A class of new perturbation equations for the Kerr geometry

書誌事項

公開日
1982-04
権利情報
  • https://www.elsevier.com/tdm/userlicense/1.0/
DOI
  • 10.1016/0375-9601(82)90507-2
公開者
Elsevier BV

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説明

Abstract A class of new inhomogeneous equations governing gravitational perturbations of the Kerr geometry is presented. It is shown that, contrary to the case of the Teukolsky equation, these new equations are of short-range nature and exhibit no divergence difficulty associated with the source term.

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