Energy and angular momentum of the weak gravitational waves on the Schwarzschild background. -- Quasilocal gauge-invariant formulation

DOI10.1023/A:1026786822107zbMath0952.83020arXivgr-qc/9801068MaRDI QIDQ1972106

Jacek Jezierski

Publication date: 18 January 2001

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9801068

zbMATH Keywords

Schwarzschild backgroundweak gravitational waves\((3+1)\)-decompositionRegge-Wheeler equationsZerilli equations

Mathematics Subject Classification ID

Black holes (83C57) Gravitational waves (83C35)

Related Items (9)

On the existence of rigid spheres in four-dimensional spacetime manifolds ⋮ Gauge invariant perturbations of the Schwarzschild spacetime ⋮ Gauge-invariant description of weak gravitational field on a spherically symmetric background with cosmological constant ⋮ Gauge-invariant quadratic approximation of quasi-local mass and its relation with Hamiltonian for gravitational field ⋮ The wave equation on the Schwarzschild metric II. Local decay for the spin-2 Regge–Wheeler equation ⋮ Conformal Yano-Killing tensors in Einstein spacetimes ⋮ Compatibility complex for black hole spacetimes ⋮ Morawetz estimate for linearized gravity in Schwarzschild ⋮ The linear stability of the Schwarzschild solution to gravitational perturbations in the generalised wave gauge

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