited

Strange stars admixed with mirror dark matter: confronting observations of XTE J1814-338

Shu-Hua Yang, Chun-Mei Pi, Fridolin Weber

In this paper, we explore a novel framework for explaining the mass and radius relationships of observed neutron stars by considering strange stars (SSs) admixed with mirror dark m…

astro-ph.HE2024

Color-flavor locked strange stars admixed with mirror dark matter and the observations of compact stars

S. -H. Yang, C. -M. Pi

We investigate the structure and the tidal deformability of the color-flavor locked strange stars admixed with mirror dark matter. Assuming the stars in the GW170817 event have a m…

astro-ph.HE2023★ 1 cited

Confronting strange stars with compact-star observations and new physics

Shu-Hua Yang, Chun-Mei Pi, Xiao-Ping Zheng +1

Strange stars ought to exist in the universe according to the strange quark matter hypothesis, which states that matter made of roughly equal numbers of up, down, and strange quark…

astro-ph.HE2021★ 8 cited

Strange stars with a mirror-dark-matter core confronting with the observations of compact stars

Shu-Hua Yang, Chun-Mei Pi, Xiao-Ping Zheng

We investigate the structure and the tidal deformability of strange stars (SSs) with a mirror-dark-matter (MDM) core for the standard MIT bag model. We find that to explain the obs…

astro-ph.HE2021★ 20 cited

Constraints from compact star observations on non-Newtonian gravity in strange stars based on a density dependent quark mass model

Shu-Hua Yang, Chun-Mei Pi, Xiao-Ping Zheng +1

Using a density dependent quark mass (QMDD) model for strange quark matter, we investigate the effects of non-Newtonian gravity on the properties of strange stars and constrain the…

astro-ph.HE2019★ 22 cited

Non-Newtonian gravity in strange quark stars and constraints from the observations of PSR J0740+6620 and GW170817

Shu-Hua Yang, Chun-Mei PI, Xiao-Ping Zheng +1

We investigate the effects of non-Newtonian gravity on the properties of strange quark stars (QSs) and constrain the parameters of the standard MIT bag model used to describe stran…

astro-ph.HE2014★ 12 cited

R-mode instability of strange stars and observations of neutron stars in LMXBs

Chun-Mei PI, Shu-Hua Yang, Xiao-Ping Zheng

Using a realistic equation of state (EOS) of strange quark matter, namely, the modified bag model, and considering the constraints to the parameters of EOS by the observational mas…

astro-ph.HE2011★ 26 cited

Rapid cooling of neutron star in Cassiopeia A and r-mode damping in the core

Shu-Hua Yang, Chun-Mei Pi, Xiao-Ping Zheng

We proposed alternative explanation to the rapid cooling of neutron star in Cas A. It is suggested that the star is experiencing the recovery period following the r-mode heating pr…

astro-ph.HE2010★ 16 cited

The termination shock of a magnetar wind: a possible origin of gamma-ray burst X-ray afterglow emission

Z. Mao, Yun-Wei Yu, Z. G. Dai +2

Context: Swift observations suggest that the X-ray afterglow emission of some gamma-ray bursts (GRB) may have internal origins, and the conventional external shock (ES) cannot be t…

astro-ph.HE2010

Effects of rotochemical heating on the thermal evolution of superfluid neutron stars

Chun-Mei Pi

The authors take the rotochemical heating effect into account, which may make the cooling scenario different. Their model is consistent with the observation data.

astro-ph.HE2010

The extension of radiative viscosity to superfluid matter

Chun-Mei Pi, Shu-Hua Yang, Xiao-Ping Zheng

The radiative viscosity of superfluid matter is studied, and it is found that to the lowest order of the ratio of radiative viscosity to bulk viscosity is the same as…

astro-ph.HE2009★ 7 cited

Radiative viscosity of neutron stars

Shu-Hua Yang, Xiao-Ping Zheng, Chun-Mei Pi

We study non-linear effects of radiative viscosity of matter in neutron stars for both direct Urca process and modified Urca process, and find that non-linear effects will de…

astro-ph.HE2009★ 8 cited

The role of -mode damping in the thermal evolution of neutron stars

Shu-Hua Yang, Xiao-Ping Zheng, Chun-Mei Pi +1

The thermal evolution of neutron stars (NSs) is investigated by coupling with the evolution of -mode instability that is described by a second order model.The heating e…

astro-ph.HE2009★ 9 cited

Neutrino Emissivity of Non-equilibrium beta processes With Nucleon Superfluidity

Chun-Mei Pi, Xiao-Ping Zheng, Shu-Hua Yang

We investigate the influence of nucleon superfluidity on the neutrino emissivity of non-equilibrium beta processes. Calculations are performed of the reduction factors for direct a…