hmf
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hmf.cosmology.cosmo
hmf.cosmology.growth_factor
hmf.density_field.transfer
hmf.density_field.transfer_models
hmf.density_field.halofit
hmf.density_field.filters
hmf.halos.mass_definitions
hmf.mass_function.hmf
hmf.mass_function.fitting_functions
hmf.mass_function.integrate_hmf
hmf.alternatives.wdm
hmf.alternatives.wdm.Bode01
hmf.alternatives.wdm.Bode01.__init__
hmf.alternatives.wdm.Bode01.get_models
hmf.alternatives.wdm.Bode01.transfer
hmf.alternatives.wdm.Bode01.lam_eff_fs
hmf.alternatives.wdm.Bode01.lam_hm
hmf.alternatives.wdm.Bode01.m_fs
hmf.alternatives.wdm.Bode01.m_hm
hmf.alternatives.wdm.Lovell14
hmf.alternatives.wdm.MassFunctionWDM
hmf.alternatives.wdm.Schneider12
hmf.alternatives.wdm.Schneider12_vCDM
hmf.alternatives.wdm.TransferWDM
hmf.alternatives.wdm.Viel05
hmf.alternatives.wdm.WDM
hmf.alternatives.wdm.WDMRecalibrateMF
hmf.helpers.sample
hmf.helpers.functional
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hmf.alternatives.wdm.Bode01
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hmf.alternatives.wdm.Bode01.__init__
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hmf.alternatives.wdm.Bode01.__init__
¶
Bode01.
__init__
(
mx
,
cosmo=FlatLambdaCDM(name="Planck15"
,
H0=67.7
km
/
(Mpc
s)
,
Om0=0.307
,
Tcmb0=2.725
K
,
Neff=3.05
,
m_nu=[0.
0.
0.06]
eV
,
Ob0=0.0486)
,
z=0
,
**model_params
)
¶
Initialize self. See help(type(self)) for accurate signature.
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