We construct a SU(2) connection formulation of Kerr isolated horizons. As in the non-rotating case, the model is based on a SU(2) Chern–Simons theory describing the degrees of freedom on the horizon. The presence of a non-vanishing angular momentum modifies the admissibility conditions for spin network states. Physical states of the system are in correspondence with open intertwiners with total spin matching the angular momentum of the spacetime. © 2014, Springer Science+Business Media New York.

Modelling black holes with angular momentum in loop quantum gravity

Pranzetti, Daniele;
2014-01-01

Abstract

We construct a SU(2) connection formulation of Kerr isolated horizons. As in the non-rotating case, the model is based on a SU(2) Chern–Simons theory describing the degrees of freedom on the horizon. The presence of a non-vanishing angular momentum modifies the admissibility conditions for spin network states. Physical states of the system are in correspondence with open intertwiners with total spin matching the angular momentum of the spacetime. © 2014, Springer Science+Business Media New York.
2014
46
12
1
16
https://arxiv.org/abs/1212.5166
http://inspirehep.net/record/1208284
https://zbmath.org/?t=&s=0&q=Modelling+black+holes+with+angular+momentum+in+loop+quantum+gravity
Frodden, E.; Perez, A.; Pranzetti, Daniele; Röken, D.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11767/33268
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