Abstract It has been shown that disk fragmentation within several tens of au from the star is very difficult when the gravitational instability and cooling time criterion are considered. However, in the stochastic fragmentation scenario, things may be different. We investigate stochastic fragmentation in protoplanetary disks. In the stochastic fragmentation model, we consider the effects of the external irradiation on the fragmentation process. For the stochastic fragmentation, owing to the probability of generating bound fragments at longer cooling times relative to the critical value and the short collapsing times in the external irradiation region, the inner boundary of the fragmentation region extends inward to 19 au. We find that the required self-gravitating lifetime for fragmentation in the external irradiation region is far less than the self-gravitating lifetime of the disk. Therefore, once a radius is in the external irradiation region, the fragmentation probability increases quickly to 1 after gravitational instability sets in, and fragmentation occurs within a short period of time. We also find that the self-gravitating lifetime required for fragmentation decreases significantly as the radius increases in the external irradiation region.
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