A Lemaitre-Tolman-Bondi cosmological wormhole
classification
🌀 gr-qc
math-phmath.MP
keywords
shellwormholeaccretionanalyticalbecomescomovingconditionscosmic
read the original abstract
We present a new analytical solution of the Einstein field equations describing a wormhole shell of zero thickness joining two Lema{\i}tre-Tolman-Bondi universes, with no radial accretion. The material on the shell satisfies the energy conditions and, at late times, the shell becomes comoving with the dust-dominated cosmic substratum.
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.