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On 3+1 Lorentzian Einstein Manifolds with One Rotational Isometry

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arxiv 1703.06331 v1 pith:CWMHB4PK submitted 2017-03-18 gr-qc math.APmath.DG

classification gr-qcmath.APmath.DG
keywords einsteinequationslorentzianmanifoldsassumedconsidercoupledexplicit
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abstract

We consider 3+1 rotationally symmetric Lorentzian Einstein spacetime manifolds with $\Lambda >0$ and reduce the equations to 2+1 Einstein equations coupled to `shifted' wave maps. Subsequently, we prove various (explicit) positive mass-energy theorems. No smallness is assumed.

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Cited by 1 Pith paper

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  1. On Axially Symmetric Perturbations of Kerr Black Hole Spacetimes

    gr-qc 2025-07 conditional novelty 4.0 of 10

    For subextremal Kerr spacetimes, the paper constructs a positive-definite, conserved Hamiltonian energy for axially symmetric linear perturbations, indicating a form of linear stability within this symmetry class.

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