Collisional theory of non-identical particles in a gravitational field

DOI10.1007/BF00058906zbMath0591.70014MaRDI QIDQ1075074

K. A. Hämeen-Anttila

Publication date: 1984

Published in: Earth, Moon, and Planets (Search for Journal in Brave)

zbMATH Keywords

gravitational fieldfirst-order differential equationsequilibrium statespartially elastic collisionscentral bodyapproximate potential for an axially symmetric disc around aapproximate potential for an axially symmetric disc around a central bodycomputer simulations of Keplerian systemsnon-identical particlesplanetesimals

Mathematics Subject Classification ID

Celestial mechanics (70F15) Statistical astronomy (85A35)

Related Items (3)

Turbulence in circumstellar discs ⋮ Collisional evolution of rotating, non-identical particles ⋮ Generalized theory of impacts in particulate systems

Cites Work

• An improved and generalized theory for the collisional evolution of Keplerian systems
• Collisions in self-gravitating clouds of planetesimals
• Starn's rings and bimodality of Keplerian systems

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