Evolution of domain walls in the early Universe

The evolution of domain walls in the early Universe is studied via two-dimensional computer simulation. The walls are initially configured on a triangular lattice and then released from the lattice, their evolution driven by the wall curvature and by universal expansion. The walls attain an average velocity of about 0.3c and their surface area per volume (as measured in comoving coordinates) goes down with a slope of -1 with respect to conformal time regardless of whether the Universe is matter or radiation dominated. The additional influence of vacuum pressure causes the energy density to fall away from this slope and steepen, thus allowing a situation in which domain walls can constitute a significant portion of the energy density of the Universe without provoking an unacceptably large perturbation upon the microwave background