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We show that radio bursts from cusps on superconducting strings are linearlypolarized, thus, providing a signature that can be used to distinguish themfrom astrophysical sources. We write the event rate of string-generated radiotransients in terms of observational variables, namely, the event duration andflux. Assuming a canonical set of observational parameters, we find that theburst event rate can be quite reasonable, e.g., order ten a year for GrandUnified strings with 100 TeV currents, and a lack of observed radio bursts canpotentially place strong constraints on particle physics models.

Radio bursts from superconducting strings