scholarly journals A 3+1 perspective on null hypersurfaces and isolated horizons

2006 ◽  
Vol 423 (4-5) ◽  
pp. 159-294 ◽  
Author(s):  
Eric Gourgoulhon ◽  
José Luis Jaramillo
2014 ◽  
Vol 2014 ◽  
pp. 1-10 ◽  
Author(s):  
K. L. Duggal

Totally geodesic null hypersurfaces have been widely used in the study of isolated black holes. In this paper, we introduce a new quasilocal notion of a family of totally umbilical null hypersurfaces called evolving null horizons (ENH) of a dynamical spacetime, satisfied under an appropriate energy condition. We focus on a variety of examples of ENHs and in some cases establish their relation with event and isolated horizons. We also present two specific physical models of an ENH in a black hole spacetime. Beside the examples, for further study we propose two open problems on possible general existence of an ENH in a black hole spacetime and its canonical or unique existence. The results of this paper have ample scope of working on totally umbilical null hypersurfaces of Lorentzian and, in general, semiRiemannian manifolds.


1992 ◽  
Vol 9 (5) ◽  
pp. 1309-1328 ◽  
Author(s):  
J N Goldberg ◽  
D C Robinson ◽  
C Soteriou

2006 ◽  
Vol 73 (8) ◽  
Author(s):  
Alejandro Corichi ◽  
Ulises Nucamendi ◽  
Marcelo Salgado

2000 ◽  
Vol 4 (1) ◽  
pp. 1-94 ◽  
Author(s):  
Abhay Ashtekar ◽  
John C. Baez ◽  
Kirill Krasnov

A method is described by means of which the characteristic initial value problem can be reduced to the Cauchy problem and examples are given of how it can be used in practice. As an application it is shown that the characteristic initial value problem for the Einstein equations in vacuum or with perfect fluid source is well posed when data are given on two transversely intersecting null hypersurfaces. A new discussion is given of the freely specifiable data for this problem.


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