An adjustable law of motion for relativistic spherical shells

Abstract A classical and a relativistic law of motion for an advancing shell are deduced applying the thin layer approximation. A new parameter connected with the quantity of absorbed matter in the expansion is introduced; this allows the matching of theory with observation.

Gespeichert in:

Autor*in:	Zaninetti, Lorenzo [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2011

Schlagwörter:	relativistic fluid dynamics relativistic plasmas supernova remnants

Anmerkung:	© © Versita Warsaw and Springer-Verlag Wien 2011

Übergeordnetes Werk:	Enthalten in: Central European journal of physics - Warsaw : Central European Science Journals, 2003, 10(2011), 1 vom: 27. Okt., Seite 32-39
Übergeordnetes Werk:	volume:10 ; year:2011 ; number:1 ; day:27 ; month:10 ; pages:32-39

Links:	Volltext

DOI / URN:	10.2478/s11534-011-0089-1

Katalog-ID:	SPR020731833

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allfields	10.2478/s11534-011-0089-1 doi (DE-627)SPR020731833 (SPR)s11534-011-0089-1-e DE-627 ger DE-627 rakwb eng Zaninetti, Lorenzo verfasserin aut An adjustable law of motion for relativistic spherical shells 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © © Versita Warsaw and Springer-Verlag Wien 2011 Abstract A classical and a relativistic law of motion for an advancing shell are deduced applying the thin layer approximation. A new parameter connected with the quantity of absorbed matter in the expansion is introduced; this allows the matching of theory with observation. relativistic fluid dynamics (dpeaa)DE-He213 relativistic plasmas (dpeaa)DE-He213 supernova remnants (dpeaa)DE-He213 Enthalten in Central European journal of physics Warsaw : Central European Science Journals, 2003 10(2011), 1 vom: 27. Okt., Seite 32-39 (DE-627)358627494 (DE-600)2097188-6 1644-3608 nnns volume:10 year:2011 number:1 day:27 month:10 pages:32-39 https://dx.doi.org/10.2478/s11534-011-0089-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2110 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 10 2011 1 27 10 32-39
spelling	10.2478/s11534-011-0089-1 doi (DE-627)SPR020731833 (SPR)s11534-011-0089-1-e DE-627 ger DE-627 rakwb eng Zaninetti, Lorenzo verfasserin aut An adjustable law of motion for relativistic spherical shells 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © © Versita Warsaw and Springer-Verlag Wien 2011 Abstract A classical and a relativistic law of motion for an advancing shell are deduced applying the thin layer approximation. A new parameter connected with the quantity of absorbed matter in the expansion is introduced; this allows the matching of theory with observation. relativistic fluid dynamics (dpeaa)DE-He213 relativistic plasmas (dpeaa)DE-He213 supernova remnants (dpeaa)DE-He213 Enthalten in Central European journal of physics Warsaw : Central European Science Journals, 2003 10(2011), 1 vom: 27. Okt., Seite 32-39 (DE-627)358627494 (DE-600)2097188-6 1644-3608 nnns volume:10 year:2011 number:1 day:27 month:10 pages:32-39 https://dx.doi.org/10.2478/s11534-011-0089-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2110 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 10 2011 1 27 10 32-39
allfields_unstemmed	10.2478/s11534-011-0089-1 doi (DE-627)SPR020731833 (SPR)s11534-011-0089-1-e DE-627 ger DE-627 rakwb eng Zaninetti, Lorenzo verfasserin aut An adjustable law of motion for relativistic spherical shells 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © © Versita Warsaw and Springer-Verlag Wien 2011 Abstract A classical and a relativistic law of motion for an advancing shell are deduced applying the thin layer approximation. A new parameter connected with the quantity of absorbed matter in the expansion is introduced; this allows the matching of theory with observation. relativistic fluid dynamics (dpeaa)DE-He213 relativistic plasmas (dpeaa)DE-He213 supernova remnants (dpeaa)DE-He213 Enthalten in Central European journal of physics Warsaw : Central European Science Journals, 2003 10(2011), 1 vom: 27. Okt., Seite 32-39 (DE-627)358627494 (DE-600)2097188-6 1644-3608 nnns volume:10 year:2011 number:1 day:27 month:10 pages:32-39 https://dx.doi.org/10.2478/s11534-011-0089-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2110 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 10 2011 1 27 10 32-39
allfieldsGer	10.2478/s11534-011-0089-1 doi (DE-627)SPR020731833 (SPR)s11534-011-0089-1-e DE-627 ger DE-627 rakwb eng Zaninetti, Lorenzo verfasserin aut An adjustable law of motion for relativistic spherical shells 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © © Versita Warsaw and Springer-Verlag Wien 2011 Abstract A classical and a relativistic law of motion for an advancing shell are deduced applying the thin layer approximation. A new parameter connected with the quantity of absorbed matter in the expansion is introduced; this allows the matching of theory with observation. relativistic fluid dynamics (dpeaa)DE-He213 relativistic plasmas (dpeaa)DE-He213 supernova remnants (dpeaa)DE-He213 Enthalten in Central European journal of physics Warsaw : Central European Science Journals, 2003 10(2011), 1 vom: 27. Okt., Seite 32-39 (DE-627)358627494 (DE-600)2097188-6 1644-3608 nnns volume:10 year:2011 number:1 day:27 month:10 pages:32-39 https://dx.doi.org/10.2478/s11534-011-0089-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2110 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 10 2011 1 27 10 32-39
allfieldsSound	10.2478/s11534-011-0089-1 doi (DE-627)SPR020731833 (SPR)s11534-011-0089-1-e DE-627 ger DE-627 rakwb eng Zaninetti, Lorenzo verfasserin aut An adjustable law of motion for relativistic spherical shells 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © © Versita Warsaw and Springer-Verlag Wien 2011 Abstract A classical and a relativistic law of motion for an advancing shell are deduced applying the thin layer approximation. A new parameter connected with the quantity of absorbed matter in the expansion is introduced; this allows the matching of theory with observation. relativistic fluid dynamics (dpeaa)DE-He213 relativistic plasmas (dpeaa)DE-He213 supernova remnants (dpeaa)DE-He213 Enthalten in Central European journal of physics Warsaw : Central European Science Journals, 2003 10(2011), 1 vom: 27. Okt., Seite 32-39 (DE-627)358627494 (DE-600)2097188-6 1644-3608 nnns volume:10 year:2011 number:1 day:27 month:10 pages:32-39 https://dx.doi.org/10.2478/s11534-011-0089-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2110 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 10 2011 1 27 10 32-39
language	English
source	Enthalten in Central European journal of physics 10(2011), 1 vom: 27. Okt., Seite 32-39 volume:10 year:2011 number:1 day:27 month:10 pages:32-39
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author	Zaninetti, Lorenzo
spellingShingle	Zaninetti, Lorenzo misc relativistic fluid dynamics misc relativistic plasmas misc supernova remnants An adjustable law of motion for relativistic spherical shells
authorStr	Zaninetti, Lorenzo
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topic_title	An adjustable law of motion for relativistic spherical shells relativistic fluid dynamics (dpeaa)DE-He213 relativistic plasmas (dpeaa)DE-He213 supernova remnants (dpeaa)DE-He213
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topic_unstemmed	misc relativistic fluid dynamics misc relativistic plasmas misc supernova remnants
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title	An adjustable law of motion for relativistic spherical shells
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title_full	An adjustable law of motion for relativistic spherical shells
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title_sort	adjustable law of motion for relativistic spherical shells
title_auth	An adjustable law of motion for relativistic spherical shells
abstract	Abstract A classical and a relativistic law of motion for an advancing shell are deduced applying the thin layer approximation. A new parameter connected with the quantity of absorbed matter in the expansion is introduced; this allows the matching of theory with observation. © © Versita Warsaw and Springer-Verlag Wien 2011
abstractGer	Abstract A classical and a relativistic law of motion for an advancing shell are deduced applying the thin layer approximation. A new parameter connected with the quantity of absorbed matter in the expansion is introduced; this allows the matching of theory with observation. © © Versita Warsaw and Springer-Verlag Wien 2011
abstract_unstemmed	Abstract A classical and a relativistic law of motion for an advancing shell are deduced applying the thin layer approximation. A new parameter connected with the quantity of absorbed matter in the expansion is introduced; this allows the matching of theory with observation. © © Versita Warsaw and Springer-Verlag Wien 2011
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title_short	An adjustable law of motion for relativistic spherical shells
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up_date	2024-07-03T17:55:02.647Z
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