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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) 
Rocha, J., De Oliveira, E.S. & Rocha, J.V. (2018). Superradiance of rotating cohomogeneity-1 black holes: Scalar case. In 14th Marcel Grossman Meeting On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories, Proceedings. (pp. 1810-1815).
Exportar Referência (IEEE) 
J. M. Rocha et al.,  "Superradiance of rotating cohomogeneity-1 black holes: Scalar case", in 14th Marcel Grossman Meeting On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories, Proc., 2018, pp. 1810-1815
Exportar BibTeX 
@inproceedings{rocha2018_1732209364545,
	author = "Rocha, J. and De Oliveira, E.S. and Rocha, J.V.",
	title = "Superradiance of rotating cohomogeneity-1 black holes: Scalar case",
	booktitle = "14th Marcel Grossman Meeting On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories, Proceedings",
	year = "2018",
	editor = "",
	volume = "",
	number = "",
	series = "",
	doi = "10.1142/9789813226609_0187",
	pages = "1810-1815",
	publisher = "",
	address = "",
	organization = "",
	url = "http://www.scopus.com/inward/record.url?eid=2-s2.0-85059065875&partnerID=MN8TOARS"
}
Exportar RIS 
TY  - CPAPER
TI  - Superradiance of rotating cohomogeneity-1 black holes: Scalar case
T2  - 14th Marcel Grossman Meeting On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories, Proceedings
AU  - Rocha, J.
AU  - De Oliveira, E.S.
AU  - Rocha, J.V.
PY  - 2018
SP  - 1810-1815
DO  - 10.1142/9789813226609_0187
UR  - http://www.scopus.com/inward/record.url?eid=2-s2.0-85059065875&partnerID=MN8TOARS
AB  - Greybody factors of rotating cohomogeneity-1 black holes in higher odd dimensions are studied for the cases in which the cosmological constant is zero, positive, or negative. Attention is given to the main superradiant modes. It is shown that the increase of the intensity of the cosmological constant can have diverse effects on the maximum amplification obtained. In the case of de Sitter (dS) black holes, maximum amplification is enhanced for higher values of the cosmological constant. In the case of Anti-de Sitter (AdS) black holes, the increase of the absolute value of the cosmological constant has the effect of suppressing the maximum amplification initially, but eventually this behavior reverses and we observe growth. This phenomenon can be interpreted as contributions from amplification peaks of distinct origin that become dominant in different regimes.
ER  -