The Kerr spacetime in generalized Bondi–Sachs coordinates
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Publication:4467554
DOI10.1088/0264-9381/20/19/302zbMath1048.83014OpenAlexW1981268759MaRDI QIDQ4467554
A. W.-C. Lun, Steven J. Fletcher
Publication date: 10 June 2004
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1088/0264-9381/20/19/302
Related Items (16)
Peeling of Dirac field on Kerr spacetime ⋮ A note on the Newman-Unti group and the BMS charge algebra in terms of Newman-Penrose coefficients ⋮ Rotating black holes embedded in a cosmological background for scalar-tensor theories ⋮ Intermediate behavior of Kerr tails ⋮ Thermal Hawking radiation of black hole with supertranslation field ⋮ Characteristic evolution and matching ⋮ The Kerr–de Sitter spacetime in Bondi coordinates ⋮ BMS charge algebra ⋮ Characteristic evolution and matching ⋮ Peeling on Kerr spacetime: linear and semi-linear scalar fields ⋮ Gravitational memory effects and Bondi-Metzner-Sachs symmetries in scalar-tensor theories ⋮ A lower bound of the Trautman–Bondi energy ⋮ Dual gravitational charges and soft theorems ⋮ Characteristic evolution and matching ⋮ Kerr Black Holes in Horizon-Generating Form ⋮ Notes on self-dual gravity
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