  Observations imply that gamma-ray bursts (GRBs) are produced by the
dissipation of the kinetic energy of a highly relativistic fireball.
Photo-meson interactions of protons with gamma-rays within the fireball
dissipation region are expected to convert a significant fraction of the
fireball energy into high energy neutrinos. In this talk we summarize the
results of an analysis of the internal shock model of GRBs, where production of
synchrotron photons and photo-meson neutrinos with energies about 10^14 eV are
self-consistently calculated. These neutrinos will be coincident with the GRB.
We show that the fraction of fireball energy converted into high energy
neutrinos is not sensitive to uncertainties in the fireball model parameters,
such as the expansion Lorentz factor and characteristic variability time. Other
processes of neutrinos emission from GRBs are also reviewed. Photomeson
interactions within the plasma region shocked by the reverse shock, may produce
a burst of 10^18 eV neutrinos following the GRB on the time scale of 10 s.
Inelastic p-n nuclear collisions result in the production of a burst of around
10 GeV neutrinos in coincidence with the GRB. Planned 1 km^3 neutrino
telescopes are expected to detect ten 100 TeV neutrino events and several 10^18
eV events, correlated with GRBs, per year. A suitably densely spaced detector
may allow the detection of several 10 GeV events per year.

Astrophysics;High Energy Physics - Phenomenology