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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...
Autores principales: | , |
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Lenguaje: | eng |
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2012
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Acceso en línea: | https://dx.doi.org/10.1007/978-3-319-06761-2_15 http://cds.cern.ch/record/1502085 |
_version_ | 1780927101876043776 |
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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. |
id | cern-1502085 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2012 |
record_format | invenio |
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 |