Abstract
We have developed a framework within which the probability density for the occurrence of structures within a random field may be assessed. This framework is rather general, but we have used it mainly in the context of the large scale structure of the Universe, where the most relevant structures are: voids, galaxy clusters, filaments and laminae.
We have also considered the probability densities of structures in point distributions, starting with the Poissonian case and generalizing the results founds in this case to a general distribution. The comparison, in the high density limit, with the appropriate continuous random field renders several useful results.
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© 1997 Springer Science+Business Media New York
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Betancort-Rijo, J.E. (1997). Structures in Random Fields. In: Babu, G.J., Feigelson, E.D. (eds) Statistical Challenges in Modern Astronomy II. Springer, New York, NY. https://doi.org/10.1007/978-1-4612-1968-2_26
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DOI: https://doi.org/10.1007/978-1-4612-1968-2_26
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