2026-06-28T10:09:24Zhttps://docta.ucm.es/rest/oai/requestoai:docta.ucm.es:20.500.14352/594742023-08-25T15:52:56Zcom_20.500.14352_14col_20.500.14352_15
Docta Complutense
author
Fernández Jambrina, L.
author
Chinea Trujillo, Francisco Javier
2023-06-20T19:16:50Z
2023-06-20T19:16:50Z
1993-10-18
0031-9007
10.1103/PhysRevLett.71.2521
https://hdl.handle.net/20.500.14352/59474
http://prl.aps.org/pdf/PRL/v71/i16/p2521_1
http://journals.aps.org/
A method for interpreting discontinuities of the twist potential of vacuum stationary axisymmetric solutions of Einstein's equations is introduced. Surface densities for the angular momentum of the source can be constructed after solving a linear partial differential equation with boundary conditions at infinity. This formalism is applied to the Kerr metric, obtaining a regularized version of the density calculated with other formalisms. The main result is that the integral defining the total angular momentum is finite for the Kerr metric.
eng
Angular momentum surface density of the kerr metric
journal article
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File
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146571
application/pdf
Chinea06libre.pdf
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File
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a4ddac6f4d7be437a5704ad9cde80380
9634
text/plain
Chinea06libre.pdf.txt