Shadow of a Kaluza-Klein rotating dilaton black hole

dc.creator	Amarilla, Leonardo
dc.creator	Eiroa, Ernesto Fabian
dc.date.accessioned	2015-06-05T19:12:33Z
dc.date.accessioned	2018-11-06T15:58:37Z
dc.date.available	2015-06-05T19:12:33Z
dc.date.available	2018-11-06T15:58:37Z
dc.date.created	2015-06-05T19:12:33Z
dc.date.issued	2013-02
dc.identifier	Amarilla, Leonardo; Eiroa, Ernesto Fabian; Shadow of a Kaluza-Klein rotating dilaton black hole; Amer Physical Soc; Physical Review D; 87; 4; 2-2013; 44057(7);
dc.identifier	1550-7998
dc.identifier	http://hdl.handle.net/11336/608
dc.identifier.uri	http://repositorioslatinoamericanos.uchile.cl/handle/2250/1903118
dc.description.abstract	We study the shadow produced by a spinning Kaluza-Klein black hole in Einstein gravity coupled to a Maxwell field and a dilaton. The size and the shape of the shadow depend on the mass, the charge, and the angular momentum. We find that, for fixed values of these parameters, the shadow is slightly larger and less deformed than for its Kerr-Newman counterpart.
dc.language	eng
dc.publisher	Amer Physical Soc
dc.relation	info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1103/PhysRevD.87.044057
dc.rights	https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rights	info:eu-repo/semantics/openAccess
dc.subject	KALUZA-KLEIN
dc.subject	GRAVITY
dc.subject	BLACK HOLE
dc.subject	SHADOW
dc.title	Shadow of a Kaluza-Klein rotating dilaton black hole
dc.type	Artículos de revistas
dc.type	Artículos de revistas
dc.type	Artículos de revistas