activity
20222026
most citedOscillation Modes and Gravitational Waves from Strangeon Stars

25 citations · 54 across the 11 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2026

Continuous Gravitational Waves from Thermo-Elastic Mountains in Ultraluminous X-ray Pulsars

Hong-Bo Li, Ziming Wang, Lijing Shao +1

Fast-spinning, nonaxisymmetrically deformed neutron stars (NSs) are promising targets for continuous gravitational-wave (CGW) searches with current and next-generation ground-based…

astro-ph.HE2026

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…

astro-ph.HE2026

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…

hep-ph2025

U-spin symmetry energy and hyperon puzzle in -admixed neutron stars

Hao-Song You, Ting-Lan Yu, Sophia Han +2

By combining the (,) I-spin doublets or (,) U-spin doublets, the SU(3) flavor symmetry of light quarks can be decomposed into SU(2)U(1) or SU(2)…

astro-ph.HE2025

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…

astro-ph.HE2025

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…

hep-ph2025

Multibaryon states in the framework of an equivparticle model

Hao-Song You, Xinmei Zhu, Cheng-Jun Xia +2

Within the framework of an equivparticle model employing mean-field approximation, we investigate systematically the mass spectra of color-singlet -quark configurations with $N…

gr-qc2024★ 1 cited

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…

hep-ph2024

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…

hep-ph2024

Strangelets at finite temperature

Hao-Song You, Huai-Min Chen, Jian-Feng Xu +3

We study the properties of strangelets at finite temperature , employing an equivparticle model that incorporates both linear confinement and leading-order perturbative interact…

astro-ph.HE2023★ 7 cited

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…

hep-ph2023★ 4 cited

Strangelets at finite temperature: nucleon emission rates, interface and shell effects

Hao-Song You, Huai-Min Chen, Jian-Feng Xu +3

We investigate the properties of strangelets at finite temperature , where an equivparticle model is adopted with both the linear confinement and leading-order perturbative inte…

nucl-th2023★ 17 cited

Hybrid Strangeon Stars

Chen Zhang, Yong Gao, Cheng-Jun Xia +1

It was conjectured that the basic units of the ground state of bulk strong matter may be strange-clusters called strangeons, and they can form self-bound strangeon stars that are h…

gr-qc2022★ 25 cited

Oscillation Modes and Gravitational Waves from Strangeon Stars

Hong-Bo Li, Yong Gao, Lijing Shao +2

The strong interaction at low energy scales determines the equation of state (EOS) of supranuclear matters in neutron stars (NSs). It is conjectured that the bulk dense matter may…