Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2000-02-18
Phys.Lett. B486 (2000) 300-305
Physics
High Energy Physics
High Energy Physics - Phenomenology
12 pages, no figure, plain latex, errors corrected, accepted for publication in PLB
Scientific paper
10.1016/S0370-2693(00)00782-6
Cosmlogical domain walls produced during phase transition are expected to collapse on a cosmologically safe timescale if Vilenkin's condition is satisfied. We show that the decaying processes of these unstable domain walls should be changed significantly if weak scale inflation takes place. The usual condition for the safe decay of the cosmological domain wall must be changed, depending on their scales and interactions. As a result, the energy scales and explicit breaking terms of such walls must satisfy severe requirements. We also make a brief comment on cosmological structure formation.
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