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The W3-string spectrum

C. N. Pope, L. J. Romans, E. Sezgin, K. S. Stelle

hep-tharXiv:hep-th/9110015

Abstract

We study the spectrum of W3 strings. In particular, we show that for appropriately chosen space-time signature, one of the scalar fields is singled out by the spin-3 constraint and is ``frozen'': no creation operators from it can appear in physical states and the corresponding momentum must assume a specific fixed value. The remaining theory is unitary and resembles an ordinary string theory in d26 with anomalies cancelled by appropriate background charges. In the case of the W3 string, however, the spin-two ``graviton'' is massive.

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