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Joseph R Farah1,2, Logan J Prust3,4, D Andrew Howell5,6

  • 1Las Cumbres Observatory, Goleta, CA, USA. jfarah@lco.global.

Nature
|March 12, 2026
PubMed
概括

超发光超新星 (SLSNe-I) 是由磁星提供动力,观察到的光曲线凸起是由磁星周围的Lense-Thirring前行解释的. 这证实了SLSNe-I亮度的磁铁旋转下降模型,并为广义相对论提供了新的测试.

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