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INTERACTING KASNER-TYPE COSMOLOGIES

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dc.creatorYOSELIN MAURICIO CATALDO MONSALVES
dc.date2011
dc.date.accessioned2025-01-10T14:42:45Z
dc.date.available2025-01-10T14:42:45Z
dc.date.issued2011
dc.description.abstractIT IS WELL KNOWN THAT KASNER-TYPE COSMOLOGIES PROVIDE A USEFUL FRAMEWORK FOR ANALYZING THE THREE-DIMENSIONAL ANISOTROPIC EXPANSION BECAUSE OF THE SIMPLIFICATION OF THE ANISOTROPIC DYNAMICS. IN THIS PAPER RELATIVISTIC MULTI-FLUID KASNER-TYPE SCENARIOS ARE STUDIED. WE FIRST CONSIDER THE GENERAL CASE OF A SUPERPOSITION OF TWO IDEAL COSMIC FLUIDS, AS WELL AS THE PARTICULAR CASES OF NON-INTERACTING AND INTERACTING ONES, BY INTRODUCING A PHENOMENOLOGICAL COUPLING FUNCTION Q( T). FOR TWO-FLUID COSMOLOGICAL SCENARIOS THERE EXIST ONLY COSMOLOGICAL SCALING SOLUTIONS, WHILE FOR THREE-FLUID CONFIGURATIONS THERE EXIST NOT ONLY COSMOLOGICAL SCALING ONES, BUT ALSO MORE GENERAL SOLUTIONS. IN THE CASE OF TRIPLY INTERACTING COSMIC FLUIDS WE CAN HAVE ENERGY TRANSFER FROM TWO FLUIDS TO A THIRD ONE, OR ENERGY TRANSFER FROM ONE COSMIC FLUID TO THE OTHER TWO. IT IS SHOWN THAT BY REQUIRING THE POSITIVITY OF ENERGY DENSITIES THERE ALWAYS IS A MATTER COMPONENT WHICH VIOLATES THE DOMINANT ENERGY CONDITION IN THIS KIND OF ANISOTROPIC COSMOLOGICAL SCENARIOS.
dc.formatapplication/pdf
dc.identifier.doi10.1007/s10509-011-0596-y
dc.identifier.issn1572-946X
dc.identifier.issn0004-640X
dc.identifier.urihttps://repositorio.ubiobio.cl/handle/123456789/8632
dc.languagespa
dc.publisherASTROPHYSICS AND SPACE SCIENCE
dc.relation.uri10.1007/s10509-011-0596-y
dc.rightsPUBLICADA
dc.titleINTERACTING KASNER-TYPE COSMOLOGIES
dc.typeARTÍCULO
dspace.entity.typePublication
ubb.EstadoPUBLICADA
ubb.Otra ReparticionFACULTAD DE CIENCIAS
ubb.SedeCONCEPCIÓN
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