Self-similar spherical implosion

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We study the self-similar compression of a gas sphere. The radial and time dependencies of density, temperature and velocity are obtained. A central hot region is produced. The model sets no upper limit to the compression factor. We determine the time dependence of the required driving power, which...

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Detalles Bibliográficos
Autores principales: Ferro Fontán, Constantino, Gratton, Julio
Publicado: 1975
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03759601_v55_n1_p35_FerroFontan
http://hdl.handle.net/20.500.12110/paper_03759601_v55_n1_p35_FerroFontan
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Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_03759601_v55_n1_p35_FerroFontan
record_format dspace
spelling paper:paper_03759601_v55_n1_p35_FerroFontan2023-06-08T15:38:45Z Self-similar spherical implosion Ferro Fontán, Constantino Gratton, Julio We study the self-similar compression of a gas sphere. The radial and time dependencies of density, temperature and velocity are obtained. A central hot region is produced. The model sets no upper limit to the compression factor. We determine the time dependence of the required driving power, which agrees with known computer results for optimized implosions. © 1975. Fil:Ferro Fontan, C. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Gratton, J. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 1975 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03759601_v55_n1_p35_FerroFontan http://hdl.handle.net/20.500.12110/paper_03759601_v55_n1_p35_FerroFontan
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description We study the self-similar compression of a gas sphere. The radial and time dependencies of density, temperature and velocity are obtained. A central hot region is produced. The model sets no upper limit to the compression factor. We determine the time dependence of the required driving power, which agrees with known computer results for optimized implosions. © 1975.
author Ferro Fontán, Constantino
Gratton, Julio
spellingShingle Ferro Fontán, Constantino
Gratton, Julio
Self-similar spherical implosion
author_facet Ferro Fontán, Constantino
Gratton, Julio
author_sort Ferro Fontán, Constantino
title Self-similar spherical implosion
title_short Self-similar spherical implosion
title_full Self-similar spherical implosion
title_fullStr Self-similar spherical implosion
title_full_unstemmed Self-similar spherical implosion
title_sort self-similar spherical implosion
publishDate 1975
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03759601_v55_n1_p35_FerroFontan
http://hdl.handle.net/20.500.12110/paper_03759601_v55_n1_p35_FerroFontan
work_keys_str_mv AT ferrofontanconstantino selfsimilarsphericalimplosion
AT grattonjulio selfsimilarsphericalimplosion
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