Article
Open Access
Formation and dynamics of Saturn and its disk simulated by using a new N-body model
-
A. Pavlov
and
Y. Pavlova
Published/Copyright:
December 1, 2003
Published Online: 2003-12-1
Published in Print: 2003-12-1
© 2003 Versita Warsaw
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- Two models of quantum random walk
- Sezawa and love modes in Co/Cu superlattices
- The dynamics of multiparticle collisions in motion of a granular material
- A boson approach to the structure of A=22 nuclei
- Surface morphology of PrBa2Cu3O7-δ single crystals after the long-lasting high-temperature reduction
- Formation and dynamics of Saturn and its disk simulated by using a new N-body model
- Positron annihilation study for cadmium (electronic structure and enhancement effect)
- Centrifugal (centripetal) and Coriolis' velocities and accelerations in $$ (\bar L_n ,g) $$ -spaces
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Keywords for this article
N-body model;
gravitation;
planets;
Saturn's rings;
computer simulation;
95.10;
96.60;
97.00;
98.10
Creative Commons
BY-NC-ND 3.0
Articles in the same Issue
- Two models of quantum random walk
- Sezawa and love modes in Co/Cu superlattices
- The dynamics of multiparticle collisions in motion of a granular material
- A boson approach to the structure of A=22 nuclei
- Surface morphology of PrBa2Cu3O7-δ single crystals after the long-lasting high-temperature reduction
- Formation and dynamics of Saturn and its disk simulated by using a new N-body model
- Positron annihilation study for cadmium (electronic structure and enhancement effect)
- Centrifugal (centripetal) and Coriolis' velocities and accelerations in $$ (\bar L_n ,g) $$ -spaces
- On entanglement distillation and quantum error correction for unknown states and channels
- High power self-controled volume discharge based molecular lasers
