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Updated: Nov 25, 2025

Setting Limits on Supersymmetry Using Simplified Models
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Published on: November 15, 2013

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ニュートロン星状態方程式とハッブル定数に関するマルチメッセンジャー制約

Tim Dietrich1,2, Michael W Coughlin3, Peter T H Pang2,4

  • 1Institut für Physik und Astronomie, Universität Potsdam, 14476 Potsdam, Germany. tim.dietrich@uni-potsdam.de.

Science (New York, N.Y.)
|December 18, 2020
PubMed
まとめ

重力波と電磁気信号で観測された ニュートロン星の融合は 密度の高い物質と ハッブル定数を理解するのに役立ちます この研究は中性子星の半径を[公式:テキストを参照]kmとハッブル定数を[公式:テキストを参照]に制限した.

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