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The High Altitude Water Cherenkov (HAWC) Observatory is a ground-based TeVgamma-ray observatory in the state of Puebla, Mexico at an altitude of 4100 m.Its 22,000 m$^2$ instrumented area, wide field of view ($\sim$2 sr), and >95%uptime make it an ideal instrument for discovering gamma-ray burst (GRB)emission at $\sim$100 GeV. Such a discovery would provide key information aboutthe origins of prompt GRB emission as well as constraints on extra-galacticbackground light (EBL) models and the violation of Lorentz invariance. We willpresent prospects for discovering GRB emission at $\sim$100 GeV with a simple,all-sky search algorithm using HAWC data that is most sensitive to short GRBs.The search algorithm presented here can also be used to detect other shorttransients with timescales and fluxes similar to short GRBs.

All-sky sensitivity of HAWC to Gamma-Ray Bursts