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astro-ph.HE2026
A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap
Tian Huang, Xizhen Lu, Guoliang Lü +8
Observations of binary black hole (BBH) mergers detected by LIGO -- such as GW170729, GW190620, GW190706, GW230107, GW230820, and GW230928 -- feature high effective spins and prima…
astro-ph.SR2026
Mass distribution of neutron stars in binary systems
Zhe Hu, GuoLiang Lv, ChunHua Zhu +5
It is known that the mass distribution of the known neutron stars (NSs) exhibits a bimodal pattern. The origin of this distribution remains a subject of debate. We constructed a su…
astro-ph.SR2026
Evolution of cataclysmic variables under different magnetic braking prescriptions
Bingyao Zhou, Chunhua Zhu, Guoliang Lü +3
Context. The evolution of cataclysmic variables (CVs) - interacting binaries where a low-mass donor transfers matter to a white dwarf via an accretion disk - is critically controll…