CINECA IRIS Institutial research information system (University of Pisa) · 2011 · 20 citations · 0 references
Natural SciencesEarth SciencesPhysicsAstrophysicsPlanetary GeologyPlanetary GeophysicsAsteroid DynamicsAstrophysical SimulationsComputational AstrophysicsGeodynamic ModelingOrbital DynamicsThrust BeltsAsteroid Family DynamicsAsteroid Orbital EvolutionAsteroid Pair DynamicsCollisional EvolutionMain Belt AsteroidsMain-belt Asteroid DynamicsNumerical Modeling Of Thrust Belts
We have adapted the planet building code, a multizone code, to study the collisional evolution of asteroids in the main belt. In this way the effects of resonances and Yarkowski's drift are statistically included and we can estimate the flux of bodies into NEO orbits.