Scattering of scalar particles by a black hole

M. Yu. Kuchiev and V. V. Flambaum
Phys. Rev. D 70, 044022 – Published 18 August 2004
PDFExport Citation

Abstract

The absorption cross section for scalar particle impact on a Schwarzschild black hole is found. The process is dominated by two physical phenomena. One of them is the well-known greybody factor that arises from the energy-dependent potential barrier outside the horizon that filters the incoming and outgoing waves. The other is related to the reflection of particles on the horizon (M.Yu. Kuchiev, gr-qc/0310008, [19,20]). This latter effect strongly diminishes the cross section for low energies, forcing it to vanish in the infrared limit. It is argued that this is a general property, the absorption cross section vanishes in the infrared limit for scattering of particles of arbitrary spin.

  • Received 14 December 2003

DOI:https://doi.org/10.1103/PhysRevD.70.044022

©2004 American Physical Society

Authors & Affiliations

M. Yu. Kuchiev* and V. V. Flambaum

  • School of Physics, University of New South Wales, Sydney 2052, Australia

  • *Email address: kuchiev@newt.phys.unsw.edu.au
  • Also at Institute for Advanced Study, Einstein Drive, Princeton, New Jersey 08540, USA. Email address: flambaum@newt.phys.unsw.edu.au

References (Subscription Required)

Click to Expand
Issue

Vol. 70, Iss. 4 — 15 August 2004

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review D

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×