pith. sign in

arxiv: gr-qc/0404037 · v1 · pith:AEXTZSYJnew · submitted 2004-04-08 · 🌀 gr-qc

Cosmological evolution of a ghost scalar field

classification 🌀 gr-qc
keywords wormholeaccelerationcosmologicalfieldscalarcaseconnectconsider
0
0 comments X
read the original abstract

We consider a scalar field with a negative kinetic term minimally coupled to gravity. We obtain an exact non-static spherically symmetric solution which describes a wormhole in cosmological setting. The wormhole is shown to connect two homogeneous spatially flat universes expanding with acceleration. Depending on the wormhole's mass parameter $m$ the acceleration can be constant (the de Sitter case) or infinitely growing.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.