Ponente
Heinrich Päs
(Universität Dortmund)
Descripción
We suggest a structure for the vacuum comprised of a network of tightly knotted/linked flux tubes formed in a QCD-like cosmological phase transition and show that such a network can drive cosmological inflation. As the network can be topologically stable only in three space dimensions, this scenario provides a dynamical explanation for the existence of exactly three large spatial dimensions in our Universe.
Autor primario
Heinrich Päs
(Universität Dortmund)
