On the statistics of the gravitational field

dc.creatorDel Popolo, A.
dc.date2001-10-26
dc.date.accessioned2026-07-07T02:01:01Z
dc.date.available2026-07-07T02:01:01Z
dc.descriptionIn this paper we extend Chandrasekhar and von Neumann's analysis of the statistics of the gravitational field to systems in which particles (e.g. stars, galaxies) are not homogeneously distributed. We derive a distribution function W(F,d F/dt) giving the joint probability that a test particle is subject to a force F and an associated rate of change of F given by d F/dt. We calculate the first moment of d F/dt to study the effects of inhomogenity on dynamical friction.
dc.description2 pages; Proceedings of the international conference "Statistical Challenges in Modern Astronomy III", July 18-21, 2001, The Pennsylvania State University, State College, Pennsylvania, Usa
dc.identifierhttps://arxiv.org/abs/astro-ph/0110580
dc.identifierhttp://arxiv.org/abs/astro-ph/0110580
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3608
dc.subjectAstrophysics
dc.titleOn the statistics of the gravitational field
dc.typetext

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