Motivated by the paradigm of a super-Maltusian population catastrophe, we study a simple stochastic population model which exhibits a finite-time blowup of the population size and is strongly affected by intrinsic noise. We focus on the fluctuations of the blowup time in the asexual binary reproduction model , where two identical individuals give birth to a third one. We determine exactly the average blowup time as well as the probability distribution of the blowup time and its moments. In particular, we show that the long-time tail is purely exponential. The short-time tail exhibits an essential singularity at , and it is dominated by a single (the most likely) population trajectory which we determine analytically.

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