A deeper look into the structure of CDM haloes

Correlations between halo parameters from Einasto fits

Silviu M. Udrescu, Aaron A. Dutton, Andrea Maccio, Tobias Buck

    Research output: Contribution to journalArticle

    Abstract

    We used high resolution dark matter only cosmological simulations to investigate the structural properties of Lambda Cold Dark Matter (CDM) haloes over cosmic time. The haloes in our study range in mass from ∼1010 to ∼1012 M, and are resolved with 105 to 107 particles. We fit the spherically averaged density profiles of DM haloes with the three parameter Einasto function. For our sample of haloes, the Einasto shape parameter, α, is uncorrelated with the concentration, c, at fixed halo mass, and at all redshifts. Previous reports of an anticorrelation are traced to fitting degeneracies, which our fits are less sensitive to due to our higher spatial resolution. However, for individual haloes the evolution in α and c is anticorrelated: at redshift z = 7, α 0.4 and decreases with time, while c 3 and increases with time. The evolution in structure is primarily due to accretion of mass at larger radii. We suggest that α traces the evolutionary state of the halo, with dynamically young haloes having high α (closer to a top-hat: α−1 = 0), and dynamically relaxed haloes having low α (closer to isothermal: α = 0). Such an evolutionary dependence reconciles the increase of α versus peak height, ν, with the dependence on the slope of the power spectrum of initial density fluctuations found by previous studies.

    Original languageEnglish (US)
    Pages (from-to)5259-5267
    Number of pages9
    JournalMonthly Notices of the Royal Astronomical Society
    Volume482
    Issue number4
    DOIs
    StatePublished - Feb 1 2019

    Fingerprint

    halos
    dark matter
    spatial resolution
    accretion
    simulation
    cold
    parameter
    high resolution
    power spectra
    slopes
    radii
    profiles
    young
    particle

    Keywords

    • Cosmology: theory
    • Dark matter
    • Galaxies: formation
    • Galaxies: structure
    • Methods: numerical

    ASJC Scopus subject areas

    • Astronomy and Astrophysics
    • Space and Planetary Science

    Cite this

    A deeper look into the structure of CDM haloes : Correlations between halo parameters from Einasto fits. / Udrescu, Silviu M.; Dutton, Aaron A.; Maccio, Andrea; Buck, Tobias.

    In: Monthly Notices of the Royal Astronomical Society, Vol. 482, No. 4, 01.02.2019, p. 5259-5267.

    Research output: Contribution to journalArticle

    Udrescu, Silviu M. ; Dutton, Aaron A. ; Maccio, Andrea ; Buck, Tobias. / A deeper look into the structure of CDM haloes : Correlations between halo parameters from Einasto fits. In: Monthly Notices of the Royal Astronomical Society. 2019 ; Vol. 482, No. 4. pp. 5259-5267.
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