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arxiv: gr-qc/0606064 · v2 · submitted 2006-06-14 · 🌀 gr-qc · hep-th

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Rigid upper bounds for the angular momentum and centre of mass of non-singular asymptotically anti-de Sitter space-times

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classification 🌀 gr-qc hep-th
keywords anti-decasemasssitterangularasymptoticallyboundscentre
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We prove upper bounds on angular momentum and centre of mass in terms of the Hamiltonian mass and cosmological constant for non-singular asymptotically anti-de Sitter initial data sets satisfying the dominant energy condition. We work in all space-dimensions larger than or equal to three, and allow a large class of asymptotic backgrounds, with spherical and non-spherical conformal infinities; in the latter case, a spin-structure compatibility condition is imposed. We give a large class of non-trivial examples saturating the inequality. We analyse exhaustively the borderline case in space-time dimension four: for spherical cross-sections of Scri, equality together with completeness occurs only in anti-de Sitter space-time. On the other hand, in the toroidal case, regular non-trivial initial data sets saturating the bound exist.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Positivity of holographic energy

    gr-qc 2026-04 unverdicted novelty 6.0

    Positivity of a weighted holographic energy is proven for 4D spacetimes with negative cosmological constant and conformally static boundaries of spherical or toroidal topology with compatible spin structure.

  2. Positivity of holographic energy

    gr-qc 2026-04 unverdicted novelty 5.0

    Positivity is proven for a weighted holographic energy in 4D asymptotically AdS spacetimes with conformally static boundaries of spherical or toroidal topology.