On symplectic form for null boundary phase space
From MaRDI portal
Publication:2682418
DOI10.1007/s10714-022-02997-2OpenAlexW4308429946MaRDI QIDQ2682418
Publication date: 1 February 2023
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2209.05043
Related Items (3)
Hydro \& thermo dynamics at causal boundaries, examples in \(3d\) gravity ⋮ Topical collection: in memory of Professor T Padmanabhan ⋮ Null Raychaudhuri: canonical structure and the dressing time
Cites Work
- Unnamed Item
- T-Witts from the horizon
- Symmetries and charges of general relativity at null boundaries
- Extended symmetries at the black hole horizon
- A boundary term for the gravitational action with null boundaries
- Chiral massive news: null boundary symmetries in topologically massive gravity
- Null boundary phase space: slicings, news \& memory
- Extended corner symmetry, charge bracket and Einstein's equations
- Symmetries, charges and conservation laws at causal diamonds in general relativity
- Field theories with conformal Carrollian symmetry
- Entropy of a generic null surface from its associated Virasoro algebra
- Flat holography and Carrollian fluids
- Nonrelativistic particles and wave equations
- Symmetries at null boundaries: two and three dimensional gravity cases
- Conformal Carroll groups
- Covariant Galilean versus Carrollian hydrodynamics from relativistic fluids
- Residual diffeomorphisms and symplectic soft hairs: The need to refine strict statement of equivalence principle
- Black hole entropy is the Noether charge
- Conformal Carroll groups and BMS symmetry
- Black Hole Physics
- Embedding Galilean and Carrollian geometries. I. Gravitational waves
- Carrollian conservation laws and Ricci-flat gravity
- Carrollian physics at the black hole horizon
- Carroll symmetry of plane gravitational waves
- Carroll versus Newton and Galilei: two dual non-Einsteinian concepts of time
This page was built for publication: On symplectic form for null boundary phase space
