Hamiltonian dynamics in the space of asymptotically Kerr-de Sitter spacetimes
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🌀 gr-qc
keywords
asymptoticallydynamicshamiltoniankerr-desitterspaceblack-holecalculated
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We determine all spacetime flows which lead to a Hamiltonian dynamics in the space of general relativistic initial data sets with asymptotically Kerr-de Sitter ends. The corresponding Hamiltonians are calculated. Some implications for black-hole thermodynamics are pointed out.
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Cited by 1 Pith paper
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Quantum-statistical constraints restrict the infinite family of KadS thermodynamic descriptions to a subclass that reduces to Schwarzschild-AdS and Kerr cases in appropriate limits, with uniqueness for co-rotating and...
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