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Authordc.contributor.authorGratton, F. T. 
Authordc.contributor.authorGnavi, G. 
Authordc.contributor.authorGalvão, R. M.O. 
Authordc.contributor.authorGomberoff, L. 
Admission datedc.date.accessioned2019-01-29T15:34:48Z
Available datedc.date.available2019-01-29T15:34:48Z
Publication datedc.date.issued1997
Cita de ítemdc.identifier.citationAstrophysics and Space Science, Volumen 256, Issue 1-2, 2018, Pages 311-319
Identifierdc.identifier.issn0004640X
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/161729
Abstractdc.description.abstractWe study the modulational instability of an electron-positron plasma with relativistic temperatures and phonon damping. It is shown that when the phonon damping is O (1) or O (ε), a modulational instability appears even for classical temperatures. When the phonon damping is O (ε2)), we find that in the non-relativistic limit, previous results are recovered, and for ultrarelativistic temperatures, the instability occurs in a wider band around the relativistic plasma frequency.
Lenguagedc.language.isoen
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
Sourcedc.sourceAstrophysics and Space Science
Keywordsdc.subjectAstronomy and Astrophysics
Keywordsdc.subjectSpace and Planetary Science
Títulodc.titleGrowth rates of envelope modulations of electromagnetic waves in relativistic temperature electron-positron plasmas, stimulated by weak or finite phonon damping
Document typedc.typeArtículo de revista
Catalogueruchile.catalogadorSCOPUS
Indexationuchile.indexArtículo de publicación SCOPUS
uchile.cosechauchile.cosechaSI


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Attribution-NonCommercial-NoDerivs 3.0 Chile
Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile