Generalized superradiant scattering
- 1. Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, B.C. V6T 1Z1 (Canada)
- 2. Astrophysics Sector, International School for Advanced Studies, Via Beirut 2-4, 34014 Trieste (Italy) and INFN, Sezione di Trieste (Italy)
Description
We analyze the necessary and sufficient conditions for the occurrence of superradiance. Starting with a wave equation we examine the possibility of superradiance in terms of an effective potential and boundary conditions. In particular, we show that the existence of an ergoregion is not sufficient; an appropriate boundary condition, e.g. only ingoing group velocity waves at an event horizon, is also crucial. After applying our scheme to the standard examples of superradiance, we show that analogue models of gravity without an event horizon do not necessarily exhibit superradiance. Particularly, we show that the superradiant phenomenon is absent in purely rotating inviscid fluids with vorticity. We argue that there should be a catalogue of superradiant systems that can be found by focusing on the necessary and sufficient conditions outlined below.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.80.124016;
- arXiv
- arXiv:0909.2317v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 80
- Journal Issue
- 12
- Journal Page Range
- p. 124016-124016.5
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41056908
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- BOUNDARY CONDITIONS; GRAVITATION; POTENTIALS; SCATTERING; SUPERRADIANCE; VELOCITY; WAVE EQUATIONS
- Descriptors DEC
- DIFFERENTIAL EQUATIONS; EMISSION; ENERGY-LEVEL TRANSITIONS; EQUATIONS; PARTIAL DIFFERENTIAL EQUATIONS; PHOTON EMISSION; STIMULATED EMISSION
Optional Information
- Notes
- (c) 2009 The American Physical Society