activity
20022025
most citedRapid cooling of neutron star in Cassiopeia A and r-mode damping in the core

26 citations · 148 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.HE2025

XTE J1814-338 as a strange star admixed with bosonic dark matter

Shu-Hua Yang, Fridolin Weber

We show that the compact star XTE J1814-338 can be explained as a strange star admixed with self-interacting bosonic dark matter (BDM), provided the dark matter fraction exceeds ap…

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.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.HE2023★ 5 cited

Neutron star phase transition as the origin for the fast radio bursts and soft gamma-ray repeaters of SGR J1935+2154

Jun-Yi Shen, Yuan-Chuan Zou, Shu-Hua Yang +2

Magnetars are believed as neutron stars (NSs) with strong magnetic fields. X-ray flares and fast radio bursts (FRBs) have been observed from the magnetar (soft gamma-ray repeater,…

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…