halomod.concentration.Ludlow16

class halomod.concentration.Ludlow16(cosmo: ~hmf.cosmology.cosmo.Cosmology = <hmf.cosmology.cosmo.Cosmology object>, filter0: ~hmf.density_field.filters.Filter | None = None, growth: ~hmf.cosmology.growth_factor.GrowthFactor | None = None, delta_c: float = 1.686, profile: ~halomod.profiles.Profile | None = None, mdef: ~hmf.halos.mass_definitions.MassDefinition | None = None, **model_parameters)

Bases: CMRelation

Analytical Concentration-Mass relation of Ludlow et al.(2016) [1].

See documentation for Bias for information on input parameters. This model has two model parameters.

Notes

Note

The form of the concentration is described by eq(6) and eq(7) in [1].

Parameters:

• f (float) – Default value is f=0.02 and C=650

• C (float) – Default value is f=0.02 and C=650

References

[1] (1,2)

Ludlow, A. D. et al., “The mass-concentration-redshift relation of cold and warm dark matter haloes “, https://ui.adsabs.harvard.edu/abs/2016MNRAS.460.1214L.

cm(m, z=0)

Return concentration parameter for mass m at z.

Parameters:

• z (float) – Redshift. Must not be an array.

• m (float) – Halo Mass.

delta_halo(z=0)

classmethod get_models() → Dict[str, Type]

Get a dictionary of all implemented models for this component.

mass_nonlinear(z)

Return the nonlinear mass at z.

Parameters:

z (float) – Redshift. Must not be an array.

native_mdefs = (<hmf.halos.mass_definitions.SOCritical object>,)