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| 1 | #ifndef CONSTCOSMO_SEEN | 
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| 2 | #define CONSTCOSMO_SEEN | 
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| 3 |  | 
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| 4 | static const double SpeedOfLight_Cst = 299792.458; // speed of light "km/sec" | 
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| 5 | static const double G_Newton_Cst = 6.6742e-11; // G_N in SI units "m^3 / kg /s^2" | 
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| 6 | static const double h_Planck_Cst = 6.6260693e-34;   // Planck constant SI units "J s" | 
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| 7 | static const double k_Boltzman_Cst = 1.3806503e-23;  // Boltzman constant SI "J / K" | 
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| 8 | //            Sigma = 2*PI^5*K^4/(15.*C^2*H^3) = PI^2*K^4/(60.*Hbar^3*C2) | 
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| 9 | static const double StefBoltz_Cst = 5.670400e-8; // constante de Stefan-Boltzman in "W/m^2/K^4" | 
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| 10 | static const double Zeta_3_Cst = 1.2020569031595942854; // Zeta(3) | 
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| 11 |  | 
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| 12 | static const double YeartoSec_Cst = 31556925.2; // 1 year into seconds | 
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| 13 | static const double MpctoMeters_Cst = 3.0856e+22; // 1 Mpc into meters | 
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| 14 | static const double LightYear_Cst = 9.46073042e+15; // 1 Light-Year into "m" | 
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| 15 | static const double Jansky2Watt_cst = 1.e-26;  // 1 Jansky into "Watt/m^2/Hz == J/m^2" | 
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| 16 | static const double SolarMass_Cst = 1.98844e+33; // 1 Solar mass into "g" | 
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| 17 | //                  GCm3toMsolMpc3_Cst = (MpctoMeters_Cst*100)^3 / SolarMass_Cst | 
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| 18 | static const double GCm3toMsolMpc3_Cst = 1.477428208143872e+40; // 1 g/cm^3 into 1 Msol/Mpc^3 | 
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| 19 | static const double ProtonMass_Cst = 1.67262171e-24; // 1 "proton mass" in "g" | 
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| 20 | static const double Deg2Rad_Cst = (M_PI/180.); // 1 deg into rad | 
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| 21 |  | 
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| 22 | static const double T_CMB_Par = 2.725;  // temperature du CMB en "K" | 
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| 23 | static const double T_NU_Par = 1.9;  // temperature des neutrinos en "K" | 
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| 24 | static const double Fr_HyperFin_Par = 1.420405751786;  // frequence de la raie hyperfine HI en "GHz" | 
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| 25 |  | 
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| 26 | #endif | 
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