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Local angular fractal and galaxy distribution

1996/12/23 by Yu Shi, Shi, Yu
Biochemistry, Genetics and Molecular Biology · Physics and Astronomy · #Fractal and DNA sequence analysis #Scientific Research and Discoveries #Advanced Mathematical Theories and Applications

paper · pdf · doi:10.48550/arxiv.astro-ph/9612225

Abstract

The power-law dependence of the angle in the angular projection of galaxy distribution is explained by assuming that in the spherical shells within a small angle the distributions are also fractal. If this local angular fractal is possessed, a fractal structure is angularly-isotropic at each occupied point though inhomogeneous, and is compatible with the present evidence claimed to be of homogeneity for galaxy distribution. Further, it is most likely to be isotropic rather than only angularly-isotropic. Several related issues are discussed.

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