Shadow of a Kaluza-Klein rotating dilaton black hole
Leonardo D. AmarillaDepartamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Ciudad Universitaria, Pabellón 1, 1428 Buenos Aires, ArgentinaErnesto F. EiroaInstituto de Astronomía y Física del Espacio, Casilla de Correo 67 Sucursal 28, 1428 Buenos Aires, Argentina
2013en
Ochiq kirishBronza
ABI
Annotatsiya
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.
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