Non Extensivity in Meteor Showers

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dc.creatorSotolongo-Costa, Oscar
dc.creatorGamez, R.
dc.creatorLuzon, F.
dc.creatorPosadas, A.
dc.creatorBeckmann, Pablo Weigandt
dc.date2007-10-25
dc.date.accessioned2026-07-07T08:38:46Z
dc.date.available2026-07-07T08:38:46Z
dc.descriptionA meteor shower is a luminous phenomenon that takes place by the entry into the Earths atmosphere of a cascade of particles coming from a stream intersected by our planet in its orbit. Here we investigate the possibility of a description of the mass distribution of meteoroids in meteor showers int terms of a non extensive formulation, which could shed light and give some insight into the origin of such particles.
dc.descriptionTo be submitted for publication
dc.identifierhttps://arxiv.org/abs/0710.4963
dc.identifierhttp://arxiv.org/abs/0710.4963
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/140849
dc.subjectStatistical Mechanics
dc.titleNon Extensivity in Meteor Showers
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