The search for muon neutrinos from gamma-ray bursts with AMANDA B-10 and AMANDA-II

Gamma-ray bursts have been observed for more than three decades and, yet, much about their nature remains a mystery. Here we describe the results of the ongoing search for high-energy muon neutrinos from gamma-ray bursts with the Antarctic Muon and Neutrino Detector Array (AMANDA). Current results are consistent with no neutrino emission; thus preliminary upper limits are derived for the event rate, four-year combined flux, and single-year fluence. We also address plans for improving these limits in the future.