Universal scaling between magnetar field and initial spin period for short gamma ray bursts

arXiv:2607.18698 · astro-ph.HE, hep-ph · Submitted 2026-07-21 · Read on arXiv

Qin-Mei Li, Qi-Bin Sun, Sheng-Bang Qian, Li-Yin Zhu, Fu-Xing Li, Si-Yuan Zhu, Ming Lian, Jing Li

astro-ph.HE, hep-ph

Submitted: 2026-07-21

Comments: 10 pages, 2 figures and 1 table

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Core — 4× in this paper · explained in 2 episodes
• Trace — 2× in this paper · explained in 2 episodes
• Diagnostic Tools — 1× in this paper · explained in 2 episodes
• Star Formation Rate (SFR) — 1× in this paper · explained in 5 episodes

Sources

• Magnetar Engines in Broad-lined Type Ic Supernovae and a Unified Picture for Magnetar-powered Stripped-envelope Supernovae

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