  The properties of a particular Misner - Thorne wormhole are investigated. The
"exotic stress-energy" needed to maintain the wormhole open corresponds to a
massless scalar field whose Lagrangean density contains a negative kinetic
term. While the Komar energy of the spacetime is vanishing due to the negative
energy density and radial pressure, the ADM energy is (minus) the Planck
energy. The timelike geodesics are hyperbolae and any static observer is
inertial. The null radial trajectories are also hyperbolae and Lorentz
invariant as Coleman- de Luccia expanding bubble or Ipser-Sikivie domain wall.
Using a different equation of state for the fluid on the dynamic wormhole
throat of Redmount and Suen, we reached an equation of motion for the throat (a
hyperbola) that leads to a negative surface energy density and the throat
expands with the same acceleration $2\pi |\sigma|$ as the Ipser-Sikivie domain
wall.
