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Superradiance or total reflection?

Numerical evolution of massless scalar fields on Kerr background is studied. The initial data specifications are chosen to have compact support separated from the ergoregion and to yield nearly monochromatic incident wave packets. The initial data is also tuned to maximize the effect of superradianc...

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Detalles Bibliográficos
Autores principales: László, András, Rácz, István
Lenguaje:eng
Publicado: 2012
Materias:
Acceso en línea:https://dx.doi.org/10.1007/978-3-319-06761-2_15
http://cds.cern.ch/record/1502085
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author László, András
Rácz, István
author_facet László, András
Rácz, István
author_sort László, András
collection CERN
description Numerical evolution of massless scalar fields on Kerr background is studied. The initial data specifications are chosen to have compact support separated from the ergoregion and to yield nearly monochromatic incident wave packets. The initial data is also tuned to maximize the effect of superradiance. Evidences are shown indicating that instead of the anticipated energy extraction from black hole the incident radiation fail to reach the ergoregion rather it suffers a nearly perfect reflection.
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language eng
publishDate 2012
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spelling cern-15020852023-03-14T17:53:25Zdoi:10.1007/978-3-319-06761-2_15http://cds.cern.ch/record/1502085engLászló, AndrásRácz, IstvánSuperradiance or total reflection?General Relativity and CosmologyNumerical evolution of massless scalar fields on Kerr background is studied. The initial data specifications are chosen to have compact support separated from the ergoregion and to yield nearly monochromatic incident wave packets. The initial data is also tuned to maximize the effect of superradiance. Evidences are shown indicating that instead of the anticipated energy extraction from black hole the incident radiation fail to reach the ergoregion rather it suffers a nearly perfect reflection.Numerical evolution of massless scalar fields on Kerr background is studied. The initial data is chosen to have compact support separated from the ergoregion and to yield nearly monochromatic incident wave packets. The initial data is also tuned to maximize the effect of superradiance. We give evidence indicating that instead of the anticipated energy extraction from the black hole the incident radiation fails to reach the ergoregion and instead it suffers a nearly perfect reflection.Numerical evolution of massless scalar fields on Kerr background is studied. The initial data is chosen to have compact support separated from the ergoregion and to yield nearly monochromatic incidentNumerical evolution of massless scalar fields on Kerr background is studied. The initial data specifications are chosen to have compact support separated from the ergoregion and to yield nearly monochromatic incident wave packets. The initial data is also tuned to maximize the effect of superradiance. Evidences are shown indicating that instead of the anticipated energy extraction from black hole the incident radiation fail to reach the ergoregion rather it suffers a nearly perfect reflection.arXiv:1212.4847oai:cds.cern.ch:15020852012-12-21
spellingShingle General Relativity and Cosmology
László, András
Rácz, István
Superradiance or total reflection?
title Superradiance or total reflection?
title_full Superradiance or total reflection?
title_fullStr Superradiance or total reflection?
title_full_unstemmed Superradiance or total reflection?
title_short Superradiance or total reflection?
title_sort superradiance or total reflection?
topic General Relativity and Cosmology
url https://dx.doi.org/10.1007/978-3-319-06761-2_15
http://cds.cern.ch/record/1502085
work_keys_str_mv AT laszloandras superradianceortotalreflection
AT raczistvan superradianceortotalreflection