A conserved energy for axially symmetric Newman–Penrose–Maxwell scalars on Kerr black holes

DOI10.1098/RSPA.2018.0686zbMath1425.83027arXiv1806.09162OpenAlexW3105832748WikidataQ128627097 ScholiaQ128627097MaRDI QIDQ5243631

Nishanth Gudapati

Publication date: 19 November 2019

Published in: Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1806.09162

zbMATH Keywords

Maxwell's equationsKerr black holesstability of black holes

Mathematics Subject Classification ID

Black holes (83C57) Electromagnetic fields in general relativity and gravitational theory (83C50)

Related Items (4)

Price's law for spin fields on a Schwarzschild background ⋮ Sharp decay for Teukolsky equation in Kerr spacetimes ⋮ Sharp decay estimates for massless Dirac fields on a Schwarzschild background ⋮ Almost Price's law in Schwarzschild and decay estimates in Kerr for Maxwell field

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