W-singularities in cosmological models

Fernández Jambrina, Leonardo (2011). W-singularities in cosmological models. "Journal of Physics: Conference Series", v. 314 (n. 1); pp.. ISSN 1742-6596. https://doi.org/10.1088/1742-6596/314/1/012061.


Title: W-singularities in cosmological models
  • Fernández Jambrina, Leonardo
Item Type: Article
Título de Revista/Publicación: Journal of Physics: Conference Series
Date: September 2011
ISSN: 1742-6596
Volume: 314
Faculty: E.T.S.I. Navales (UPM)
Department: Enseñanzas Básicas de la Ingeniería Naval [hasta 2014]
Creative Commons Licenses: Recognition - No derivative works - Non commercial

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Recently a new type of cosmological singularity has been postulated for infinite barotropic index w in the equation of state p = wρ of the cosmological fluid, but vanishing pressure and density at the singular event. Apparently the barotropic index w would be the only physical quantity to blow up at the singularity. In this talk we would like to discuss the strength of such singularities and compare them with other types. We show that they are weak singularities

More information

Item ID: 11227
DC Identifier: https://oa.upm.es/11227/
OAI Identifier: oai:oa.upm.es:11227
DOI: 10.1088/1742-6596/314/1/012061
Official URL: http://iopscience.iop.org/1742-6596/314/1/012061/
Deposited by: Memoria Investigacion
Deposited on: 04 Jul 2012 11:03
Last Modified: 20 Apr 2016 19:22
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