borg_public/libLSS/physics/cosmo.hpp

197 lines
5.9 KiB
C++
Raw Normal View History

2023-05-29 10:41:03 +02:00
/*+
ARES/HADES/BORG Package -- ./libLSS/physics/cosmo.hpp
Copyright (C) 2014-2020 Guilhem Lavaux <guilhem.lavaux@iap.fr>
Copyright (C) 2009-2020 Jens Jasche <jens.jasche@fysik.su.se>
Additional contributions from:
Guilhem Lavaux <guilhem.lavaux@iap.fr> (2023)
+*/
#ifndef __LIBLSS_COSMO_HPP
#define __LIBLSS_COSMO_HPP
#include <string>
#include <functional>
#include <CosmoTool/hdf5_array.hpp>
#include "libLSS/tools/bisection.hpp"
#include "libLSS/tools/auto_interpolator.hpp"
namespace LibLSS {
struct CosmologicalParameters {
double omega_r; /* negligible radiation density */
double omega_k; /* curvature - flat prior for everything! */
double omega_m;
double omega_b;
double omega_q;
double w;
double n_s;
double fnl; /* non-linearity parameter, for primordial non-Gaussianity */
double wprime;
double sigma8;
double rsmooth;
double h;
double beta;
double z0;
double a0; /* scale factor at epoch of observation usually 1*/
double sum_mnu; /* sum of neutrino masses */
CosmologicalParameters()
: omega_r(0), omega_k(0), omega_m(0), omega_b(0), omega_q(0), w(0),
n_s(0), fnl(0), wprime(0), sigma8(0), h(0), beta(0), z0(0), a0(0),
sum_mnu(0) {}
bool operator==(CosmologicalParameters const &p2) const {
return omega_r == p2.omega_r && omega_k == p2.omega_k &&
omega_m == p2.omega_m && omega_b == p2.omega_b &&
omega_q == p2.omega_q && w == p2.w && n_s == p2.n_s &&
wprime == p2.wprime && sigma8 == p2.sigma8 && h == p2.h &&
sum_mnu == p2.sum_mnu;
}
bool operator!=(CosmologicalParameters const &p2) const {
return !operator==(p2);
}
};
static const double A_MIN = 0.;
static const double A_MAX = 30000.;
static const double COSMO_EPS = 1e-6;
#define LIBLSS_COSMOLOGY_INVERSE_FUNCTION( \
TARGET, ORIGINAL, RANGE_MIN, RANGE_MAX) \
double TARGET(double X) const { \
return bisection( \
RANGE_MIN, RANGE_MAX, 1e-6, X, \
std::bind(&Cosmology::ORIGINAL, this, std::placeholders::_1)); \
}
class Cosmology {
private:
CosmologicalParameters parameters;
double A_spec; /* Normalization of the power spectrum */
int spec_type; /* indicates which power spectrum is currently used, and whether the normalization has to be reevaluated*/
double norm_d_plus;
double aux_d_plus(double a, double *result_d_plus_prime = 0) const;
std::shared_ptr<auto_interpolator<double>> pre_com2a, pre_dplus,
pre_dplus_prime;
public:
Cosmology(const CosmologicalParameters &parameters);
void precompute_com2a();
void precompute_d_plus();
CosmologicalParameters const &getParameters() const { return parameters; }
double a2z(double a) const { return 1 / a - 1; }
double z2a(double z) const { return 1 / (1 + z); }
double d_plus(double a) const { return aux_d_plus(a) / norm_d_plus; }
double d2dlum(double z, double d) const { return (1 + z) * d; }
double dlum2d(double z, double dlum) const { return dlum / (1 + z); }
double g_plus(double a) const {
double d_plus, d_plus_prime;
d_plus = aux_d_plus(a, &d_plus_prime);
return (a > COSMO_EPS) ? (a / d_plus * d_plus_prime) : 1.0;
}
double a2com(double a) const;
double com2a(double com) const;
double z2com(double z) const {
double a = z2a(z);
double dcom = a2com(a);
return dcom;
};
double dcom_dz(double z) const;
double com2comph(double r) const { return parameters.h * r; }
double comph2com(double r) const { return r / parameters.h; }
double comph2d_plus(double r) const;
double comph2g_plus(double r) const;
double comph2Hubble(double r) const;
double comph2a(double r) const;
double a2dlum(double a) const {
double z = a2z(a);
double dcom = a2com(a);
return (1 + z) * dcom;
};
double z2dlum(double z) const {
double a = z2a(z);
double dcom = a2com(a);
return (1 + z) * dcom;
};
LIBLSS_COSMOLOGY_INVERSE_FUNCTION(dlum2a, a2dlum, A_MIN, A_MAX);
double a2dA(double a) const {
double z = a2z(a);
double dcom = a2com(a);
return dcom / (1 + z);
};
double z2dA(double z) const {
double a = z2a(z);
double dcom = a2com(a);
return dcom / (1 + z);
};
//a2dA not invertible over full redhsiftrange
LIBLSS_COSMOLOGY_INVERSE_FUNCTION(dA2a, a2dA, 0.5, A_MAX);
double Hubble(double a) const;
double hNow() const { return parameters.h; }
double k_J(double a);
double kF_baryon(double a);
double kSZ_kernel(double a);
void print_cdmspec2file(std::string outputFileName);
double power_spectrum(double k, int type);
double transfer_function(double k);
double power_spectrum_grav(double k, int type);
double rho_background_matter(double a);
double gravpot_norm();
double return_cosmo_par(std::string cosmopar);
double FHubble(double a) { return (parameters.h * 100 / (a * Hubble(a))); }
double dtr(double ai, double af);
double dtv(double ai, double af);
double integral_d_plus(double ai, double af);
double rho_crit();
double mass_of_volume(double V);
};
#undef LIBLSS_COSMOLOGY_INVERSE_FUNCTION
} // namespace LibLSS
// clang-format off
CTOOL_STRUCT_TYPE(LibLSS::CosmologicalParameters,
HDF5T_CosmologicalParameters,
((double, omega_r))
((double, omega_k))
((double, omega_m))
((double, omega_b))
((double, omega_q))
((double, w))
((double, n_s))
((double, fnl))
((double, wprime))
((double, sigma8))
((double, rsmooth))
((double, h))
((double, beta))
((double, z0))
((double, a0))
);
// clang-format on
#endif