English

Infinitely Many Strings in De Sitter Spacetime: Expanding and Oscillating Elliptic Function Solutions

High Energy Physics - Theory 2009-10-22 v1

Abstract

The exact general evolution of circular strings in 2+12+1 dimensional de Sitter spacetime is described closely and completely in terms of elliptic functions. The evolution depends on a constant parameter bb, related to the string energy, and falls into three classes depending on whether b<1/4b<1/4 (oscillatory motion), b=1/4b=1/4 (degenerated, hyperbolic motion) or b>1/4b>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\tau 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 EE as a function of the string proper size SS, and analyze it for the expanding and oscillating strings. For expanding strings (S˙>0)(\dot{S}>0): E0E\neq 0 even at S=0S=0, EE decreases for small SS and increases S\propto\hspace*{-1mm}S for large SS. For an oscillating string (0SSmax)(0\leq S\leq S_{max}), the average energy <E><E> over one oscillation period is expressed as a function of SmaxS_{max} as a complete elliptic integral of the third kind.

Keywords

Cite

@article{arxiv.hep-th/9312115,
  title  = {Infinitely Many Strings in De Sitter Spacetime: Expanding and Oscillating Elliptic Function Solutions},
  author = {H. J. de Vega and A. L. Larsen and N. Sánchez},
  journal= {arXiv preprint arXiv:hep-th/9312115},
  year   = {2009}
}

Comments

32 pages, Latex file, figures available from the authors under request. LPTHE-PAR 93-56

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