A conserved current for perturbations of Einstein-Maxwell space-times
From MaRDI portal
Publication:3485568
DOI10.1098/rspa.1990.0080zbMath0705.53038OpenAlexW2079083752MaRDI QIDQ3485568
Gregory A. Burnett, Robert M. Wald
Publication date: 1990
Published in: Proceedings of the Royal Society of London. Series A: Mathematical and Physical Sciences (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1098/rspa.1990.0080
Applications of local differential geometry to the sciences (53B50) Einstein-Maxwell equations (83C22)
Related Items (19)
Gauge-invariant observables, gravitational dressings, and holography in AdS ⋮ The holographic shape of entanglement and Einstein's equations ⋮ The Wald–Zoupas prescription for asymptotic charges at null infinity in general relativity ⋮ Stability of black holes and black branes ⋮ A gauge-invariant symplectic potential for tetrad general relativity ⋮ General definition of “conserved quantities” in general relativity and other theories of gravity ⋮ Boundary effects in general relativity with tetrad variables ⋮ Gravitational edge modes, coadjoint orbits, and hydrodynamics ⋮ Adjoint operators and perturbation theory of black holes ⋮ Conserved currents for electromagnetic fields in the Kerr spacetime ⋮ A class of conserved currents for linearized gravity in the Kerr spacetime ⋮ Anomalies in gravitational charge algebras of null boundaries and black hole entropy ⋮ Self-adjoint operators and conserved currents ⋮ SYMMETRIES ASSOCIATED WITH SYMPLECTIC CURRENTS ⋮ Brown-York charges at null boundaries ⋮ A conserved current for the field perturbations in the Einstein–Yang–Mills-dilaton–axion theory ⋮ The Hamiltonian dynamics of bounded spacetime and black hole entropy: the canonical method ⋮ Covariant canonical formalism for four-dimensional BF theory ⋮ Dark matter influence on black objects thermodynamics
This page was built for publication: A conserved current for perturbations of Einstein-Maxwell space-times