2018/11/30 by Ion I. Cotaescu, Ciprian A. Sporea
Physics and Astronomy · #gr-qc
paper · pdf · doi:10.1140/epjc/s10052-018-6525-2
published as Eur. Phys. J. C, (2019) 79:15 · v2: matches the published version in EPJC; 8 pages two-column, 3 figures; this work is connected to arXiv:1409.7201
arxiv created 2019/01/14 · arxiv updated 2019/01/15
The asymptotic form of Dirac spinors in the field of a Schwarzschild black hole is used for deriving analytically for the first time the phase shifts of the partial wave analysis of Dirac fermions scattered from massive spherical bodies, imagined as black holes surrounded by a surface producing total reflection. A simple model is analyzed by using graphical methods.