Note on trapped surfaces in the Vaidya solution

DOI10.1103/PHYSREVD.79.024027zbMath1222.83090arXiv0809.2213WikidataQ62561520 ScholiaQ62561520MaRDI QIDQ3093681

Ingemar Bengtsson, José M. M. Senovilla

Publication date: 18 October 2011

Published in: Physical Review D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0809.2213

Mathematics Subject Classification ID

Black holes (83C57) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (7)

Shear-free dust solution in general covariant Hořava-Lifshitz gravity ⋮ Slowly evolving horizons in Einstein gravity and beyond ⋮ Black hole regions containing no trapped surfaces ⋮ INVOLUTE, MINIMAL, OUTER AND INCREASINGLY TRAPPED SURFACES ⋮ TRAPPED SURFACES ⋮ Vaidya solution in general covariant Hořava–Lifshitz gravity with the minimum coupling and without projectability: Infrared limit ⋮ Vaidya solutions in general covariant Hořava–Lifshitz gravity without projectability: Infrared limit

Cites Work

• Isolated and dynamical horizons and their applications
• ‘Newtonian’ Time in General Relativity
• Kerr-Schild symmetries

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