The exact general evolution of circular strings in 2+1 dimensional de
Sitter spacetime is described closely and completely in terms of elliptic
functions. The evolution depends on a constant parameter b, related to the
string energy, and falls into three classes depending on whether b<1/4
(oscillatory motion), b=1/4 (degenerated, hyperbolic motion) or b>1/4
(unbounded motion). The novel feature here is that one single world-sheet
generically describes {\it infinitely many} (different and independent)
strings. The world-sheet time τ is an infinite-valued function of the
string physical time, each branch yields a different string. This has no
analogue in flat spacetime. We compute the string energy E as a function of
the string proper size S, and analyze it for the expanding and oscillating
strings. For expanding strings (S˙>0): E=0 even at S=0, E
decreases for small S and increases ∝S for large S.
For an oscillating string (0≤S≤Smax), the average energy
over one oscillation period is expressed as a function of Smax as a
complete elliptic integral of the third kind.Comment: 32 pages, Latex file, figures available from the authors under
request. LPTHE-PAR 93-5