Geodesic
Simulation of planet formation in circumstellar disks
Numerical methods and programming, Tome 13 (2012) no. 3, pp. 443-451.

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A numerical model of dynamics for a massive self-gravitating protoplanetary is proposed with consideration of inelastic pair collisions of particles. In the conducted computing experiments with ring structures in a disk, it is shown that the mass range change of particles occurs with the reproduction of the ring structure. It is found that the released thermal energy in bodies is maximal for bodies of small mass.
Keywords: self-gravitating circumstellar disk; particle-in-cell method; direct modeling method; formation of planetary embryos. 
@article{VMP_2012_13_3_a9,
     author = {T. V. Markelova and V. N. Snytnikov},
     title = {Simulation of planet formation in circumstellar disks},
     journal = {Numerical methods and programming},
     pages = {443--451},
     publisher = {mathdoc},
     volume = {13},
     number = {3},
     year = {2012},
     language = {ru},
     url = {http://geodesic.mathdoc.fr/item/VMP_2012_13_3_a9/}
}
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T. V. Markelova; V. N. Snytnikov. Simulation of planet formation in circumstellar disks. Numerical methods and programming, Tome 13 (2012) no. 3, pp. 443-451. http://geodesic.mathdoc.fr/item/VMP_2012_13_3_a9/