  We calculate the high energy neutrino spectrum from gamma-ray bursts where
the emission arises in a dissipative jet photosphere determined by either
baryonically or magnetically dominated dynamics, and compare these neutrino
spectra to those obtained in conventional internal shock models. We also
calculate the diffuse neutrino spectra based on these models, which appear
compatible with the current IceCube 40+59 constraints. While a re-analysis
based on the models discussed here and the data from the full array would be
needed, it appears that only those models with the most extreme parameters are
close to being constrained at present. A multi-year operation of the full
IceCube and perhaps a next generation of large volume neutrino detectors may be
required in order to distinguish between the various models discussed.
