The short time structure (possibly shot noise) might reveal much about the spatial nature of the GRB source. In the case of GRBs from Primordial Black Holes (PBHs), the initial explosion region is∼10−13 cmin size, much smaller than any other known compact object. The BATSE team has already reported on one interesting event. We report here on the study of the TTE data from three BATSE events that may be PBH candidates. The latest results will be presented at the meeting. ©1996 American Institute of Physics.