collaborators

5 papers

astro-ph.SR2026

Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae

Wenyu Xin, Ken'ichi Nomoto, Chun-Ming Yip +4

Recently discovered very metal-poor (VMP) star LAMOST J1010+2358 shows a peculiar abundance pattern that is remarkably well fit by a Pop III pair-instability supernova (PISN) of $\…

astro-ph.HE2026

The Impact of the New Fe Decay Rates on Fe and Al Nucleosynthesis in Massive Stars

Bingyang Tan, Wenyu Xin, Ruizheng Jiang +2

The diffuse -ray emission from short-lived radioactive Al and Fe provides a direct probe of ongoing nucleosynthesis in the Galaxy. However, theoretical models hav…

astro-ph.SR2026

Constraints on the CO and O+O Reaction Rates from Binary Black Holes Detected via Gravitational Wave Signals

Wenyu Xin, Xiaokun Hou, Xianfei Zhang +2

Gravitational-wave observations of binary black hole (BH) mergers provide a novel avenue for testing massive-star evolution and the resulting BH mass spectrum. Recent population an…

astro-ph.SR2025

Abundance Pattern Fitting with Bayesian Inference: Constraining First Stars' Properties and Their Explosion Mechanism with Extremely Metal-poor Stars

Ruizheng Jiang, Haining Li, Gang Zhao +2

The abundance patterns of extremely metal-poor stars preserve a fossil record of the Universe's earliest chemical enrichment by the supernova explosions from the evolution of first…

astro-ph.SR2025

The Impact of C()O Reaction on the Presupernova Evolution and Supernova Explodability of Massive Stars

Wenyu Xin, Ken'ichi Nomoto, Gang Zhao

Among the uncertainties of stellar evolution theory, we investigate how the C()O reaction rate affects the evolution of massive stars for the initial masses o…