Class
NumCosmoPowspecMNLHaloFit
Description [src]
class NumCosmo.PowspecMNLHaloFit : NumCosmo.PowspecMNL
{
/* No available fields */
}Nonlinear matter power spectrum from Halofit model.
Provides the nonlinear matter power spectrum using Halofit model [Smith et al (2003)][XSmith2003] and [Takahashi et al. (2012)][XTakahashi2012].
For PKEqual see [Casarini et al. (2009)][XCasarini2009] and [Casarini et al. (2016)][XCasarini2016].
Instance methods
nc_powspec_mnl_halofit_pkequal
Whether to use PKEqual to adjust the HaloFit formula when using a NcHICosmoDECpl
model, see [Casarini et al. (2009)][XCasarini2009] and [Casarini et al. (2016)][XCasarini2016].
nc_powspec_mnl_halofit_set_kbounds_from_ml
Sets mode $k$ boundaries from the linear matter power spectrum.
Methods inherited from NcPowspecMNL (2)
nc_powspec_mnl_free
Atomically decrements the reference count of ps_mnl by one.
If the reference count drops to 0, all memory allocated by ps_mnl is released.
nc_powspec_mnl_ref
Increases the reference count of ps_mnl by one atomically.
Methods inherited from NcmPowspec (29)
Please see NcmPowspec for a full list of methods.
Properties
Properties inherited from NcmPowspec (5)
NumCosmoMath.Powspec:kmax
The maximum mode (wave-number) value to compute $P(k,z)$.
NumCosmoMath.Powspec:kmin
The minimum mode (wave-number) value to compute $P(k,z)$.
NumCosmoMath.Powspec:reltol
The relative tolerance on the interpolation error.
NumCosmoMath.Powspec:zf
The final time (redshift) to compute $P(k,z)$.
NumCosmoMath.Powspec:zi
The initial time (redshift) to compute $P(k,z)$.
Signals
Signals inherited from GObject (1)
GObject::notify
The notify signal is emitted on an object when one of its properties has its value set through g_object_set_property(), g_object_set(), et al.