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We consider observational properties of gamma-ray bursts (GRB) transmitted byhypothetical wormholes (WH). Such burst would be observable as repeatingsource, analogous to Soft Gamma-Repeaters (SGR). We show that the known sourcesof SGR cannot be WH candidates. We also discuss observational properties of GRBwhich might be a signature of WH.

To the search for observational evidence of wormholes