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2nd International Conference On Astronomy, Astrophysics & Astrobiology
Auckland, New ZealandEvolution of stress distributions in piles
In the early stage of the pile formation, the stress distribution beneath the piles have been affected by the kinetic energy of the granular flow and the granular impact by the granular feeding in the present calculation. We compared the calculated stress distributions of which the granular velocities beneath the piles were less than 1 mm/s with the experimental results of Ai.et al. The effect of the kinetic energy and the granular impact of the granular velocity less than 1 mm/s were negligibly small in the present stress distributions.
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