| 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 |
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| 10 | #include "pexceptions.h"
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| 11 | #include "cspline.h"
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| 12 |
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| 13 | #include "constcosmo.h"
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| 14 | #include "cosmocalc.h"
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| 15 | #include "geneutils.h"
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| 16 |
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| 17 |
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| 18 | ///////////////////////////////////////////////////////////
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| 19 | //*********************** CosmoCalc *********************//
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| 20 | ///////////////////////////////////////////////////////////
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| 21 |
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| 22 | //----------------------------------------------------------
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| 23 | // flat = 0 : no compute Otot from other
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| 24 | // = 1 : change Omatter to get Otot=1
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| 25 | // = 2 : change Olambda to get Otot=1
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| 26 | // = 3 : change Orelat to get Otot=1
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| 27 | // usespline = "true" : compute integrale then use spline to extrapolate
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| 28 | // = "false" : compute integrale everytime
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| 29 | // zmax : maximum redshift(only if usespline=true)
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| 30 |
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| 31 | CosmoCalc::CosmoCalc(unsigned short flat,bool usespline,double zmax)
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| 32 | : _flat(flat),
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| 33 | _zold(-1.) , _integval(0.),
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| 34 | _usespline(usespline), _computespl(true), _zmax(zmax), _spline(NULL),
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| 35 | _nspl(0), _xspl(NULL), _yspl(NULL)
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| 36 | {
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| 37 | if(_usespline && _zmax<=0.) {
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| 38 | cout<<"CosmoCalc::CosmoCalc: Error bad _zmax value zmax="<< _zmax<<endl;
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| 39 | throw ParmError("CosmoCalc::UseSpline: Error bad _zmax value");
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| 40 | }
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| 41 | DefaultParam();
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| 42 | SetInteg();
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| 43 | }
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| 44 |
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| 45 | CosmoCalc::CosmoCalc(CosmoCalc& univ)
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| 46 | : _spline(NULL), _xspl(NULL), _yspl(NULL)
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| 47 | {
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| 48 | Clone(univ);
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| 49 | if(_usespline && _zmax<=0.) {
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| 50 | cout<<"CosmoCalc::CosmoCalc: Error bad _zmax value zmax="<< _zmax<<endl;
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| 51 | throw ParmError("CosmoCalc::UseSpline: Error bad _zmax value");
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| 52 | }
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| 53 | }
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| 54 |
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| 55 | CosmoCalc::~CosmoCalc(void)
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| 56 | {
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| 57 | if(_spline != NULL) delete _spline; _spline = NULL;
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| 58 | if(_xspl != NULL) delete [] _xspl; _xspl = NULL;
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| 59 | if(_yspl != NULL) delete [] _yspl; _yspl = NULL;
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| 60 | }
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| 61 |
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| 62 | void CosmoCalc::Clone(CosmoCalc& univ)
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| 63 | {
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| 64 | _flat = univ._flat;
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| 65 | _h100 = univ._h100;
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| 66 | _H0 = univ._H0;
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| 67 | _Olambda0 = univ._Olambda0;
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| 68 | _W0 = univ._W0;
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| 69 | _Omatter0 = univ._Omatter0;
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| 70 | _Obaryon0 = univ._Obaryon0;
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| 71 | _Orelat0 = univ._Orelat0;
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| 72 | _Otot0 = univ._Otot0;
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| 73 | _Ocurv0 = univ._Ocurv0;
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| 74 | _Dhubble = univ._Dhubble;
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| 75 |
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| 76 | _dperc = univ._dperc;
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| 77 | _dzinc = univ._dzinc;
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| 78 | _dzmax = univ._dzmax;
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| 79 | _glorder = univ._glorder;
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| 80 | if(_xgausl.size()>0) {
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| 81 | _xgausl.resize(0); _wgausl.resize(0);
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| 82 | for(int i=0;i<(int)_xgausl.size();i++) {
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| 83 | _xgausl.push_back(univ._xgausl[i]);
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| 84 | _wgausl.push_back(univ._wgausl[i]);
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| 85 | }
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| 86 | }
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| 87 |
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| 88 | _zold = -1.;
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| 89 | _integval = -1.;
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| 90 |
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| 91 | _usespline = univ._usespline;
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| 92 | _computespl = true;
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| 93 | _zmax = univ._zmax;
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| 94 | _nspl = 0;
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| 95 | if(_spline) delete _spline; _spline = NULL;
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| 96 | if(_xspl) delete [] _xspl; _xspl = NULL;
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| 97 | if(_yspl) delete [] _yspl; _yspl = NULL;
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| 98 | }
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| 99 |
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| 100 | //----------------------------------------------------------
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| 101 | // On va couper l'intervalle entre [0,zmax]:
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| 102 | // On parcourt [0,zmax] par pas de dzinc
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| 103 | // et on cree un intervalle
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| 104 | // - si la fonction varie de plus de "dperc"
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| 105 | // - ou si l'increment en z est superieur a "dzmax"
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| 106 | void CosmoCalc::SetInteg(double dperc,double dzinc,double dzmax,unsigned short order)
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| 107 | {
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| 108 | _dperc = dperc; _dzinc = dzinc; _dzmax = dzmax;
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| 109 |
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| 110 | if(_dperc<=0.) _dperc = 0.01;
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| 111 |
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| 112 | if(_dzinc<=0.) _dzinc = _zmax/100.;
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| 113 | if(_dzinc>=_zmax/2.) _dzinc = _zmax/2.; // Protection against big dzinc
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| 114 |
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| 115 | if(_dzmax<=0.) _dzmax = _zmax;
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| 116 | if(_dzmax<_dzinc) _dzmax = _dzinc;
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| 117 |
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| 118 | _glorder = order;
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| 119 | if(_glorder<=1) _glorder = 4;
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| 120 | Compute_GaussLeg(_glorder,_xgausl,_wgausl,0.,1.);
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| 121 |
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| 122 | _computespl=true;
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| 123 | }
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| 124 |
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| 125 |
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| 126 | void CosmoCalc::PrtInteg(void)
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| 127 | {
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| 128 | printf("CosmoCalc::PrtInteg: dperc=%g dzinc=%g dzmax=%g glorder=%hu\n",_dperc,_dzinc,_dzmax,_glorder);
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| 129 | }
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| 130 |
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| 131 | void CosmoCalc::SetObaryon0(double v)
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| 132 | {
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| 133 | _Obaryon0 = v;
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| 134 | if(_Obaryon0<0.) {
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| 135 | cout<<"CosmoCalc::SetObaryon0: Error bad _Obaryon0 value: "<<_Obaryon0<<endl;
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| 136 | throw ParmError("CosmoCalc::SetObaryon0: Error bad _Obaryon0 value");
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| 137 | }
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| 138 | }
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| 139 |
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| 140 | void CosmoCalc::SetDynParam(double h100,double om0,double or0,double ol0,double w0)
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| 141 | {
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| 142 | _computespl=true;
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| 143 |
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| 144 | _h100 = h100;
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| 145 | _H0 = 100. * _h100 ;
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| 146 | _Dhubble = SpeedOfLight_Cst / _H0;
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| 147 |
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| 148 | _Omatter0 = om0;
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| 149 | _Orelat0 = or0;
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| 150 | _Olambda0 = ol0;
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| 151 | _W0 = w0;
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| 152 | _Otot0 = _Olambda0 + _Omatter0 + _Orelat0;
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| 153 | _Ocurv0 = 1. - _Otot0;
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| 154 | if( _h100<0. || _Omatter0<0. || _Orelat0<0. || _Olambda0<0. ) {
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| 155 | cout<<"CosmoCalc::SetDynParam: Error bad parameter value"<<endl;
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| 156 | throw ParmError("CosmoCalc::SetDynParam: Error bad parameter value");
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| 157 | }
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| 158 | if(_flat==0) return;
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| 159 |
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| 160 | _Otot0 = 1.; _Ocurv0 = 0.;
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| 161 | if(_flat==1) {
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| 162 | _Omatter0 = _Otot0 - _Olambda0 - _Orelat0;
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| 163 | if( _Omatter0<0. ) {
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| 164 | cout<<"CosmoCalc::SetDynParam: Error bad _Omatter0 value: "<<_Omatter0<<endl;
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| 165 | throw ParmError("CosmoCalc::SetDynParam: Error bad _Omatter0 value");
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| 166 | }
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| 167 | return;
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| 168 | }
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| 169 |
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| 170 | //--
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| 171 | if(_flat==2) {
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| 172 | _Olambda0 = _Otot0 - _Omatter0 - _Orelat0;
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| 173 | if( _Olambda0<0. ) {
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| 174 | cout<<"CosmoCalc::SetDynParam: Error bad _Olambda0 value: "<<_Olambda0<<endl;
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| 175 | throw ParmError("CosmoCalc::SetDynParam: Error bad _Olambda0 value");
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| 176 | }
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| 177 | return;
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| 178 | }
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| 179 |
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| 180 | //--
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| 181 | if(_flat==3) {
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| 182 | _Orelat0 = _Otot0 - _Omatter0 - _Olambda0;
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| 183 | if( _Orelat0<0. ) {
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| 184 | cout<<"CosmoCalc::SetDynParam: Error bad _Orelat0 value: "<<_Orelat0<<endl;
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| 185 | throw ParmError("CosmoCalc::SetDynParam: Error bad _Orelat0 value");
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| 186 | }
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| 187 | return;
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| 188 | }
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| 189 |
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| 190 | cout<<"CosmoCalc::SetDynParam: Error bad _flat value: "<<_flat<<endl;
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| 191 | throw ParmError("CosmoCalc::SetDynParam: Error bad _flat value");
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| 192 |
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| 193 | }
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| 194 |
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| 195 | void CosmoCalc::DefaultParam(void)
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| 196 | {
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| 197 | _computespl=true;
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| 198 |
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| 199 | double h100 = 0.71;
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| 200 | double ol0 = 0.73, w0 = -1.;
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| 201 | double om0 = 0.135/(h100*h100);
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| 202 | // Relat = photons (2.725 K) + neutrinos (1.9 K)
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| 203 | double or0 = 2.47e-5 * (1. + 21./8.*pow(T_NU_Par/T_CMB_Par,4.)) / (h100*h100);
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| 204 | SetDynParam(h100,om0,or0,ol0,w0);
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| 205 | _Obaryon0 = 0.0224/(h100*h100);
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| 206 |
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| 207 | return;
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| 208 | }
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| 209 |
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| 210 | //----------------------------------------------------------
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| 211 | void CosmoCalc::Print(double z)
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| 212 | {
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| 213 | if(z<0.) z = 0.;
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| 214 |
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| 215 | printf("CosmoCalc::Print(spl=%d,zmax=%g,flat=%u) for z=%g\n",int(_usespline),ZMax(),Flat(),z);
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| 216 | printf("h100=%g H0=%g Dhub=%g H(z)=%g Rhoc=%g g/cm^3 =%g Msol/Mpc^3\n"
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| 217 | ,h100(),H0(),Dhubble(),H(z),Rhoc(z),Rhoc(z)*GCm3toMsolMpc3_Cst);
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| 218 | printf("Olambda=%g W0=%g\n",Olambda(z),_W0);
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| 219 | printf("Omatter=%g Obaryon=%g\n",Omatter(z),Obaryon(z));
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| 220 | printf("Orelat=%g\n",Orelat(z));
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| 221 | printf("Otot=%g Ocurv=%g\n",Otot(z),Ocurv(z));
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| 222 | if(z <= 0.) return;
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| 223 | printf("Distance comoving: los=%g Mpc, transv=%g Mpc\n",Dloscom(z),Dtrcom(z));
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| 224 | printf("Distance: angular=%g Mpc, lum=%g Mpc\n",Dang(z),Dlum(z));
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| 225 | printf("Volume comoving element: %g Mpc^3/sr/dz=1\n",dVol(z));
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| 226 | printf("Volume comoving in [0,z] for 4Pi sr: %g Mpc^3\n",Vol4Pi(z));
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| 227 |
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| 228 | }
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| 229 | //----------------------------------------------------------
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| 230 | double CosmoCalc::Olambda(double z)
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| 231 | {
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| 232 | double v = _Olambda0;
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| 233 | if(_W0 != -1.) v *= pow((1.+z),3.*(1+_W0));
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| 234 | return v / E2(z);
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| 235 | }
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| 236 |
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| 237 | double CosmoCalc::Omatter(double z)
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| 238 | {
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| 239 | return _Omatter0 * (1.+z)*(1.+z)*(1.+z) /E2(z);
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| 240 | }
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| 241 |
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| 242 | double CosmoCalc::Obaryon(double z)
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| 243 | {
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| 244 | return _Obaryon0 * (1.+z)*(1.+z)*(1.+z) /E2(z);
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| 245 | }
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| 246 |
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| 247 | double CosmoCalc::Orelat(double z)
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| 248 | {
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| 249 | double z2 = (1.+z)*(1.+z);
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| 250 | return _Orelat0 * z2*z2 /E2(z);
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| 251 | }
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| 252 |
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| 253 | double CosmoCalc::Ocurv(double z)
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| 254 | {
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| 255 | return _Ocurv0 * (1.+z)*(1.+z) /E2(z);
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| 256 | }
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| 257 |
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| 258 | double CosmoCalc::Otot(double z)
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| 259 | {
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| 260 | return Olambda(z)+Omatter(z)+Orelat(z);
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| 261 | }
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| 262 |
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| 263 | double CosmoCalc::Rhoc(double z)
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| 264 | // Densite critique au redshift "z" en "g/cm^3"
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| 265 | {
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| 266 | double h2 = H(z) / MpctoMeters_Cst; h2 *= h2;
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| 267 | return 3.* h2 / (8.*M_PI*G_Newton_Cst) * 1000.;
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| 268 | }
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| 269 |
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| 270 | //----------------------------------------------------------
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| 271 | double CosmoCalc::Dloscom(double z) /* Mpc comobile */
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| 272 | {
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| 273 | return _Dhubble * NInteg(z);
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| 274 | }
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| 275 |
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| 276 | double CosmoCalc::Dtrcom(double z) /* Mpc comobile */
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| 277 | {
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| 278 | double v = NInteg(z); // Zero curvature
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| 279 |
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| 280 | if(_flat) return _Dhubble * v;
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| 281 |
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| 282 | if(_Ocurv0>0.) { // hyperbolique
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| 283 | double s = sqrt(_Ocurv0);
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| 284 | v = sinh(s*v)/s;
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| 285 | } else if(_Ocurv0<0.) { // spherique
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| 286 | double s = sqrt(-_Ocurv0);
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| 287 | v = sin(s*v)/s;
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| 288 | }
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| 289 |
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| 290 | return _Dhubble * v;
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| 291 |
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| 292 | }
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| 293 |
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| 294 | double CosmoCalc::Dang(double z) /* Mpc */
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| 295 | {
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| 296 | return Dtrcom(z) / (1.+z);
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| 297 | }
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| 298 |
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| 299 | double CosmoCalc::Dlum(double z) /* Mpc */
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| 300 | {
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| 301 | return (1.+z) * Dtrcom(z);
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| 302 | }
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| 303 |
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| 304 | double CosmoCalc::dVol(double z) /* Mpc^3/ sr / unite z */
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| 305 | {
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| 306 | double d = Dtrcom(z);
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| 307 | return _Dhubble * d*d / E(z);
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| 308 | }
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| 309 |
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| 310 | //----------------------------------------------------------
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| 311 | double CosmoCalc::Vol4Pi(double z) /* Mpc^3 pour 4Pi sr entre [0,z] */
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| 312 | // --- on pose x = dm/dh = (1+z)*da/dh, s = sqrt(|Ok|)
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| 313 | // Ok=0 : V(z)/dh^3 = (4*Pi/3) * x^3
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| 314 | // Ok>0 : V(z)/dh^3 = (4*Pi/(2*Ok)) * (x*sqrt(1+Ok*x^2) - 1/s * asinh(s*x))
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| 315 | // Ok<0 : V(z)/dh^3 = (4*Pi/(2*Ok)) * (x*sqrt(1+Ok*x^2) - 1/s * asin(s*x) )
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| 316 | // --- on pose y = s*x (y>0)
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| 317 | // Ok>0 : V(z)/dh^3 = (4*Pi/(2*Ok*s)) * (y*sqrt(1+y^2) - asinh(y))
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| 318 | // Ok<0 : V(z)/dh^3 = (4*Pi/(2*Ok*s)) * (y*sqrt(1-y^2) - asin(y) )
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| 319 | // --- a petit "z" on a pour "y -> 0+" en faisant le DL
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| 320 | // Ok>0 : V(z)/dh^3 = 4*Pi*y^3 / (3*Ok*s) * (1 - 3*y^2/10) + O(y^7)
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| 321 | // Ok<0 : V(z)/dh^3 = -4*Pi*y^3 / (3*Ok*s) * (1 + 3*y^2/10) + O(y^7)
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| 322 | // (remarque: Ok^(3/2) = s*Ok)
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| 323 | {
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| 324 | double v,x = Dtrcom(z)/_Dhubble;
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| 325 |
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| 326 | if(_flat) {
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| 327 | v = 4.*M_PI/3. * x*x*x;
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| 328 | } else if(_Ocurv0>0.) {
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| 329 | double s = sqrt(_Ocurv0), y = s*x, y2 = y*y;
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| 330 | if(y<1e-6) {
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| 331 | v = 1. - 3.*y2/10.;
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| 332 | v *= 4.*M_PI*y*y2 / (3.*_Ocurv0*s);
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| 333 | } else {
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| 334 | v = y*sqrt(1.+y2) - asinh(y);
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| 335 | v *= 4.*M_PI/(2.*_Ocurv0*s);
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| 336 | }
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| 337 | } else if (_Ocurv0<0.) {
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| 338 | double s = sqrt(-_Ocurv0), y = s*x, y2 = y*y;
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| 339 | if(y<1e-6) {
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| 340 | v = 1. + 3.*y2/10.;
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| 341 | v *= -4.*M_PI*y*y2 / (3.*_Ocurv0*s);
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| 342 | } else {
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| 343 | v = y*sqrt(1.-y2) - asin(y);
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| 344 | v *= 4.*M_PI/(2.*_Ocurv0*s);
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| 345 | }
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| 346 | } else {
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| 347 | v = 4.*M_PI/3. * x*x*x;
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| 348 | }
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| 349 |
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| 350 | return v * _Dhubble*_Dhubble*_Dhubble;
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| 351 | }
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| 352 |
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| 353 | double CosmoCalc::Vol4Pi(double z1,double z2) /* Mpc^3 pour 4Pi sr entre [z1,z2] */
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| 354 | {
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| 355 | return Vol4Pi(z2) - Vol4Pi(z1);
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| 356 | }
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| 357 |
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| 358 | double CosmoCalc::E2(double z) const
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| 359 | {
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| 360 | z += 1.;
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| 361 | double oldum = _Olambda0;
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| 362 |
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| 363 | if(oldum>0. && _W0!=-1.) oldum *= pow(z,3.*(1.+_W0));
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| 364 |
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| 365 | return oldum + z*z*(_Ocurv0 + z*(_Omatter0+z*_Orelat0));
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| 366 | }
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| 367 |
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| 368 | //----------------------------------------------------------
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| 369 | double CosmoCalc::NInteg(double z)
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| 370 | {
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| 371 | if(z<0.) {
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| 372 | cout<<"CosmoCalc::NInteg: Error bad z value z="<<z<<endl;
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| 373 | throw ParmError("CosmoCalc::NInteg: Error bad z value");
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| 374 | }
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| 375 |
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| 376 | // On utilise le spline
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| 377 | if(_usespline) {
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| 378 | if( (!_computespl) && (z==_zold) ) return _integval;
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| 379 | if(z>_zmax) {_zmax = z+_dzmax; _computespl = true;}
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| 380 | if(_computespl) Init_Spline();
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| 381 | _integval = _spline->CSplineInt(z);
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| 382 | _zold = z;
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| 383 | return _integval;
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| 384 | }
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| 385 |
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| 386 | // On calcule l'integrale
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| 387 | if(z != _zold) {
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| 388 | _integval = IntegrateFunc(*this,0.,z,_dperc,_dzinc,_dzmax,_glorder);
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| 389 | _zold = z;
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| 390 | }
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| 391 | return _integval;
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| 392 |
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| 393 | }
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| 394 |
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| 395 | int_4 CosmoCalc::Init_Spline(void)
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| 396 | {
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| 397 | if(_spline!=NULL)
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| 398 | {delete _spline; delete [] _xspl; delete [] _yspl;}
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| 399 |
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| 400 | //-- Look for intervalles and integrate
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| 401 | vector<double> x,y;
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| 402 | x.push_back(0.); y.push_back(0.);
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| 403 | double zbas=0., fbas = Integrand(zbas);
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| 404 | for(double z=_dzinc;;z+=_dzinc) {
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| 405 | double f = Integrand(z);
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| 406 | //cout<<fbas<<","<<f<<" : "<<fabs(f-fbas)<<" >? "<<_dperc*fabs(fbas)<<endl;
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| 407 | if( z>_zmax || z-zbas>_dzmax || fabs(f-fbas)>_dperc*fabs(fbas) ) {
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| 408 | double sum=0., dz=z-zbas;
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| 409 | for(unsigned short i=0;i<_glorder;i++) sum += _wgausl[i]*Integrand(zbas+_xgausl[i]*dz);
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| 410 | x.push_back(z); y.push_back(sum*dz);
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| 411 | //cout<<"...set... "<<zbas<<","<<z<<" , "<<fbas<<","<<f<<endl;
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| 412 | zbas = z; fbas = f;
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| 413 | if( z>_zmax ) break;
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| 414 | }
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| 415 | }
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| 416 |
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| 417 | //-- Protection car il faut au moins 4 points pour un spline cubique
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| 418 | if(x.size()<4) {
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| 419 | x.resize(0); y.resize(0);
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| 420 | x.push_back(0.); y.push_back(0.);
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| 421 | for(int i=1;i<4;i++) {
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| 422 | x.push_back(i*_zmax/3.);
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| 423 | double sum=0., dz=x[i]-x[i-1];
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| 424 | for(unsigned short i=0;i<_glorder;i++) sum += _wgausl[i]*Integrand(x[i-1]+_xgausl[i]*dz);
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| 425 | y.push_back(sum*dz);
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| 426 | }
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| 427 | }
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| 428 |
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| 429 | //-- Fill spline
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| 430 | _nspl = x.size();
|
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| 431 | _xspl = new double[_nspl];
|
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| 432 | _yspl = new double[_nspl];
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| 433 | for(int i=0;i<_nspl;i++) {
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| 434 | _xspl[i] = x[i];
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| 435 | _yspl[i] = y[i];
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| 436 | if(i!=0) _yspl[i] += _yspl[i-1];
|
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| 437 | }
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| 438 |
|
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| 439 | #if 1
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| 440 | cout<<"CosmoCalc::Init_Spline called: (zmax="<<_zmax<<") _nspl="<<_nspl<<endl;
|
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| 441 | int n = (_nspl>5)? 5: _nspl;
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| 442 | cout<<_nspl<<"...";
|
|---|
| 443 | for(int i=0;i<n;i++) cout<<_xspl[i]<<" ("<<_yspl[i]<<") ";
|
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| 444 | cout<<"\n... ";
|
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| 445 | n = (_nspl<5)? 0: _nspl-5;
|
|---|
| 446 | for(int i=n;i<_nspl;i++) cout<<_xspl[i]<<" ("<<_yspl[i]<<") ";
|
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| 447 | cout<<endl;
|
|---|
| 448 | #endif
|
|---|
| 449 |
|
|---|
| 450 | double yp1 = Integrand(_xspl[0]);
|
|---|
| 451 | double ypn = Integrand(_xspl[_nspl-1]);
|
|---|
| 452 | _spline = new CSpline(_nspl,_xspl,_yspl,yp1,ypn,CSpline::NoNatural,false);
|
|---|
| 453 | _spline->ComputeCSpline();
|
|---|
| 454 | _computespl = false;
|
|---|
| 455 |
|
|---|
| 456 | return _nspl;
|
|---|
| 457 | }
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