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Abstract The basic structure of comet nuclei is an aggregation of grains, with a size distribution that extends over several orders of magnitude and a similar distribution of pores. Although attempts… (More)
Abstract We describe a Monte Carlo model that simulates dust migration in a porous cometary nucleus. We present computations for media in which the pore-size distributions are either random or… (More)
NBTI has been extensively studied to understand physics of degradation in recent years. However, little has been done to find out the lifetime distributions of NBTI at both transistor and product… (More)