activity
20242026
collaborators

6 papers

astro-ph.HE2026

Impact of Decay-Chain Feeding by Long-Lived Heavy Nuclei on Nuclear Cosmochronology

Qiu-Hong Chen, Meng-Hua Chen, Xianlin Yang +1

Nuclear cosmochronology provides an independent method for determining the ages of astrophysical objects without relying on Galactic chemical evolution models. Long-lived radioacti…

astro-ph.HE2026

MeV Gamma-Ray Lines from Radioactive Nuclei in Magnetar Giant Flares

Wu-Zimo Qiumu, Meng-Hua Chen, Qiu-Hong Chen +4

The rapid neutron-capture process (r-process) is widely regarded as the dominant mechanism responsible for the synthesis of heavy elements in the universe, yet its astrophysical si…

astro-ph.HE2026

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…

astro-ph.HE2025

Neutron Star-White Dwarf Merger as One Possible Optional Source of Kilonova-like Emission: Implications for GRB 211211A

Xiao-Xuan Liu, Hou-Jun Lü, Qiu-Hong Chen +2

Long-duration GRB 211211A, which lacked an associated supernova at such a low redshift , but was associated with a possible kilonova emission, has attracted great attentio…

astro-ph.HE2025

Kilonova Emission from Neutron Star Mergers with Different Equations of State

Wu-Zimo Qiumu, Meng-Hua Chen, Qiu-Hong Chen +1

Kilonova is an optical-infrared transient powered by the radioactive decay of heavy nuclei from binary neutron star mergers. Its observational characteristics depend on the mass an…

astro-ph.HE2024

Neutron Star Mergers as the Dominant Contributor to the Production of Heavy -Process Elements

Meng-Hua Chen, Li-Xin Li, Qiu-Hong Chen +2

The discovery of the radioactively powered kilonova AT2017gfo, associated with the short-duration gamma-ray burst GRB 170817A and the gravitational wave source GW170817, has provid…