Class
NumCosmoHaloBiasTinker
Description [src]
class NumCosmo.HaloBiasTinker : NumCosmo.HaloBias
{
/* No available fields */
}Tinker halo bias function type.
Object implementation to compute the halo bias function given the Tinker mass function. A description of the mechanism is given below. Check nc_halo_bias.c for a description of halo biases and nc_multiplicity_func_tinker.c for the Tinker mass function.
The Tinker bias was obtained empirically and is given by \begin{align} b(\nu) &= 1 - A \frac{\nu^a}{\nu^a + \delta_c^a} + B \nu^b + C \nu^c , \end{align} where $b(\nu)$ is the Tinker bias, $\delta_c$ is the critical threshold, $\nu = \frac{\delta_c}{\sigma}$ and the free parameters $(A,a,B,b,C,c)$ depend on the value of the overdensity chosen.
The user must provide input the values: NcHaloMassFunction, delta_c, B, b and c delta_c - nc_halo_bias_ps_new_full().
Instance methods
nc_halo_bias_tinker_set_delta_c
Sets the value delta_c to the NcHaloBiasTinker:critical-delta property.
Methods inherited from NcHaloBias (3)
nc_halo_bias_eval
Computes the Halo Bias at a given redshift.
nc_halo_bias_free
Atomically decrements the reference count of bias by one. If the reference count drops to 0,
all memory allocated by bias is released.
nc_halo_bias_integrand
This function is the integrand of the mean bias, i.e., the product of the mass function with the bias function. As both functions depend on the standard deviation of the matter density contrast, we implement this function to compute \f$ \sigma (M, z) \f$ just once.
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.