Fetching the paper…
Reading the bibliography…
We provide a detailed analysis of quantum field theory around a collapsing shell and discuss several conceptual issues related to the emission of radiation flux and formation of black holes.
S Hawking, Nature
1975
Earlier work this paper cites.
D N Page, Phys. Rev
1976
Earlier work this paper cites.
P C W Davies, S A Fulling and W G Unruh, Phys. Rev
1976
Earlier work this paper cites.
W G Unruh, Phys. Rev
1976
Earlier work this paper cites.
N G Sanchez, Phys. Rev
1978
Earlier work this paper cites.
J M Bardeen, Phys. Rev. Lett
1981
Earlier work this paper cites.
J W York, Jr., Phys. Rev
1983
Earlier work this paper cites.
N D Birrell and P C W Davies, Quantum Fields in Curved Space
1984
Earlier work this paper cites.
K W Howard, Phys. Rev
1984
Cited alongside, same era.
T P Singh and T Padmanabhan, Ann. Phys
1988
Cited alongside, same era.
R Brout, S Massar, R Parentani and Ph Spindel, Phys. Rept
1995
Cited alongside, same era.
S Massar, Phys. Rev
1995
Cited alongside, same era.
R Brout, et al., Phys. Rev
1995
Cited alongside, same era.
G L Alberghi, R Casadio, G P Vacca and G Venturi, Phys. Rev
2001
Cited alongside, same era.
M Visser, Int. J. Mod. Phys
2003
Cited alongside, same era.
2005
Later among the works it cites.
T Vachaspati, D Stojkovic and L M Krauss, Phys. Rev
2007
Later among the works it cites.
2008
Later among the works it cites.
A B Nielsen and D-h Yeom, arXiv:0804.4435 (2008)
2008
Later among the works it cites.
C Barcelo, S Liberati, S Sonego and M Visser, Phys. Rev
2008
Later among the works it cites.
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…
For completeness, we also note that had we done the analysis with ϵ = 0 \epsilon=0 exactly, we would find that as u → ∞ u\to\infty , v ent ( V ) v_{\rm ent}(V) linearises around the “last escaper” ray (see Appendix A 1), and the contribution from the second term is suppressed like ∼ e − u / 2 M \sim e^{-u/2M} . In practice, since we can expect u ex ( u ent = 0 ) > 2 M u_{\rm ex}(u_{\rm ent}=0)>2M , the second term will remain highly suppressed at all times. The Hawking flux therefore arises entirely from the first term in Eqn. ( 30
Cited in the paper.
2008
Later among the works it cites.
B A Brown and J Lindesay, Class. Quant. Grav
2032
Closest in time.