dc.creator | DOLAN, Sam R. | |
dc.creator | OLIVEIRA, Ednilton S. | |
dc.creator | CRISPINO, Luis C. B. | |
dc.date.accessioned | 2012-04-19T00:12:22Z | |
dc.date.accessioned | 2018-07-04T14:41:49Z | |
dc.date.available | 2012-04-19T00:12:22Z | |
dc.date.available | 2018-07-04T14:41:49Z | |
dc.date.created | 2012-04-19T00:12:22Z | |
dc.date.issued | 2009 | |
dc.identifier | PHYSICAL REVIEW D, v.79, n.6, 2009 | |
dc.identifier | 1550-7998 | |
dc.identifier | http://producao.usp.br/handle/BDPI/16369 | |
dc.identifier | 10.1103/PhysRevD.79.064014 | |
dc.identifier | http://dx.doi.org/10.1103/PhysRevD.79.064014 | |
dc.identifier.uri | http://repositorioslatinoamericanos.uchile.cl/handle/2250/1613191 | |
dc.description.abstract | This is a study of a monochromatic planar perturbation impinging upon a canonical acoustic hole. We show that acoustic hole scattering shares key features with black hole scattering. The interference of wave fronts passing in opposite senses around the hole creates regular oscillations in the scattered intensity. We examine this effect by applying a partial wave method to compute the differential scattering cross section for a range of incident wavelengths. We demonstrate the existence of a scattering peak in the backward direction, known as the glory. We show that the glory created by the canonical acoustic hole is approximately 170 times less intense than the glory created by the Schwarzschild black hole, for equivalent horizon-to-wavelength ratios. We hope that direct experimental observations of such effects may be possible in the near future. | |
dc.language | eng | |
dc.publisher | AMER PHYSICAL SOC | |
dc.relation | Physical Review D | |
dc.rights | Copyright AMER PHYSICAL SOC | |
dc.rights | restrictedAccess | |
dc.title | Scattering of sound waves by a canonical acoustic hole | |
dc.type | Artículos de revistas | |