An infinite-dimensional family of black-hole microstate geometries
✍ Scribed by Iosif Bena; Nikolay Bobev; Stefano Giusto; Clément Ruef; Nicholas P. Warner
- Publisher
- Springer-Verlag
- Year
- 2011
- Tongue
- English
- Weight
- 584 KB
- Volume
- 2011
- Category
- Article
- ISSN
- 1126-6708
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📜 SIMILAR VOLUMES
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
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 ϕ = 0. Likewise,