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The Schwarzschild metric describes a static spherically symmetric mass distribution. But if a spinning star collapses into a black hole, its angular momentum is conserved. Black holes defined only by their mass and angular momentum are described by the Kerr metric which Kerr found in 1963.

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Kerr Metric and Detection of Two Kerr Black Holes

  • 章节

  • 发表日期：

    2026年

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  • Sebastian Boblest,
  • Thomas Müller,
  • Günter Wunner

摘要

The Schwarzschild metric describes a static spherically symmetric mass distribution. But if a spinning star collapses into a black hole, its angular momentum is conserved. Black holes defined only by their mass and angular momentum are described by the Kerr metric which Kerr found in 1963.