Accurate analytic mass–scale relations for dark matter haloes of all masses and redshifts

Accurate analytic mass–scale relations for dark matter haloes of all masses and redshifts

ABSTRACT CUSP is a powerful formalism that recovers, from first principles and with no free parameter, all the macroscopic properties of dark matter haloes found in cosmological N-body simulations and unveils the origin of their characteristic features. Since it is not restricted by the limitations...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2023-05, Vol.521 (2), p.1988-2001
Hauptverfasser: Salvador-Solé, Eduard, Manrique, Alberto, Canales, David, Botella, Ignacio
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container_end_page 2001
container_issue 2
container_start_page 1988
container_title Monthly notices of the Royal Astronomical Society
container_volume 521
creator Salvador-Solé, Eduard
Manrique, Alberto
Canales, David
Botella, Ignacio
description ABSTRACT CUSP is a powerful formalism that recovers, from first principles and with no free parameter, all the macroscopic properties of dark matter haloes found in cosmological N-body simulations and unveils the origin of their characteristic features. Since it is not restricted by the limitations of simulations, it covers the whole mass and redshift ranges. In the present Paper we use CUSP to calculate the mass–scale relations holding for halo density profiles fitted to the usual NFW and Einasto functions in the most relevant cosmologies and for the most usual mass definitions. We clarify the origin of these relations and provide accurate analytic expressions holding for all masses and redshifts. The performance of those expressions is compared to that of previous models and to the mass–concentration relation spanning more than 20 orders of magnitude in mass at z = 0 obtained in recent simulations of a 100 GeV WIMP universe.
doi_str_mv 10.1093/mnras/stad642
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title Accurate analytic mass–scale relations for dark matter haloes of all masses and redshifts
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