Stable and unstable circular strings in inflationary universes.

It was shown by Garriga and Vilenkin that the circular shape of nucleated cosmic strings, of zero loop energy in de Sitter space, is stable in the sense that the ratio of the mean fluctuation amplitude to the loop radius is constant. This result can be generalized to all expanding strings (of nonzero loop energy) in de Sitter space. In other curved spacetimes the situation, however, may be different. In this paper we develop a general formalism treating fluctuations around circular strings embedded in arbitrary spatially flat FRW spacetimes. As examples we consider Minkowski space, de Sitter space, and power law expanding universes. In the special case of power law inflation we find that in certain cases the fluctuations grow much slower than the radius of the underlying unperturbed circular string. The inflation of the Universe thus tends to wash out the fluctuations and to stabilize these strings.