
pmid: 10011905
The dynamics of thick domain walls are studied in the context of the classical field theory for a real scalar field. We treat, by numerically solving the equation of motion for the scalar field, the collision of two plane-symmetric walls as well as the collapse of walls that have spherical and cylindrical symmetry. Walls in both sine-Gordon and ${\ensuremath{\varphi}}^{4}$ theories are considered. We illustrate the striking and at times surprising differences between thin and thick walls. We also discuss the formation of black holes during spherical collapse.
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| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Top 10% | |
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