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Updated: Jun 5, 2025

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超新星轴线在原始恒星的磁场中转化为马射线

Claudio Andrea Manzari1, Yujin Park1, Benjamin R Safdi1

  • 1Berkeley Center for Theoretical Physics, <a href="https://ror.org/01an7q238">University of California</a>, Berkeley, California 94720, USA and Theoretical Physics Group, <a href="https://ror.org/02jbv0t02">Lawrence Berkeley National Laboratory</a>, Berkeley, California 94720, USA.

Physical review letters
|December 6, 2024
PubMed
概括

超新星观测限制了轴向特性. 未来的马射线望远镜可以从超新星和中子星的合并中检测到轴子 (假设粒子),帮助暗物质研究.

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