Class
NumCosmoPowspecML
Description [src]
abstract class NumCosmo.PowspecML : NumCosmoMath.Powspec
{
/* No available fields */
}Abstract class for linear matter power spectrum implementation.
This module comprises the set of functions to compute the linear matter power spectrum and derived quantities.
Following the description presented in NcmPowspec, in this case we have that the
field $\delta(\vec{x})$ represents the matter density fluctuations, i.e.,
$$\delta(\vec{x}) = \frac{\rho(\vec{x}) - \bar{\rho}}{\bar{\rho}},$$ where $\rho$ is
the cold matter density field and $\bar{\rho}$ its mean.
Functions
nc_powspec_ml_clear
If ps_ml is different from NULL,
atomically decrements the reference count of ps_ml by one.
If the reference count drops to 0,
all memory allocated by ps_ml is released and ps_ml is set to NULL.
Instance methods
nc_powspec_ml_free
Atomically decrements the reference count of ps_ml by one.
If the reference count drops to 0, all memory allocated by ps_ml is released.
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.