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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) 
Aniceto, P., Pani, P. & Rocha, J. V. (2016). Radiating black holes in Einstein-Maxwell-dilaton theory and cosmic censorship violation. Journal of High Energy Physics.
Exportar Referência (IEEE) 
A. P. et al.,  "Radiating black holes in Einstein-Maxwell-dilaton theory and cosmic censorship violation", in Journal of High Energy Physics, 2016
Exportar BibTeX 
@article{p.2016_1715088970823,
	author = "Aniceto, P. and Pani, P. and Rocha, J. V.",
	title = "Radiating black holes in Einstein-Maxwell-dilaton theory and cosmic censorship violation",
	journal = "Journal of High Energy Physics",
	year = "2016",
	volume = "",
	number = "",
	doi = "10.1007/JHEP05(2016)115"
}
Exportar RIS 
TY  - JOUR
TI  - Radiating black holes in Einstein-Maxwell-dilaton theory and cosmic censorship violation
T2  - Journal of High Energy Physics
AU  - Aniceto, P.
AU  - Pani, P.
AU  - Rocha, J. V.
PY  - 2016
SN  - 1126-6708
DO  - 10.1007/JHEP05(2016)115
AB  - We construct exact, time-dependent, black hole solutions of Einstein-Maxwell-dilaton theory with arbitrary dilaton coupling, a. For a = 1 this theory arises as the four-dimensional low-energy effective description of heterotic string theory. These solutions represent electrically charged, spherically symmetric black holes emitting or absorbing charged null fluids and generalize the Vaidya and Bonnor-Vaidya solutions of general relativity and of Einstein-Maxwell theory, respectively. The a = 1 case stands out as special, in the sense that it is the only choice of the coupling that allows for a time-dependent dilaton field in this class of solutions. As a by-product, when a = 1 we show that an electrically charged black hole in this theory can be overcharged by bombarding it with a stream of electrically charged null fluid, resulting in the formation of a naked singularity. This provides an example of cosmic censorship violation in an exact dynamical solution to low-energy effective string theory and in a case in which the total stress-energy tensor satisfies all energy conditions. When a ≠ 1, our solutions necessarily have a time-independent scalar field and consequently cannot be overcharged.
ER  -