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- W2002754310 abstract "We derived the stationary distribution of the mass of planetesimals from the coagulation equation under the assumption of energy equipartition. In the three-dimensional case, we found that the stationary solution is expressed as n(m)∝m−83, where n is the surface number density and m is the mass of the planetesimals. This solution is in excellent agreement with the result of direct N-body simulations and the numerical integration of the coagulation equation, for the range of mass which contains most of the total mass of the planetesimals (1022–1025 g). In the two-dimensional case, the stationary solution exists but cannot be realized in a finite time. This difference is the direct consequence of the fact that runaway growth takes place in three dimensions, but not in two dimensions." @default.
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- W2002754310 date "1998-11-01" @default.
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- W2002754310 title "On the mass distribution of planetesimals in the early runaway stage" @default.
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- W2002754310 doi "https://doi.org/10.1016/s1384-1076(98)00021-9" @default.
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