Matches in SemOpenAlex for { <https://semopenalex.org/work/W2143114413> ?p ?o ?g. }
- W2143114413 endingPage "701" @default.
- W2143114413 startingPage "689" @default.
- W2143114413 abstract "We study the mass assembly history (MAH) of dark matter haloes. We compare MAHs obtained using (i) merger trees constructed with the extended Press–Schechter (EPS) formalism, (ii) numerical simulations and (iii) the Lagrangian perturbation code pinocchio. We show that the pinocchio MAHs are in excellent agreement with those obtained using numerical simulations, while the EPS formalism predicts MAHs that occur too late. pinocchio, which is much less CPU intensive than N-body simulation, can be run on a simple personal computer, and does not require any labour intensive post-simulation analysis, therefore provides a unique and powerful tool to investigate the growth history of dark matter haloes. Using a suite of 55 pinocchio simulations, with 2563 particles each, we study the MAHs of 12 924 cold dark matter (CDM) haloes in a ΛCDM concordance cosmology. This is by far the largest set of haloes used for any such analysis. For each MAH we derive four different formation redshifts, which characterize different epochs during the assembly history of a dark matter halo. We show that haloes less massive than the characteristic non-linear mass scale establish their potential wells much before they acquire most of their mass. The time when a halo reaches its maximum virial velocity roughly divides its mass assembly into two phases, a fast-accretion phase which is dominated by major mergers, and a slow-accretion phase dominated by minor mergers. Each halo experiences about 3 ± 2 major mergers since its main progenitor had a mass equal to 1 per cent of the final halo mass. This major merger statistic is found to be virtually independent of halo mass. However, the average redshift at which these major mergers occur is strongly mass dependent, with more massive haloes experiencing their major mergers later." @default.
- W2143114413 created "2016-06-24" @default.
- W2143114413 creator A5002282147 @default.
- W2143114413 creator A5032020402 @default.
- W2143114413 creator A5032581326 @default.
- W2143114413 creator A5034120384 @default.
- W2143114413 date "2007-08-01" @default.
- W2143114413 modified "2023-10-01" @default.
- W2143114413 title "On the assembly history of dark matter haloes" @default.
- W2143114413 cites W1886836907 @default.
- W2143114413 cites W1929623410 @default.
- W2143114413 cites W1963831836 @default.
- W2143114413 cites W1969514664 @default.
- W2143114413 cites W1973215726 @default.
- W2143114413 cites W1973368884 @default.
- W2143114413 cites W1982533357 @default.
- W2143114413 cites W1987041072 @default.
- W2143114413 cites W1994905665 @default.
- W2143114413 cites W1998577648 @default.
- W2143114413 cites W1999367759 @default.
- W2143114413 cites W2001085255 @default.
- W2143114413 cites W2001677179 @default.
- W2143114413 cites W2002142654 @default.
- W2143114413 cites W2003182532 @default.
- W2143114413 cites W2003864863 @default.
- W2143114413 cites W2004976613 @default.
- W2143114413 cites W2014409422 @default.
- W2143114413 cites W2015828000 @default.
- W2143114413 cites W2020868196 @default.
- W2143114413 cites W2023344562 @default.
- W2143114413 cites W2023393371 @default.
- W2143114413 cites W2025786375 @default.
- W2143114413 cites W2026263995 @default.
- W2143114413 cites W2028914745 @default.
- W2143114413 cites W2032925149 @default.
- W2143114413 cites W2039804150 @default.
- W2143114413 cites W2043685494 @default.
- W2143114413 cites W2050469528 @default.
- W2143114413 cites W2057867577 @default.
- W2143114413 cites W2059079076 @default.
- W2143114413 cites W2063919788 @default.
- W2143114413 cites W2065201732 @default.
- W2143114413 cites W2076384560 @default.
- W2143114413 cites W2077351580 @default.
- W2143114413 cites W2079374409 @default.
- W2143114413 cites W2084287642 @default.
- W2143114413 cites W2086963345 @default.
- W2143114413 cites W2091059059 @default.
- W2143114413 cites W2094015484 @default.
- W2143114413 cites W2095338281 @default.
- W2143114413 cites W2100157321 @default.
- W2143114413 cites W2101568531 @default.
- W2143114413 cites W2104006840 @default.
- W2143114413 cites W2113191053 @default.
- W2143114413 cites W2120819856 @default.
- W2143114413 cites W2129124428 @default.
- W2143114413 cites W2131828218 @default.
- W2143114413 cites W2134712793 @default.
- W2143114413 cites W2136147728 @default.
- W2143114413 cites W2148882585 @default.
- W2143114413 cites W2150746633 @default.
- W2143114413 cites W2165386494 @default.
- W2143114413 cites W2171285677 @default.
- W2143114413 cites W2950207807 @default.
- W2143114413 cites W3098042124 @default.
- W2143114413 cites W3098339022 @default.
- W2143114413 cites W3098905467 @default.
- W2143114413 cites W3099084022 @default.
- W2143114413 cites W3100110286 @default.
- W2143114413 cites W3100987559 @default.
- W2143114413 cites W3101849758 @default.
- W2143114413 cites W3102310698 @default.
- W2143114413 cites W3105949757 @default.
- W2143114413 doi "https://doi.org/10.1111/j.1365-2966.2007.11942.x" @default.
- W2143114413 hasPublicationYear "2007" @default.
- W2143114413 type Work @default.
- W2143114413 sameAs 2143114413 @default.
- W2143114413 citedByCount "80" @default.
- W2143114413 countsByYear W21431144132012 @default.
- W2143114413 countsByYear W21431144132013 @default.
- W2143114413 countsByYear W21431144132014 @default.
- W2143114413 countsByYear W21431144132015 @default.
- W2143114413 countsByYear W21431144132016 @default.
- W2143114413 countsByYear W21431144132018 @default.
- W2143114413 countsByYear W21431144132020 @default.
- W2143114413 countsByYear W21431144132021 @default.
- W2143114413 countsByYear W21431144132022 @default.
- W2143114413 countsByYear W21431144132023 @default.
- W2143114413 crossrefType "journal-article" @default.
- W2143114413 hasAuthorship W2143114413A5002282147 @default.
- W2143114413 hasAuthorship W2143114413A5032020402 @default.
- W2143114413 hasAuthorship W2143114413A5032581326 @default.
- W2143114413 hasAuthorship W2143114413A5034120384 @default.
- W2143114413 hasBestOaLocation W21431144132 @default.
- W2143114413 hasConcept C121332964 @default.
- W2143114413 hasConcept C126320844 @default.
- W2143114413 hasConcept C1276947 @default.
- W2143114413 hasConcept C142362112 @default.