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
โฆ LIBER โฆ
Erratum: Nonexistence of time-periodic solutions of the Dirac equation in an axisymmetric black hole geometry
โ 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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โฆ 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.
๐ SIMILAR VOLUMES
Nonexistence of time-periodic solutions
Nonexistence of time-periodic solutions of the Dirac equation in an axisymmetric black hole geometry
โ
Felix Finster; Niky Kamran; Joel Smoller; Shing-Tung Yau
๐
Article
๐
2000
๐
John Wiley and Sons
๐
English
โ 174 KB
๐ 1 views