%0 Journal Article %@holdercode {isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S} %@nexthigherunit 8JMKD3MGPCW/3ESGTTP %@archivingpolicy denypublisher denyfinaldraft24 %@resumeid 8JMKD3MGP5W/3C9JJ5D %@resumeid 8JMKD3MGP5W/3C9JH4A %@resumeid %@resumeid 8JMKD3MGP5W/3C9JHC3 %@usergroup administrator %@usergroup simone %3 extreme event.pdf %X The search for turbulent-like patterns in nonlinear gravitational clustering has recently advanced due to N-body simulations based on the cold dark matter scenario. In this work we present a computational statistical analysis of the formation of galaxy halos by gravitational collapse in N-body simulation from the Virgo Consortium Data. We find that rescaled data points of gravitational energy for different redshifts collapse into similar patterns, well approximated by a Generalized Extreme Value (GEV) distribution. Once similar statistical behavior was found for chaotic advection, this result is discussed in the context of non-dissipative turbulent-like behavior. From our analysis the unstable gravity field itself behaves as a chaotic advecting flow where the particles (galaxies) can be interpreted as turbulent tracers. %@mirrorrepository sid.inpe.br/mtc-m18@80/2008/03.17.15.17.24 %8 Apr. %N 4 %T Extreme event dynamics in the formation of galaxy-sized dark matter structures %@secondarytype PRE PI %K Gravitational clustering, Numerical N-body simulations, Chaotic advection, Galaxies: structure and evolution, Methods: statistical. %@visibility shown %@group LAC-CTE-INPE-MCT-BR %@group LAC-CTE-INPE-MCT-BR %@group %@group LAC-CTE-INPE-MCT-BR %@secondarykey INPE--PRE/ %@secondarymark A_ASTRONOMIA_/_FÍSICA A_CIÊNCIA_DA_COMPUTAÇÃO A_CIÊNCIAS_BIOLÓGICAS_II A_ENGENHARIAS_II A_ENGENHARIAS_III A_ENGENHARIAS_IV A_GEOCIÊNCIAS A_INTERDISCIPLINAR B_QUÍMICA %@issn 0010-4655 %2 sid.inpe.br/mtc-m18@80/2009/06.26.14.57.43 %@affiliation Instituto Nacional de Pesquisas Espaciais (INPE) %@affiliation Instituto Nacional de Pesquisas Espaciais (INPE) %@affiliation %@affiliation Instituto Nacional de Pesquisas Espaciais (INPE) %B Computer Physics Communications %P 621-624 %4 sid.inpe.br/mtc-m18@80/2009/06.26.14.57 %D 2009 %V 180 %@doi 10.1016/j.cpc.2008.11.018 %A Rosa, Reinaldo Roberto, %A Ramos, Fernando Manuel, %A Caretta, C. A., %A Campos Velho, Haroldo Fraga de, %@dissemination WEBSCI %@area COMP