Abstract—When taking into account the quantum effects, a black hole can emit the so-called Hawking radiation. This Hawking radiation propagates in a curved spacetime due to the presence of a black hole. In this paper, the Myers-Perry black hole is considered, which is an uncharged, rotating black hole occurring in higher dimensions. Scalar Hawking radiation emitted from the Myers-Perry black hole is studied. The rigorous bounds on the greybody factors for massless scalar field of negative-angular-momentum modes are also derived.
Index Terms—Greybody factor, hawking radiation, myers-perry black hole, rigorous bound.
T. Ngampitipan and A. Chatrabhuti is with the Particle Physics Research Laboratory, Department of Physics, Faculty of Science, Chulalongkorn University, Bangkok 10330, Thailand (e-mail: tritos.ngampitipan@gmail.com, dma3ac2@gmail.com)).
P. Boonserm is with the Department of Mathematics and Computer Science, Faculty of Science, Chulalongkorn University, Bangkok 10330, Thailand (e-mail: petarpa.boonserm@gmail.com).
M. Visser is with the School of Mathematics, Statistics, and Operations Research, Victoria University of Wellington, PO Box 600, Wellington, New Zealand (e-mail: matt.visser@msor.vuw.ac.nz).
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Cite: Tritos Ngampitipan, Petarpa Boonserm, Auttakit Chatrabhuti, and Matt Visser, "Rigorous Bounds on Greybody Factors: Scalar Emission of Negative Angular Momentum Modes from Myers-Perry Black Holes," International Journal of Engineering and Technology vol. 8, no. 4, pp. 311-314, 2016.
