Regular black holes, universes without singularities, and phantom-scalar field transitions

Understand

We consider a procedure of elimination of cosmological singularities similar to that suggested in the recent paper by Simpson and Visser for the construction of regular black holes.

• It is shown that by imposing a non-singular cosmological evolution with a bounce in a flat Friedmann universe filled with a minimally coupled scalar field, we obtain a transition between the standard scalar field and its phantom counterpart.
• In this case, the potential of the scalar field has a non-analyticity of the cusp type.
• This result is also readily reproduced in the case of an anisotropic Bianchi I universe.