Some Statistics for Measuring Large-Scale Structure

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dc.creatorBrandenberger, Robert H.
dc.creatorKaplan, David M.
dc.creatorA, Stephen
dc.creatorRamsey
dc.date1993-10-03
dc.date.accessioned2026-07-07T02:18:54Z
dc.date.available2026-07-07T02:18:54Z
dc.descriptionGood statistics for measuring large-scale structure in the Universe must be able to distinguish between different models of structure formation. In this paper, two and three dimensional ``counts in cell" statistics and a new ``discrete genus statistic" are applied to toy versions of several popular theories of structure formation: random phase cold dark matter model, cosmic string models, and global texture scenario. All three statistics appear quite promising in terms of differentiating between the models.
dc.descriptionBROWN-HET-922 (August 1993), 13 pages, 5 figures (available from the authors), uses PHYZZX
dc.identifierhttps://arxiv.org/abs/astro-ph/9310004
dc.identifierhttp://arxiv.org/abs/astro-ph/9310004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9666
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleSome Statistics for Measuring Large-Scale Structure
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