Bose-Einstein condensation in helium white dwarf stars. I

dc.creatorMosquera, Mercedes Elisa
dc.creatorCivitarese, Enrique Osvaldo
dc.creatorBenvenuto, Omar Gustavo
dc.creatorDe Vito, María Alejandra
dc.date2010
dc.date2019-10-02T12:29:24Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/82452
dc.identifierissn:03702693
dc.descriptionThe formation of a Bose-Einstein condensate in the interior of helium white dwarfs stars is discussed. Following the proposal made by Gabadadze and Rosen, we have explored the consequences of such a mechanism by calculating the cooling time of the stars. We have found that it is shorter than the value predicted by the standard model.
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.descriptionFacultad de Ciencias Exactas
dc.formatapplication/pdf
dc.format119-122
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Astronómicas
dc.subjectBose-Einstein condensation
dc.subjectWhite dwarf
dc.titleBose-Einstein condensation in helium white dwarf stars. I
dc.typeArticulo
dc.typeArticulo


Este ítem pertenece a la siguiente institución