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I want to find out about the Vaidya thing, since it occurs in both papers it may be a significant detail
well here are the two leads I found in Bojowald et al references:
http://arxiv.org/gr-qc/9804075
Initial data and the end state of spherically symmetric gravitational collapse
P. S. Joshi, I. H. Dwivedi
31 pages no figures
Class.Quant.Grav. 16 (1999) 41-59
"Generalizing earlier results on the initial data and the final fate of dust collapse, we study here the relevance of the initial state of a spherically symmetric matter cloud towards determining its end state in the course of a continuing gravitational collapse. It is shown that given an arbitrary regular distribution of matter at the initial epoch, there always exists an evolution from this initial data which would result either in a black hole or a naked singularity depending on the allowed choice of free functions available in the solution. It follows that given any initial density and pressure profiles for the cloud, there is a non-zero measure set of configurations leading either to black holes or naked singularities, subject to the usual energy conditions ensuring the positivity of energy density. We also characterize here wide new families of black hole solutions resulting from spherically symmetric collapse without requiring the cosmic censorship assumption."
http://arxiv.org/gr-qc/9803038
Generalized Vaidya Solutions
Anzhong Wang, Yumei Wu
Gen. Relativ. Grav. 31 (1), 107-114 (1999)
"A large family of solutions, representing, in general, spherically symmetric Type II fluid, is presented, which includes most of the known solutions to the Einstein field equations, such as, the monopole-de Sitter-charged Vaidya ones."
MY COMMENT: so far it doesn't look like anything special. just some people assembling a large variety of solutions to the Einstein equation which are cases of black hole gravitational collapse. It turns out that some of the solutions give rise to naked singularities, like black holes but not shrouded in an event horizon---very hard for me to imagine---but the main value seems to be that this work gives lots of different readymade cases of matter collapsing down to a classical singularity. Something that LQG can then work on and investigate removing the singularity in these various cases.
Here is from Wang and Wu (great co-author names, Wang and Wu)
"In 1951, Vaidya[1] found a solution that represents an imploding (exploding) null dust fluid with spherical symmetry.
Sincethen, the solution has been intensively studied in gravitational collapse[2]. In particular, Papapetrou[3] first showed that this solution can give rise to the formation of naked singularities, and thus provides one of the earlier counterexamples to the cosmic censorship conjecture[4]."
...
the way it looks to me right now there are two representative papers about removing the BH singularity continuing into a BB expansion
and these two are recent (March and April 2005) and by Bojowald-Goswami-Maartens-Singh on the one hand and a less-well-known young researcher named Modesto on the other (but Modesto is at marseille with Rovelli)
and both of these recent papers mention ideas of Vaidya, some possible links are
http://arxiv.org/gr-qc/9804075
http://arxiv.org/gr-qc/9803038
these are not papers by Vaidya but they may clarify things a bit so I am going to have a look.
...
like for example in Bojowald et al on page 3 around equation (19) one sees
"a generalized Vaidya region" and "the usual Vaidya mass"
...
well here are the two leads I found in Bojowald et al references:
http://arxiv.org/gr-qc/9804075
Initial data and the end state of spherically symmetric gravitational collapse
P. S. Joshi, I. H. Dwivedi
31 pages no figures
Class.Quant.Grav. 16 (1999) 41-59
"Generalizing earlier results on the initial data and the final fate of dust collapse, we study here the relevance of the initial state of a spherically symmetric matter cloud towards determining its end state in the course of a continuing gravitational collapse. It is shown that given an arbitrary regular distribution of matter at the initial epoch, there always exists an evolution from this initial data which would result either in a black hole or a naked singularity depending on the allowed choice of free functions available in the solution. It follows that given any initial density and pressure profiles for the cloud, there is a non-zero measure set of configurations leading either to black holes or naked singularities, subject to the usual energy conditions ensuring the positivity of energy density. We also characterize here wide new families of black hole solutions resulting from spherically symmetric collapse without requiring the cosmic censorship assumption."
http://arxiv.org/gr-qc/9803038
Generalized Vaidya Solutions
Anzhong Wang, Yumei Wu
Gen. Relativ. Grav. 31 (1), 107-114 (1999)
"A large family of solutions, representing, in general, spherically symmetric Type II fluid, is presented, which includes most of the known solutions to the Einstein field equations, such as, the monopole-de Sitter-charged Vaidya ones."
MY COMMENT: so far it doesn't look like anything special. just some people assembling a large variety of solutions to the Einstein equation which are cases of black hole gravitational collapse. It turns out that some of the solutions give rise to naked singularities, like black holes but not shrouded in an event horizon---very hard for me to imagine---but the main value seems to be that this work gives lots of different readymade cases of matter collapsing down to a classical singularity. Something that LQG can then work on and investigate removing the singularity in these various cases.
Here is from Wang and Wu (great co-author names, Wang and Wu)
"In 1951, Vaidya[1] found a solution that represents an imploding (exploding) null dust fluid with spherical symmetry.
Sincethen, the solution has been intensively studied in gravitational collapse[2]. In particular, Papapetrou[3] first showed that this solution can give rise to the formation of naked singularities, and thus provides one of the earlier counterexamples to the cosmic censorship conjecture[4]."
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