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Titolo:
Small deviations from Gaussianity and the galaxy cluster abundance evolution
Autore:
Ribeiro, ALB; Wuensche, CA; Letelier, PS;
Indirizzi:
Univ Estadual Campinas, IMECC, Dept Matemat Aplicada, BR-13083970 Campinas, SP, Brazil Univ Estadual Campinas Campinas SP Brazil BR-13083970 BCpinas, SP, Brazil INPE, Div Astrofis, BR-12201970 Sao Paulo, Brazil INPE Sao Paulo Brazil BR-12201970 BCrofis, BR-12201970 Sao Paulo, Brazil
Titolo Testata:
ASTROPHYSICAL JOURNAL
fascicolo: 1, volume: 539, anno: 2000,
parte:, 1
pagine: 1 - 4
SICI:
0004-637X(20000810)539:1<1:SDFGAT>2.0.ZU;2-6
Fonte:
ISI
Lingua:
ENG
Soggetto:
STATISTICS; FLUCTUATIONS; MODEL;
Keywords:
cosmology : theory; galaxies : clusters : general; large-scale structure of universe;
Tipo documento:
Article
Natura:
Periodico
Settore Disciplinare:
Physical, Chemical & Earth Sciences
Citazioni:
26
Recensione:
Indirizzi per estratti:
Indirizzo: Ribeiro, ALB Univ Estadual Campinas, IMECC, Dept Matemat Aplicada, BR-13083970 Campinas, SP, Brazil Univ Estadual Campinas Campinas SP Brazil BR-13083970 BCazil
Citazione:
A.L.B. Ribeiro et al., "Small deviations from Gaussianity and the galaxy cluster abundance evolution", ASTROPHYS J, 539(1), 2000, pp. 1-4

Abstract

In this paper, we raise the hypothesis that the density fluctuation held, which originates the growth of large-scale structures, is a combination of two or more distributions, instead of assuming that the observed distribution of matter stems from a single Gaussian held produced in the very early universe, as is widely accepted. By applying the statistical analysis of finite-mixture distributions to a specific combination of Gaussian plus non-Gaussian random fields, we studied the case in which just a small departure from Gaussianity is allowed. Our results suggest that even a very small level of non-Gaussianity may introduce significant changes in the cluster abundance evolution rate.

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Documento generato il 19/05/13 alle ore 11:17:44