11.5. Low Energy Neutrinos
Most of the energy generated in any core collpase event and in
particular in NS2M is released as low energy (~ 5 - 10 MeV)
neutrinos
[277].
The total energy is quite large ~ a few × 1053 ergs,
leading to
flow energy -
10. However, this
neutrino signal will be quite similar to a
supernova neutrino signal, and at present only galactic SN neutrinos
can be detected. Supernovae are ten thousand times more frequent then
GRBs and therefore low energy neutrinos associated with GRB constitute
an insignificant contribution to the background at this energy range.