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Erratum: Nonexistence of time-periodic solutions of the Dirac equation in an axisymmetric black hole geometry

โœ Scribed by Felix Finster; Niky Kamran; Joel Smoller; Shing-Tung Yau


Publisher
John Wiley and Sons
Year
2000
Tongue
English
Weight
9 KB
Volume
53
Category
Article
ISSN
0010-3640

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โœฆ Synopsis


The angular eigenvalue in equation (2.16) should not be an integer but a half odd integer. The reason is that the transformation V from the Dirac operator in the symmetric frame to the usual Dirac operator in polar coordinates given at the end of Section 2.1 has a change of sign at ฯ• = 0. Likewise, the transformation U in the appendix changes sign at ฯ• = 0. As a consequence, the two-spinor ฮฑ is continuous on S 2 , and our proof of the regularity of the angular part holds as is. All other arguments and all our results remain true without any changes.


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Nonexistence of time-periodic solutions
โœ Felix Finster; Niky Kamran; Joel Smoller; Shing-Tung Yau ๐Ÿ“‚ Article ๐Ÿ“… 2000 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 174 KB ๐Ÿ‘ 1 views

We prove that in the nonextreme Kerr-Newman black hole geometry, the Dirac equation has no normalizable, time-periodic solutions. A key tool is Chandrasekhar's separation of the Dirac equation in this geometry. A similar nonexistence theorem is established in a more general class of stationary, axis