High-Performance Computing of Self-Gravity for Small Solar System Bodies.
To study the evolution of small solar system bodies like asteroids and comets, a fast method is needed to compute the self-gravity of systems composed of millions of particles. A proposed fully parallel shared-memory algorithm for dense, self-gravitating agglomerates scales efficiently with the numb...
| Publicado en: | Computer (00189162) Vol. 47; no. 9; pp. 34 - 40 |
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| Autores principales: | , , |
| Formato: | Artículo |
| Publicado: |
IEEE
Sep2014
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| Materias: | |
| Acceso en línea: | Ver este registro en EBSCOhost |
| Sumario: | To study the evolution of small solar system bodies like asteroids and comets, a fast method is needed to compute the self-gravity of systems composed of millions of particles. A proposed fully parallel shared-memory algorithm for dense, self-gravitating agglomerates scales efficiently with the number of particles as well as the number of computational resources. |
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