10 citations · 23 across the 10 of their papers we have counts for
12 papers
Tidal deformation and strain accumulation of solid compact stars
Hongxiang Shen, Yong Gao, Hong-Bo Li +1
The tidal deformability of compact stars encodes the equation of state of dense matter, and gravitational-wave observations such as GW170817 have begun to constrain it under the as…
Asteroseismology of neutron stars with both hyperons and resonances
Hao Sun, Jia-Xing Niu, Yong Gao +2
Employing various relativistic energy density functionals for nucleon-nucleon interactions, we investigate the impact of hyperons and resonances on the frequencies of non-radia…
Novae breves from magnetar giant flares: Potential probes of neutron star crusts
Jiahang Zhong, Qiu-Hong Chen, Yacheng Kang +4
Matter ejected from the magnetar crust during giant flares (GFs) may undergo -process nucleosynthesis, producing short-lived optical transients termed "novae breves". Although i…
Strangeon Ergostars
Haojia Xia, Shichuan Chen, Hong-Bo Li +2
The nature of the central engine powering short gamma-ray bursts (sGRBs) in binary neutron star (BNS) mergers remains a key open question in the era of multi-messenger astronomy. T…
Thermal Deformations in Super-Eddington Magnetized Neutron Stars: Implications for Continuous Gravitational-Wave Detectability
Hong-Bo Li, Yacheng Kang, Ren-Xin Xu
Rapidly rotating neutron stars (NSs) are promising targets for continuous gravitational-wave (CGW) searches with current and next-generation ground-based GW detectors. In this work…
Polar Mounds on Strangeon Stars: the Neutrino Emission from Ultraluminous X-ray Pulsars
Hong-Bo Li, Shi-Jie Gao, Xiang-Dong Li +1
Ultraluminous X-ray pulsars (ULXPs) serve as unique astrophysical laboratories, offering critical insights into accretion physics under extreme conditions, such as strong magnetic…
Lightcurve Features of Magnetar-Powered Superluminous Supernovae with Gravitational-Wave Emission and High-Energy Leakage
Jinghao Zhang, Yacheng Kang, Jiahang Zhong +4
Superluminous supernovae (SLSNe) are a distinct class of stellar explosions, exhibiting peak luminosities 10-100 times brighter than those of normal SNe. Their extreme luminosities…
Effects of inner crusts on -mode oscillations in neutron stars
Hao Sun, Jia-Xing Niu, Hong-Bo Li +4
In this work we investigate the influence of neutron stars' crusts on the non-radial -mode oscillations and examine their correlations with nuclear matter properties fixed by ad…
Continuous gravitational waves from thermal mountains on accreting neutron stars: effect of the nuclear pasta phase
Hong-Bo Li, Lijing Shao, Cheng-Jun Xia +1
As density increases, the shape of nuclei transitions to non-spherical ``nuclear pasta" structures. The physical properties of the nuclear pasta, such as thermal conductivity and e…
Effects from Dark Matter Halos on X-ray Pulsar Pulse Profiles
Yukun Liu, Hong-Bo Li, Yong Gao +2
Neutron stars (NSs) can capture dark matter (DM) particles because of their deep gravitational potential and high density. The accumulated DM can affect the properties of NSs. In t…
Compact dwarfs made of light-quark nuggets
Hao-Song You, Hao Sun, Hong-Bo Li +2
Utilizing an equivparticle model with both linear confinement and leading-order perturbative interactions, we obtain systematically the properties of strangelets and nonstrange qua…
Quasi-periodic oscillations during magnetar giant flares in the strangeon star model
Hong-Bo Li, Yacheng Kang, Zexin Hu +3
Soft gamma-ray repeaters (SGRs) are widely understood as slowly rotating isolated neutron stars. Their generally large spin-down rates, high magnetic fields, and strong outburst en…