Superradiant Phenomena for Spinor Fields in Rotating Black Hole Geometry
Nara Women’s University and Nara Science Academy
2 Konkuk University
3 Seoul National University
4 Tezukayama University
* e-mail: firstname.lastname@example.org
** e-mail: email@example.com
*** e-mail: firstname.lastname@example.org
**** e-mail: email@example.com
Published online: 9 January 2018
We derive the results (i) the ortho-normal and completeness relations for normal modes and (ii) non-existence of zero mode for spinor fields in rotating black hole geometry. From these results, we show that superradiant phenomena for spinor fields should be type 2: positive momentum on the horizon (pH > 0) and negative frequency at infinity (ω < 0).
© The Authors, published by EDP Sciences, 2018
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (http://creativecommons.org/licenses/by/4.0/).