GenMFGrowth¶
- class hmf.core.growth_models.GenMFGrowth(*, a_min=1e-08, dln_a=0.01)[source]¶
The growth factor of the
genmfcode (Reed et al. 2007).Exact for a flat universe with a cosmological constant, or an open universe without one, and no radiation. For other LambdaCDM cosmologies with Lambda and non-negative curvature it uses the flat formula, as an approximation. The growth rate is the derivative of the spline of ln D.
- Parameters:
Attributes
- alias: ClassVar[str | None] = 'GenMF'¶
The short name the model is registered under, if any. Set by the
aliasclass keyword; never inherited.
- backend: ClassVar[str | None] = None¶
The Boltzmann code that computes the model (
"camb"or"class"), if any.
- calibration_domain: ClassVar[Domain | None] = None¶
Where the model was calibrated, if that is stated by its source.
- parameter_source: ClassVar[str] = ''¶
The exact source (paper, version, table or equation) of the parameter defaults, e.g. “Tinker et al. 2008, ApJ 688, 709 (published), Table 2”.
- references: ClassVar[tuple[str, ...]] = ('Reed, D. S., et al., 2007. MNRAS 374, 2. https://doi.org/10.1111/j.1365-2966.2006.11204.x',)¶
References to cite when the model is used, each a formatted citation.
- valid_domain: ClassVar[Domain] = Domain(bounds=(('z', Interval(lower=0.0, upper=inf, unit=None, lower_open=False, upper_open=True)),), source='z >= 0.')¶
z >= 0. The
Growthstage checks z against the model’s class’s domain (so a model can narrow it), and also against the redshifts its solution covers (up toGrowthSolution.z_max, e.g. a table’s largest redshift): growth is never extrapolated.- Type:
Where the model can be evaluated
Methods
- check_cosmology(cosmology: FLRW) None[source]¶
Raise unless the cosmology is a flat or open LambdaCDM.
- classmethod coerce(value: object) Self¶
Convert a value to a model of this kind: the converter of a model field.
- Parameters:
value – An instance of
cls, which is returned as it is; or a name, import path or class thatget()accepts, which is looked up and instantiated with its default parameters.- Returns:
An instance of
cls.- Return type:
- Raises:
ModelNotFoundError – If
valueis a name that no model of this kind is known by.TypeError – If
valueis of any other type, or names a class that is not a concrete subclass ofcls.
Examples
>>> from hmf.core.filters import Filter, TopHat >>> Filter.coerce("TopHat") == TopHat() True
- classmethod fields_info() tuple[FieldInfo, ...]¶
Describe this class’s fields, without creating an instance.
- Returns:
The name, type, default and documentation of each field.
- Return type:
tuple of FieldInfo
- classmethod get(name: str | type[Model]) type[Self]¶
Look up a model of this kind.
- Parameters:
name – An alias (
"Tinker08"), a qualified name ("hmf.core.fits:Tinker08"), an import path to a class not yet imported ("pkg.mod:Cls"or"pkg.mod.Cls"), or a class.- Returns:
The model class (not an instance). It is always a subclass of
cls.- Return type:
- Raises:
ModelNotFoundError – If no model of this kind is known by
name, even after loading thehmf.modelsentry points and tryingnameas an import path.TypeError – If
nameresolves to something that is not a concrete subclass ofcls.
- classmethod get_aliases() Mapping[str, str]¶
Return a read-only mapping from alias to qualified name, for this kind.
- classmethod get_models() Mapping[str, type[Self]]¶
Return the registered models of this kind, by qualified name.
Plugins advertised in the
hmf.modelsentry-point group are loaded first.- Returns:
A read-only mapping from qualified name to class. Called on a kind, it is a live view of the registry. Called on a non-kind subclass, it holds only the models that subclass it.
- Return type:
Mapping
- solve(cosmology: FLRW, *, run: BoltzmannRun | None = None, disk_cache: DiskCache | None = None, k_accuracy: KAccuracy = KAccuracy(dln_k=0.02, ln_k_min=-18.420680743952367, k_max_r_min=20.0)) GrowthSolution¶
Compute the growth (see
GrowthModel.solve()).