Event Horizons  

In General > s.a. [black holes]; boundaries and holography in field theory; quantum spacetime; Rigidity; Trapped Surface.
$ Of a world-line: The past (future) event horizon is the boundary of the future (past) of the world-line.
$ Of a spacetime: The boundary of the past of +, = (I(+)) (the future event horizon is the boundary of the future of ); It is a global concept, defining from which points one can reach (null) infinity.
* Relationships: Its existence is equivalent to (+) being spacelike (> see de sitter spacetime).
* Properties: They are always null hypersurfaces; Their area always increases; They either coincide or are outside the apparent horizon (not true?).
* Remark: Being global properties, they are in general difficult to calculate, except when they can be shown to coincide with a Killing horizon or some other locally defined surface. [Defined by retarded time u = .]

Geometry and Topology > s.a. black holes; black-hole types [toroidal]; topology change [censorship]
@ Geometry: Chrusciel et al AHP(01)gq/00 [area], JGP(02)gq/00 [differentiability], CQG(06)gq/05 [no degenerate components].
@ Topology: Huang & Liang PLA(95) [torus]; Siino PRD(98)gq/97, PRD(99)gq/97.

References > s.a. black-hole phenomenology; gravitational thermodynamics.
@ And thermodynamics: Gibbons & Hawking PRD(77); Fulling & Ruijsenaars PRP(87); Davies CQG(87), CQG(88), AIHP(88), comment Raychaudhuri CQG(90); Jensen PRD(95) [stability]; Massar & Parentani NPB(00)gq/99; Padmanabhan IJMPD(04)gq [and gravity as elasticity]; Zhou et al PLB(07) [second law in accelerating universe]; > s.a. horizons.
@ Quantum effects: Hájícek PLB(86); Padmanabhan PLB(86); Sorkin in(96)gq/97 [wrinkling below threshold scale]; Chapline et al IJMPA(03)gq/00 [phase transition]; 't Hooft gq/04-in [and quantum information]; > s.a. quantum black holes.
@ Other properties: Bergamin et al CQG(06)ht/05 [physical-degree-of-freedom-to-gauge conversion].
@ Numerical methods: Libson et al PRD(96); > s.a. models in numerical general relativity.
@ Cosmological: Kaloper et al PLB(04) [observational implications].


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