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Solution of Dirac equation around a spinning black hole

✍ Scribed by Banibrata Mukhopadhyay; Sandip K. Chakrabarti


Book ID
117552931
Publisher
Elsevier Science
Year
2000
Tongue
English
Weight
224 KB
Volume
582
Category
Article
ISSN
0550-3213

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Nonexistence of time-periodic solutions
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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

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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 Ο• = 0. Likewise,