High Energy Neutrinos from the Gravitational Wave event GW150914
  possibly associated with a short Gamma-Ray Burst
  High-energy neutrino (HEN) and gravitational wave (GW) can probe
astrophysical sources in addition to electromagnetic observations.
Multimessenger studies can reveal nature of the sources which may not be
discerned from one type of signal alone. We discuss HEN emission in connection
with the Advanced Laser Interferometer Gravitational-wave Observatory (ALIGO)
event GW150914 which could be associated with a short gamma-ray burst (GRB)
detected by the $Fermi$ Gamma-ray Burst Monitor (GBM) 0.4 s after the GW event
and within localization uncertainty of the GW event. We calculate HEN flux from
this short GRB, GW150914-GBM, and show that non-detection of a high-energy
starting event (HESE) by the IceCube Neutrino Observatory can constrain the
total isotropic-equivalent jet energy of this short burst to be less than
$3\times 10^{52}$ erg.
