| 1 | #include "sopnamsp.h" | 
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| 2 | #include "machdefs.h" | 
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| 3 | #include <iostream> | 
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| 4 | #include <stdlib.h> | 
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| 5 | #include <stdio.h> | 
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| 6 | #include <string.h> | 
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| 7 | #include <math.h> | 
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| 8 | #include <unistd.h> | 
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| 9 | #include "timing.h" | 
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| 10 | #include "ntuple.h" | 
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| 11 |  | 
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| 12 | #include "luc.h" | 
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| 13 |  | 
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| 14 | void usage(void); | 
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| 15 | void usage(void) | 
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| 16 | { | 
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| 17 | cout<<"cmvtuniv z1,z2,dz"<<endl; | 
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| 18 | } | 
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| 19 |  | 
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| 20 | int main(int narg,char *arg[]) | 
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| 21 | { | 
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| 22 | // -- WMAP | 
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| 23 | double h100=0.71, om0=0.267804, or0=7.9e-05, ol0=0.73,w0=-1., ob0=0.045, oph0=5e-5; | 
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| 24 | // -- ouvert matter only | 
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| 25 | //double h100=0.71, om0=0.3, or0=0., ol0=0.,w0=-1., ob0=0.045, oph0=5e-5; | 
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| 26 | // -- plat matter only | 
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| 27 | //double h100=0.71, om0=1., or0=0., ol0=0.,w0=-1., ob0=0.045, oph0=5e-5; | 
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| 28 |  | 
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| 29 | double z1=0., z2=10., dz=1.; | 
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| 30 | if(narg>1) sscanf(arg[1],"%lf,%lf,%lf",&z1,&z2,&dz); | 
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| 31 |  | 
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| 32 | SimpleUniverse univ; | 
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| 33 | univ.SetPrtDbgLevel(1); | 
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| 34 |  | 
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| 35 | univ.Seth(h100); | 
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| 36 | univ.SetOmegaMatter(om0); | 
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| 37 | univ.SetOmegaLambda(ol0); | 
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| 38 | //univ.SetDarkEnergy(ol0,w0); | 
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| 39 | univ.SetOmegaRadiation(or0); | 
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| 40 | univ.SetOmegaBaryon(ob0); | 
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| 41 | univ.SetOmegaPhoton(oph0); | 
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| 42 |  | 
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| 43 | //univ.SetFlatUniverse_OmegaMatter(); | 
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| 44 | //univ.SetFlatUniverse_OmegaLambda(); | 
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| 45 |  | 
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| 46 | /* | 
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| 47 | for(double z=z1;z<z2+dz/2.;z+=dz) { | 
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| 48 | univ.SetEmissionRedShift(z,0.001); | 
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| 49 | cout<<endl; | 
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| 50 | univ.Print(); | 
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| 51 | } | 
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| 52 | */ | 
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| 53 |  | 
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| 54 | /**/ | 
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| 55 | double norm = univ.HubbleLengthMpc(); // 1.; | 
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| 56 | double norm3 = pow(norm,3.); | 
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| 57 | const int n = 11; | 
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| 58 | char *vname[n] = { | 
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| 59 | "z","hz","om","or","ol","ok","ot", | 
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| 60 | "da","dl","dvc","vc0" | 
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| 61 | }; | 
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| 62 | NTuple nt(n,vname); | 
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| 63 | double xnt[n]; | 
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| 64 | for(double z=z1;z<z2+dz/2.;z+=dz) { | 
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| 65 | univ.SetEmissionRedShift(z,0.001); | 
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| 66 | xnt[0]  = univ.ZE(); | 
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| 67 | xnt[1]  = univ.HZE(); | 
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| 68 | xnt[2]  = univ.OmegaMatterZE(); | 
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| 69 | xnt[3]  = univ.OmegaRadiationZE(); | 
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| 70 | xnt[4]  = 0.; //univ.OmegaLambdaZE()+univ.OmegaDarkZE(); | 
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| 71 | xnt[5]  = univ.OmegaCurvZE(); | 
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| 72 | xnt[6]  = 0.; //univ.OmegaTotalZE(); | 
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| 73 | xnt[7]  = univ.AngularDiameterDistanceMpc()/norm; | 
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| 74 | xnt[8]  = univ.LuminosityDistanceMpc()/norm; | 
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| 75 | if(xnt[8]<0.) cout<<xnt[8]<<endl; | 
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| 76 | xnt[9]  = 0.; //univ.dVolZE()/norm3; | 
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| 77 | xnt[10] = 0.; //univ.Vol4PiZE()/norm3; | 
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| 78 | nt.Fill(xnt); | 
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| 79 | } | 
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| 80 | cout<<">>>> Ecriture"<<endl; | 
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| 81 | string tag = "cmvtluc.ppf"; | 
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| 82 | POutPersist pos(tag); | 
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| 83 | tag = "nt"; pos.PutObject(nt,tag); | 
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| 84 | /**/ | 
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| 85 |  | 
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| 86 | return 0; | 
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| 87 | } | 
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| 88 |  | 
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| 89 |  | 
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| 90 | /* | 
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| 91 | openppf cmvtluc.ppf | 
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| 92 |  | 
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| 93 | set cut 1 | 
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| 94 | set cut z<100. | 
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| 95 |  | 
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| 96 | zone | 
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| 97 | n/plot nt.hz%z $cut ! "nsta" | 
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| 98 |  | 
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| 99 | zone | 
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| 100 | n/plot nt.dl%z $cut ! "nsta" | 
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| 101 | n/plot nt.da%z $cut ! "nsta same red" | 
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| 102 |  | 
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| 103 | */ | 
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