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The Vaidya solution describes the gravitational collapse of a finite shell of incoherent radiation falling into flat spacetime and giving rise to a Schwarzschild black hole.
P. C. Vaidya, The gravitational field of a radiating star
1951
Earlier work this paper cites.
P. C. Vaidya, ’Newtonian’ time in general relativity
1953
Earlier work this paper cites.
W. A. Hiscock, L. G. Williams and D. M. Eardley, Creation of particles by shell-focusing singularities
1982
Earlier work this paper cites.
A. Papapetrou, Formation of a singularity and causality
1985
Earlier work this paper cites.
D. M. Eardley, Black hole boundary conditions and coordinate conditions
1998
Cited alongside, same era.
B. Coll, S. R. Hildebrandt and J. M. M. Senovilla, Kerr-Schild symmetries
2001
Cited alongside, same era.
S. A. Hayward, Black holes: New horizons
2002
Cited alongside, same era.
A. Ashtekar and B. Krishnan, Isolated and dynamical horizons and their applications
2004
Cited alongside, same era.
I. Bengtsson and J. M. M. Senovilla, The boundary of the region with trapped surfaces in spherical symmetry
Cited in the paper.
I. Booth, Black hole boundaries
2005
Later among the works it cites.
E. Schnetter and B. Krishnan, Non-symmetric trapped surfaces in the Schwarzschild and Vaidya spacetimes
2006
Later among the works it cites.
I. Ben-Dov, Outer trapped surfaces in Vaidya spacetime
2007
Later among the works it cites.
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