1 | // Classes to compute simple quantities for radio / 21 cm
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2 | // R. Ansari - June 2010
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3 |
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4 | #ifndef RADUTIL_SEEN
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5 | #define RADUTIL_SEEN
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6 |
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7 | #include "machdefs.h" // SOPHYA .h
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8 | #include "sopnamsp.h" // SOPHYA .h
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9 |
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10 | #include "vector3d.h" // conversion d'angle
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11 |
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12 | class H21Conversions {
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13 | public:
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14 | // redshift nul, angle solide du pixel en steradian
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15 | H21Conversions(double freq=0., double opix=1.e-5);
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16 |
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17 | double toJansky(double temp); // Conversion d'une temperature (Kelvin) en jansky
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18 | double toKelvin(double jy); // Conversion de Jansky en temperature (Kelvin)
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19 |
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20 | double Mean21cmTemperature_mK(); // Temperature moyenne de l'emission a 21 cm en mK
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21 | inline double T21cm_Kelvin() { return Mean21cmTemperature_mK()/1000.; }
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22 | inline double T21cm_mK() { return Mean21cmTemperature_mK(); }
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23 |
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24 | void setFrequency(double nu); // on definit la frequence en MHz
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25 | inline void setRedshift(double z) // on definit le redshift
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26 | { setFrequency(Freq021cm_Cst/(1+z)); }
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27 | inline void setLambda(double lam) // on definit la longueur d'onde en m
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28 | { setFrequency(SpeedOfLight_Cst/lam); }
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29 |
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30 | inline void setOmegaPix(double opix) // angle solide en steradian
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31 | { omegapix_ = opix; }
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32 | inline void setOmegaPixDeg2(double opix) // angle solide en Deg^2
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33 | { double cf=Angle(1.,Angle::Degree).ToRadian(); omegapix_ = opix*cf*cf; }
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34 | inline void setOmegaPixArcmin2(double opix) // angle solide en Arcmin^2
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35 | { double cf=Angle(1.,Angle::ArcMin).ToRadian(); omegapix_ = opix*cf*cf; }
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36 |
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37 | // Definition des parametres cosmologiques utiles pour le calcul de la temperature d'emission a 21 cm
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38 | // retourne la valeur de OmegaLambda (univers plat)
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39 | double setCosmoParam(double omegamatter=0.2581, double omegabaryon=0.0441, double h100=0.719, double fracHI=0.02);
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40 | inline void setFracHI(double fracHI=0.02) { fracHI_=fracHI; }
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41 |
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42 | inline double getRedshift() { return z_; }
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43 | inline double getFrequency() { return freq_; }
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44 | inline double getLambda() { return lambda_; }
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45 |
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46 | inline double getOmegaPix() // angle solide en steradian
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47 | { return omegapix_; }
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48 | inline double getOmegaPixArcmin2() // angle solide en Arcmin^2
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49 | { double cf=Angle(1.,Angle::ArcMin).ToRadian(); return omegapix_/cf/cf; }
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50 | inline double getOmegaPixDeg2() // angle solide en Deg^2
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51 | { double cf=Angle(1.,Angle::Degree).ToRadian(); return omegapix_/cf/cf; }
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52 |
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53 |
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54 | static double SpeedOfLight_Cst; // Speed of light m/sec
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55 | static double Freq021cm_Cst; // 21 cm transition frequency in MHz
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56 | static double k_Boltzman_Cst; // Boltzmann constant (SI Units)
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57 |
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58 | double z_;
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59 | double freq_;
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60 | double lambda_;
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61 | double omegapix_;
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62 |
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63 | // Parametres cosmologiques pour calcul du coefficient de conversion Mass to T21
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64 | double OmegaMatter_;
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65 | double OmegaBaryons_;
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66 | double OmegaLambda_;
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67 | double h100_;
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68 | double fracHI_;
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69 | };
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70 |
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71 | #endif
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