Conditional calculus on fractal structures and its application to galaxy distribution

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dc.creatorShi, Yu
dc.date1996-12-23
dc.date1997-01-01
dc.date.accessioned2026-07-07T09:02:04Z
dc.date.available2026-07-07T09:02:04Z
dc.descriptionIt is shown that calculus can apply on a fractal structure with the condition that the infinitesimal limit of change of the variable is larger than the lower cut-off of the fractal structure, and an assumption called local decomposability. As an application, it is shown that the angular projection of a fractal distribution in 3-dimensional space is not homogeneous at sufficiently large angles. Therefore the angular projection of galaxy distribution for sufficiently large angles can discriminate the fractal and the homogeneity pictures.
dc.descriptionLatex, 1 figure included
dc.identifierhttps://arxiv.org/abs/astro-ph/9612227
dc.identifierhttp://arxiv.org/abs/astro-ph/9612227
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/148501
dc.subjectAstrophysics
dc.subjectCondensed Matter
dc.titleConditional calculus on fractal structures and its application to galaxy distribution
dc.typetext

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