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Schwarze Löcher

In: Geometrie der Raumzeit

Author

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  • Rainer Oloff

Abstract

Zusammenfassung Schon im zehnten Kapitel haben wir Geodäten in der Schwarzschild-Raumzeit untersucht. In diesem Kapitel stellen wir uns auf den Standpunkt, daß die gesamte Masse des diese Raumzeit erzeugenden Fixsterns bei r = 0 konzentriert ist. Damit rückt der Bereich mit dem Schwarzschild-Radius r nahe dem kritischen Wert 2μ und darunter in das Zentrum des Interesses. Diese Zahl 2μ wird oft Schwarzschild-Radius (des Fixsterns) genannt. Da wir hier diesen Namen aber schon für die radiale Koordinate reserviert haben, nennen wir diese Zahl Schwarzschild-Horizont.

Suggested Citation

  • Rainer Oloff, 1999. "Schwarze Löcher," Springer Books, in: Geometrie der Raumzeit, chapter 14, pages 189-201, Springer.
  • Handle: RePEc:spr:sprchp:978-3-663-07654-4_15
    DOI: 10.1007/978-3-663-07654-4_15
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