Source code for camb.dark_energy

from .baseconfig import F2003Class, fortran_class, numpy_1d, CAMBError, np, \
    AllocatableArrayDouble, f_pointer
from ctypes import c_int, c_double, byref, POINTER, c_bool


[docs]class DarkEnergyModel(F2003Class): """ Abstract base class for dark energy model implementations. """ _fields_ = [ ("__is_cosmological_constant", c_bool), ("__num_perturb_equations", c_int)] def validate_params(self): return True
[docs]class DarkEnergyEqnOfState(DarkEnergyModel): """ Abstract base class for models using w and wa parameterization with use w(a) = w + (1-a)*wa parameterization, or call set_w_a_table to set another tabulated w(a). If tabulated w(a) is used, w and wa are set to approximate values at z=0. See :meth:`.model.CAMBparams.set_initial_power_function` for a convenience constructor function to set a general interpolated P(k) model from a python function. """ _fortran_class_module_ = 'DarkEnergyInterface' _fortran_class_name_ = 'TDarkEnergyEqnOfState' _fields_ = [ ("w", c_double, "w(0)"), ("wa", c_double, "-dw/da(0)"), ("cs2", c_double, "fluid rest-frame sound speed squared"), ("use_tabulated_w", c_bool, "using an interpolated tabulated w(a) rather than w, wa above"), ("__no_perturbations", c_bool, "turn off perturbations (unphysical, so hidden in Python)") ] _methods_ = [('SetWTable', [numpy_1d, numpy_1d, POINTER(c_int)])]
[docs] def set_params(self, w=-1.0, wa=0, cs2=1.0): """ Set the parameters so that P(a)/rho(a) = w(a) = w + (1-a)*wa :param w: w(0) :param wa: -dw/da(0) :param cs2: fluid rest-frame sound speed squared """ self.w = w self.wa = wa self.cs2 = cs2 self.validate_params()
def validate_params(self): if not self.use_tabulated_w and self.wa + self.w > 0: raise CAMBError('dark energy model has w + wa > 0, giving w>0 at high redshift')
[docs] def set_w_a_table(self, a, w): """ Set w(a) from numerical values (used as cublic spline). Note this is quite slow. :param a: array of scale factors :param w: array of w(a) :return: self """ if len(a) != len(w): raise ValueError('Dark energy w(a) table non-equal sized arrays') if not np.isclose(a[-1], 1): raise ValueError('Dark energy w(a) arrays must end at a=1') self.f_SetWTable(a, w, byref(c_int(len(a)))) return self
[docs]@fortran_class class DarkEnergyFluid(DarkEnergyEqnOfState): """ Class implementing the w, wa or splined w(a) parameterization using the constant sound-speed single fluid model (as for single-field quintessense). """ _fortran_class_module_ = 'DarkEnergyFluid' _fortran_class_name_ = 'TDarkEnergyFluid' def validate_params(self): super().validate_params() if not self.use_tabulated_w: if self.wa and (self.w < -1 - 1e-6 or 1 + self.w + self.wa < - 1e-6): raise CAMBError('fluid dark energy model does not support w crossing -1')
[docs]@fortran_class class DarkEnergyPPF(DarkEnergyEqnOfState): """ Class implementating the w, wa or splined w(a) parameterization in the PPF perturbation approximation (`arXiv:0808.3125 <https://arxiv.org/abs/0808.3125>`_) Use inherited methods to set parameters or interpolation table. """ # cannot declare c_Gamma_ppf directly here as have not defined all fields in DarkEnergyEqnOfState (TCubicSpline) _fortran_class_module_ = 'DarkEnergyPPF' _fortran_class_name_ = 'TDarkEnergyPPF'
[docs]@fortran_class class AxionEffectiveFluid(DarkEnergyModel): """ Example implementation of a specifc (early) dark energy fluid model (`arXiv:1806.10608 <https://arxiv.org/abs/1806.10608>`_). Not well tested, but should serve to demonstrate how to make your own custom classes. """ _fields_ = [ ("w_n", c_double, "effective equation of state parameter"), ("fde_zc", c_double, "energy density fraction at z=zc"), ("zc", c_double, "decay transition redshift (not same as peak of energy density fraction)"), ("theta_i", c_double, "initial condition field value")] _fortran_class_name_ = 'TAxionEffectiveFluid' _fortran_class_module_ = 'DarkEnergyFluid' def set_params(self, w_n, fde_zc, zc, theta_i=None): self.w_n = w_n self.fde_zc = fde_zc self.zc = zc if theta_i is not None: self.theta_i = theta_i
# base class for scalar field quintessence models
[docs]class Quintessence(DarkEnergyModel): r""" Abstract base class for single scalar field quintessence models. For each model the field value and derivative are stored and splined at sampled scale factor values. To implement a new model, need to define a new derived class in Fortran, defining Vofphi and setting up initial conditions and interpolation tables (see TEarlyQuintessence as example). """ _fields_ = [ ("DebugLevel", c_int), ("astart", c_double), ("integrate_tol", c_double), ("sampled_a", AllocatableArrayDouble), ("phi_a", AllocatableArrayDouble), ("phidot_a", AllocatableArrayDouble), ("__npoints_linear", c_int), ("__npoints_log", c_int), ("__dloga", c_double), ("__da", c_double), ("__log_astart", c_double), ("__max_a_log", c_double), ("__ddphi_a", AllocatableArrayDouble), ("__ddphidot_a", AllocatableArrayDouble), ("__state", f_pointer) ] _fortran_class_module_ = 'Quintessence'
[docs]@fortran_class class EarlyQuintessence(Quintessence): r""" Example early quintessence (axion-like, as arXiv:1908.06995) with potential V(\phi) = m^2f^2 (1 - cos(\phi/f))^2 + \Lambda_{cosmological constant} """ _fields_ = [ ("n", c_double, "power index for potential"), ("f", c_double, r"f/Mpl (sqrt(8\piG)f); only used for initial search value if use_zc is True"), ("m", c_double, "mass parameter in reduced Planck mass units; " "only used for initial search value of use_zc is True"), ("theta_i", c_double, "phi/f initial field value"), ("frac_lambda0", c_double, "fraction of dark energy in cosmologicla constant today (approximated as 1)"), ("use_zc", c_bool, "solve for f, m to get specific critical reshidt zc and fde_zc"), ("zc", c_double, "reshift of peak fractional early dark energy density"), ("fde_zc", c_double, "fraction of early dark energy density to total at peak"), ("npoints", c_int, "number of points for background integration spacing"), ("min_steps_per_osc", c_int, "minimumum number of steps per background oscillation scale"), ("fde", AllocatableArrayDouble, "after initialized, the calculated backgroundearly dark energy " "fractions at sampled_a"), ("__ddfde", AllocatableArrayDouble) ] _fortran_class_name_ = 'TEarlyQuintessence' def set_params(self, n, f=0.05, m=5e-54, theta_i=0.0, use_zc=True, zc=None, fde_zc=None): self.n = n self.f = f self.m = m self.theta_i = theta_i self.use_zc = use_zc if use_zc: if zc is None or fde_zc is None: raise ValueError("must set zc and fde_zc if using use_zc") self.zc = zc self.fde_zc = fde_zc
# short names for models that support w/wa F2003Class._class_names.update({'fluid': DarkEnergyFluid, 'ppf': DarkEnergyPPF})