Quasiclassical scattering and glory effect in the gravitational field of a black hole.

Details Quasiclassical scattering and glory effect in the gravitational field of a black hole. Quasiclassical scattering and glory effect in the gravitational field of a black hole.

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jetp...69...13g&link_type=abstract

Sov. Phys. - JETP, Vol. 69, No. 1, p. 13 - 16

Physics

1

Black Holes: Scattering, Black Holes: Gravitational Field

Scientific paper

The differential cross section for backward scattering
(θ→π) of spinless particles with nonzero rest mass on the
background of a Schwarzschild geometry is calculated by
quantum-mechanical methods. It is shown that a glory exists if the
gravitational radius exceeds the particle wavelength.

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