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A publicação pode ser exportada nos seguintes formatos: referência da APA (American Psychological Association), referência do IEEE (Institute of Electrical and Electronics Engineers), BibTeX e RIS.

Exportar Referência (APA) 
Costa, João L., Natário, J & Pedro F. C. Oliveira (2019). Cosmic no-hair in spherically symmetric black hole spacetimes. Annales Henri Poincaré. 20 (9), 3059-3090
Exportar Referência (IEEE) 
J. L. Costa et al.,  "Cosmic no-hair in spherically symmetric black hole spacetimes", in Annales Henri Poincaré, vol. 20, no. 9, pp. 3059-3090, 2019
Exportar BibTeX 
@article{costa2019_1714583700960,
	author = "Costa, João L. and Natário, J and Pedro F. C. Oliveira",
	title = "Cosmic no-hair in spherically symmetric black hole spacetimes",
	journal = "Annales Henri Poincaré",
	year = "2019",
	volume = "20",
	number = "9",
	doi = "10.1007/s00023-019-00825-z",
	pages = "3059-3090",
	url = "https://link.springer.com/article/10.1007%2Fs00023-019-00825-z"
}
Exportar RIS 
TY  - JOUR
TI  - Cosmic no-hair in spherically symmetric black hole spacetimes
T2  - Annales Henri Poincaré
VL  - 20
IS  - 9
AU  - Costa, João L.
AU  - Natário, J
AU  - Pedro F. C. Oliveira
PY  - 2019
SP  - 3059-3090
SN  - 1424-0637
DO  - 10.1007/s00023-019-00825-z
UR  - https://link.springer.com/article/10.1007%2Fs00023-019-00825-z
AB  - We analyze in detail the geometry and dynamics of the cosmological region arising in spherically symmetric black hole solutions of the Einstein–Maxwell-scalar field system with a positive cosmological constant. More precisely, we solve, for such a system, a characteristic initial value problem with data emulating a dynamic cosmological horizon. Our assumptions are fairly weak, in that we only assume that the data approach that of a subextremal Reissner–Nordström-de Sitter black hole, without imposing any rate of decay. We then show that the radius (of symmetry) blows up along any null ray parallel to the cosmological horizon (“near” i+), in such a way that r= + ∞ is, in an appropriate sense, a spacelike hypersurface. We also prove a version of the cosmic no-hair conjecture by showing that in the past of any causal curve reaching infinity both the metric and the Riemann curvature tensor asymptote to those of a de Sitter spacetime. Finally, we discuss conditions under which all the previous results can be globalized.
ER  -