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Boundary charges in gauge theories: using Stokes theorem in the bulk

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arxiv hep-th/0301039 v3 pith:OGH4A2KA submitted 2003-01-07 hep-th gr-qc

Boundary charges in gauge theories: using Stokes theorem in the bulk

classification hep-th gr-qc
keywords formsboundarytheoryasymptoticallybackgroundbulkchargesconserved
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Boundary charges in gauge theories (like the ADM mass in general relativity) can be understood as integrals of linear conserved n-2 forms of the free theory obtained by linearization around the background. These forms are associated one-to-one to reducibility parameters of this background (like the time-like Killing vector of Minkowski space-time). In this paper, closed n-2 forms in the full interacting theory are constructed in terms of a one parameter family of solutions to the full equations of motion that admits a reducibility parameter. These forms thus allow one to apply Stokes theorem without bulk contributions and, provided appropriate fall-off conditions are satisfied, they reduce asymptotically near the boundary to the conserved n-2 forms of the linearized theory. As an application, the first law of black hole mechanics in asymptotically anti-de Sitter space-times is derived.

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Cited by 2 Pith papers

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    Explicit quasi-local formulae for celestial higher-spin charges and multipoles are given on finite 2-surfaces using higher-valence twistor solutions, with a phase-space derivation from self-dual gravity.

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    A consistent thermodynamics of the Kerr-Bertotti-Robinson black hole is constructed by adopting the Christodoulou-Ruffini mass relation, yielding a first law and Smarr formula without an explicit magnetic-field work term.