A review of total energy-momenta in GR with a positive cosmological constant
arXiv:1808.09265 · doi:10.1142/S0218271819300039
Abstract
A review is given of the various approaches to and expressions for total energy-momentum and mass in the presence of a positive cosmological constant in Einstein's field equations, together with a discussion of the key conceptual questions, main ideas and techniques behind them.
26 pages, nine figures and two references added
References in corpus (5)
- Initial boundary value problems for Einstein's field equations and geometric uniqueness
- Singular Yamabe metrics and initial data with exactly Kottler-Schwarzschild-de Sitter ends
- Positive mass theorems for asymptotically de Sitter spacetimes
- Asymptotically simple spacetimes and mass loss due to gravitational waves
- Penrose's quasi-local mass for asymptotically anti-de Sitter space-times
Cited by in corpus (14)
- The -BMS group of dS and new boundary conditions for AdS
- (A)dS in Bondi gauge
- Gravitational radiation condition at infinity with a positive cosmological constant
- Asymptotic Structure with a positive cosmological constant
- Energy of weak gravitational waves in spacetimes with a positive cosmological constant
- Covariant canonical formulations of classical field theories
- Conserved charges in asymptotically de Sitter spacetimes
- Asymptotics with a cosmological constant: The solution space
- Charges, conserved quantities and fluxes in de Sitter spacetime
- On the canonical energy of weak gravitational fields with a cosmological constant
- Degrees of freedom of gravitational radiation with positive cosmological constant
- Skew-symmetric endomorphisms in : A unified canonical form with applications to conformal geometry
- The Einstein metrics with smooth scri
- News tensor on null hypersurfaces