With the most recent multi-messenger detection , a new branch in modern astronomy has been arisen .
The GW170817 event together with the short gamma-ray burst GRB 170817A was the first-ever detection of the gravitational waves and an electromagnetic counterpart .
These detections encourage us to think that in the following years we will detect a single event through three different channels : including the mentioned above plus neutrinos from multiple astrophysical sources , as those detected from SN1987A .
It is believed that short GRBs are originated in the merger of a black-hole ( BH ) with a neutron star ( NS ) or NS-NS scenario .
Particularly only in the latter case , several simulations suggest that the magnetic field can be amplified up to \sim 10 ^ { 15 } -10 ^ { 16 } G. Considering this effect over created thermal neutrinos during the initial stage , we could differentiate short GRB progenitors through the neutrino expected flavor ratio and the opacity created by the the baryon-loaded winds ejected in each scenario .
Moreover , We find that it is more feasible to detect neutrinos from BH-NS than NS-NS systems .
Finally , we also estimate the number of neutrino events expected on ground-based detectors , finding that it is possible to detect neutrinos from an energetic enough source ( L \gtrsim 10 ^ { 52 } erg s ^ { -1 } ) located within a nearby vicinity , such as , GRB170817A ( d = 40 Mpc ) with Hyper-Kamiokande detector .