Ciencias,UNAM

INSTABILITIES IN A RELATIVISTIC VISCOUS-FLUID

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dc.contributor.author CORONAGALINDO, MG
dc.contributor.author KLAPP, J
dc.contributor.author VAZQUEZ, A
dc.date.accessioned 2011-01-22T10:28:52Z
dc.date.available 2011-01-22T10:28:52Z
dc.date.issued 1990
dc.identifier.issn 0185-1101
dc.identifier.uri http://hdl.handle.net/11154/3631
dc.description.abstract The hydrodynamical equations of a relativistic imperfect fluid are solved, and the hydrodynamical modes are analysed with the aim to establish correlations with cosmological structures. en_US
dc.language.iso en en_US
dc.title INSTABILITIES IN A RELATIVISTIC VISCOUS-FLUID en_US
dc.type Article en_US
dc.identifier.idprometeo 3503
dc.source.novolpages 21:28-30
dc.subject.wos Astronomy & Astrophysics
dc.description.index WoS: SCI, SSCI o AHCI
dc.subject.keywords COSMOLOGY
dc.subject.keywords HYDRODYNAMICS
dc.subject.keywords RELATIVITY
dc.relation.journal Revista Mexicana De Astronomia Y Astrofisica

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