Kerr black hole

名词 n.

英文释义

名词 n.
  1. An uncharged (q = 0), rotating (L ≠ 0) black hole.
    — At the center of the Heleus Cluster is a black hole, a huge star that has collapsed into a region of space-time with gravitational effects so powerful that even light cannot escape. This example is believed to be a Kerr black hole approximately 12 stellar masses in size, and appears to have absorbed additional mass from nearby systems.

词形变化

词源

Named after New Zealander physicist Roy Kerr.
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