Force Evaluation in Particle Methods for Self-Gravitating Multi-Phase Systems

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dc.creatorCapuzzo-Dolcetta, R.
dc.creatorDi Lisio, R.
dc.creatorMiocchi, P.
dc.date1996-12-12
dc.date.accessioned2026-07-07T02:22:33Z
dc.date.available2026-07-07T02:22:33Z
dc.descriptionA modern approach to the evolution of a mixed (stars and gas) self-gravitating system is the fully Lagrangian particle approach. The gaseous (particle) phase differs from the compact because the mutual force is given by the sum of gravity and pressure gradient. In this note we report of some characteristics, advantages and limitations of this approach for what regards the evaluation of forces in the system. In particular, a comparison between classic tree-code and fast multipole algorithm to evaluate gravitational forces is discussed.
dc.description5 pages + 1 postscript figure; to be published in the Proceedings of the XII Italian Conference on Gen. Rel. and Grav. Phys., Roma, sep. 23-27 1996
dc.identifierhttps://arxiv.org/abs/astro-ph/9612124
dc.identifierhttp://arxiv.org/abs/astro-ph/9612124
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10917
dc.subjectAstrophysics
dc.titleForce Evaluation in Particle Methods for Self-Gravitating Multi-Phase Systems
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