double captureaux_(double(*fDv)(double*),int*forSun, double*csIp,double*csIn,double*csDp, double*csDn)
{
_fDv=fDv;
return captureAux(fDv_, *forSun,*csIp, *csIn,*csDp,*csDn);
}
int main(int argc,char** argv)
{ int err,n,i;
// data corresponding to MSSM/mssmh.dat
// cross sections of DM-nucleon interaction
double csSIp=5.489E-09, csSIn=5.758E-09, csSDp=5.807E-05, csSDn=-4.503E-05; //[pb]
// cross section of DM annihilation in halo
double vcs = 0.310; // [pb]
#define nCH 5 /* annihilation channels and their fractions*/
int pdgCH[nCH] ={ 6, 5, 15, 23, 24};
double fracCH[nCH]={0.59,0.12,0.20,0.03, 0.06};
sortOddParticles(NULL);
// Mass of Dark Matter
Mcdm=189.0;
#ifdef INDIRECT_DETECTION
{
double sigmaV;
char txt[100];
double SpA[NZ],SpE[NZ],SpP[NZ];
double FluxA[NZ],FluxE[NZ],FluxP[NZ], buff[NZ];
double SMmev=320; /* solar potential in MV */
double Etest=Mcdm/2;
printf("\n==== Indirect detection =======\n");
sigmaV=vcs*2.9979E-26;
printf("sigmav=%.2E[cm^3/s]\n",sigmaV);
SpA[0]=SpE[0]=SpP[0]=Mcdm;
for(i=1;i<NZ;i++) { SpA[i]=SpE[i]=SpP[i]=0;}
// Calculation on photon, positron and antiproton spectra: summation over channels
for(n=0;n<nCH;n++) if(fracCH[n]>0)
{
basicSpectra(Mcdm,pdgCH[n],0, buff); for(i=1;i<NZ;i++) SpA[i]+=buff[i]*fracCH[n];
basicSpectra(Mcdm,pdgCH[n],1, buff); for(i=1;i<NZ;i++) SpE[i]+=buff[i]*fracCH[n];
basicSpectra(Mcdm,pdgCH[n],2, buff); for(i=1;i<NZ;i++) SpP[i]+=buff[i]*fracCH[n];
}
// Photon flux
{ double Emin=1; /* Energy cut in GeV */
double fi=0.0,dfi=M_PI/180.; /* angle of sight and 1/2 of cone angle in [rad] */
gammaFluxTab(fi,dfi, sigmaV, SpA, FluxA);
printf("Photon flux for angle of sight f=%.2f[rad]\n"
"and spherical region described by cone with angle %.2f[rad]\n",fi,2*dfi);
#ifdef SHOWPLOTS
sprintf(txt,"Photon flux[cm^2 s GeV]^{1} at f=%.2f[rad], cone angle %.2f[rad]",fi,2*dfi);
displaySpectrum(txt,Emin,Mcdm,FluxA);
#endif
printf("Photon flux = %.2E[cm^2 s GeV]^{-1} for E=%.1f[GeV]\n",SpectdNdE(Etest, FluxA), Etest);
}
// Positron flux
{ double Emin=1.;
posiFluxTab(Emin, sigmaV, SpE, FluxE);
if(SMmev>0) solarModulation(SMmev,0.0005,FluxE,FluxE);
#ifdef SHOWPLOTS
displaySpectrum("positron flux [cm^2 s sr GeV]^{-1}" ,Emin,Mcdm,FluxE);
#endif
printf("Positron flux = %.2E[cm^2 sr s GeV]^{-1} for E=%.1f[GeV] \n",
SpectdNdE(Etest, FluxE), Etest);
}
// antiproton flux
{ double Emin=1;
pbarFluxTab(Emin, sigmaV, SpP, FluxP );
if(SMmev>0) solarModulation(SMmev,1,FluxP,FluxP);
#ifdef SHOWPLOTS
displaySpectrum("antiproton flux [cm^2 s sr GeV]^{-1}" ,Emin, Mcdm,FluxP);
#endif
printf("Antiproton flux = %.2E[cm^2 sr s GeV]^{-1} for E=%.1f[GeV] \n",
SpectdNdE(Etest, FluxP), Etest);
}
}
#endif
// Interaction with nucleus
#ifdef CDM_NUCLEUS
{ double dNdE[300];
double nEvents;
printf("\n======== Direct Detection ========\n");
nEvents=nucleusRecoilAux(Maxwell,73,Z_Ge,J_Ge73,SxxGe73, csSIp,csSIn, csSDp,csSDn,dNdE);
printf("73Ge: Total number of events=%.2E /day/kg\n",nEvents);
printf("Number of events in 10 - 50 KeV region=%.2E /day/kg\n",
cutRecoilResult(dNdE,10,50));
#ifdef SHOWPLOTS
displayRecoilPlot(dNdE,"Distribution of recoil energy of 73Ge",0,199);
#endif
nEvents=nucleusRecoilAux(Maxwell,131,Z_Xe,J_Xe131,SxxXe131,csSIp,csSIn, csSDp,csSDn,dNdE);
printf("131Xe: Total number of events=%.2E /day/kg\n",nEvents);
printf("Number of events in 10 - 50 KeV region=%.2E /day/kg\n",
cutRecoilResult(dNdE,10,50));
#ifdef SHOWPLOTS
displayRecoilPlot(dNdE,"Distribution of recoil energy of 131Xe",0,199);
#endif
nEvents=nucleusRecoilAux(Maxwell,23,Z_Na,J_Na23,SxxNa23,csSIp,csSIn, csSDp,csSDn,dNdE);
printf("23Na: Total number of events=%.2E /day/kg\n",nEvents);
printf("Number of events in 10 - 50 KeV region=%.2E /day/kg\n",
cutRecoilResult(dNdE,10,50));
#ifdef SHOWPLOTS
displayRecoilPlot(dNdE,"Distribution of recoil energy of 23Na",0,199);
#endif
nEvents=nucleusRecoilAux(Maxwell,127,Z_I,J_I127,SxxI127,csSIp,csSIn, csSDp,csSDn,dNdE);
printf("I127: Total number of events=%.2E /day/kg\n",nEvents);
printf("Number of events in 10 - 50 KeV region=%.2E /day/kg\n",
cutRecoilResult(dNdE,10,50));
#ifdef SHOWPLOTS
displayRecoilPlot(dNdE,"Distribution of recoil energy of 127I",0,199);
#endif
}
#endif
// Neutrino telescope
#ifdef NEUTRINO
{ double nu[NZ], nu_bar[NZ],mu[NZ],buff[NZ];
double Crate,R,Prop;
int forSun=1;
double Emin=1;
int i,err;
double yrs=31556925.2;
printf("\n===============Neutrino Telescope======= for ");
if(forSun) printf("Sun\n"); else printf("Earth\n");
// Capture rate
Crate=captureAux(Maxwell,forSun, Mcdm,csSIp,csSIn,csSDp,csSDn);
nu[0]=nu_bar[0]=Mcdm;
for(i=1;i<NZ;i++){ nu[i]=nu_bar[i]=0;}
// Calculation of neutrino, antineutrino spectra: sumation over chanels
for(n=0;n<nCH;n++) if(fracCH[n]>0)
{ double bn[NZ],bn_[NZ];
basicNuSpectra(forSun,Mcdm, pdgCH[n], 0, bn, bn_);
for(i=1;i<NZ;i++) { nu[i] +=bn[i]*fracCH[n]; nu_bar[i] +=bn_[i]*fracCH[n];}
}
// propagation: neutrino flux at Earth
if(forSun) R=150E6; else R=6378.1; // distance in km
Prop=yrs/(4*M_PI*R*R); // in Year*km^2
for(i=1;i<NZ;i++) { nu[i]*= 0.5*Crate*Prop; nu_bar[i]*=0.5*Crate*Prop; }
// Display neutrino flux
#ifdef SHOWPLOTS
displaySpectra("neutrino fluxes [1/Year/km^2/GeV]",Emin,Mcdm,2, nu,"nu",nu_bar,"nu_bar");
#endif
{
printf(" E>%.1E GeV neutrino flux %.3E [1/Year/km^2] \n",Emin,spectrInfo(Emin,nu,NULL));
printf(" E>%.1E GeV anti-neutrino flux %.3E [1/Year/km^2]\n", Emin,spectrInfo(Emin,nu_bar,NULL));
}
//Exclusion level
if(forSun) printf("IceCube22 exclusion confidence level = %.2E%%\n", exLevIC22(nu,nu_bar,NULL));
}
#endif
#ifdef CLEAN
#endif
killPlots();
return 0;
}
