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Protons accelerated in the internal shocks of a long duration gamma ray burstcan escape the fireball as cosmic rays by converting to neutrons. Hadronicinteractions of these neutrons inside a stellar wind bubble created by theprogenitor star will produce TeV gamma rays via neutral meson decay andsynchrotron radiation by charged pion-decay electrons in the wind magneticfield. Such gamma rays should be observable from nearby gamma ray bursts bycurrently running and upcoming ground-based detectors.

Prompt TeV Emission from Cosmic Rays Accelerated by Gamma Ray Bursts Interacting with Surrounding Stellar Wind