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Updated: Dec 15, 2025

Setting Limits on Supersymmetry Using Simplified Models
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明るい二重中性子星の合併における非対称な質量比

R D Ferdman1, P C C Freire2, B B P Perera3

  • 1Faculty of Science, University of East Anglia, Norwich, UK. r.ferdman@uea.ac.uk.

Nature
|July 10, 2020
PubMed
まとめ

研究者達が発見した ダブルニュートロン星系は これまでに最も不対称で 結合しています PSR J1913+1102です この発見は,GW170817のような重力波の異常なキロノヴァの放出を 説明する可能性があることを示唆している.

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