int main(int argc,char** argv)
{
int err,outP;
double M,Emin,Ntot,Etot,sigmaV,v=0.001,fi,tab[250];
char mess[100];
char txt[100];
if(argc==1)
{
printf(" The program needs 1 argument:\n"
"name of file with parameters\n");
exit(1);
}
err=readVar(argv[1]);
if(err==-1) {printf("Can not open the file\n"); exit(2);}
else if(err>0) { printf("Wrong file contents at line %d\n",err);exit(3);}
outP=0; /* for gamma rays */
Emin=0.1; /* Erergy cut */
fi=0; /* angle of sight */
err=sortOddParticles(mess);
if(err) { printf("Can't calculate %s\n",mess); return 1;}
sigmaV=calcSpectrum(v,outP,tab,&err); /* sigma*v in cm^3/sec */
M=lopmass_();
spectrInfo(Emin/M,tab, &Ntot,&Etot);
sprintf(txt,"%s: N=%.2e,<E/2M>=%.2f,vsc=%.2e sm^3/sec,M(%s)=%.2e",
outNames[outP],Ntot,Etot,sigmaV,mess,M);
spectrTable(tab,"tab",txt, Emin/M ,300);
system("../CalcHEP_src/bin/tab_view < tab&");
printf("gamma flux [ph/cm^2/s/sr] =%.2E\n",
HaloFactor(fi,rhoQisotermic)*sigmaV*Ntot/M/M);
{ double e[6];
int i;
printf("Check of energy conservation:\n");
for(i=0;i<6;i++)
{
sigmaV=calcSpectrum(v,i,tab,&err);
spectrInfo(Emin/M,tab, NULL,e+i);
}
printf("1 = %.2f\n",e[0]+2*(e[1]+e[2]+e[3]+e[4]+e[5]) );
}
return 0;
}
int main(int argc,char** argv)
{ int err;
char cdmName[10];
int spin2, charge3,cdim;
ForceUG=0; /* to Force Unitary Gauge assign 1 */
if(argc< 2)
{
printf(" Correct usage: ./main <file with parameters> \n");
printf("Example: ./main data1.par \n");
exit(1);
}
err=readVar(argv[1]);
if(err==-1) {printf("Can not open the file\n"); exit(1);}
else if(err>0) { printf("Wrong file contents at line %d\n",err);exit(1);}
err=sortOddParticles(cdmName);
if(err) { printf("Can't calculate %s\n",cdmName); return 1;}
qNumbers(cdmName, &spin2, &charge3, &cdim);
printf("\nDark matter candidate is '%s' with spin=%d/2\n",
cdmName, spin2);
if(charge3) { printf("Dark Matter has electric charge %d*3\n",charge3); exit(1);}
if(cdim!=1) { printf("Dark Matter ia a color particle\n"); exit(1);}
#ifdef MASSES_INFO
{
printf("\n=== MASSES OF HIGG AND ODD PARTICLES: ===\n");
printHiggs(stdout);
printMasses(stdout,1);
}
#endif
#ifdef OMEGA
{ int fast=1;
double Beps=1.E-5, cut=0.0001;
double Omega,Xf;
// deltaY=4.4E-13;
// to exclude processes with virtual W/Z in DM annihilation
VZdecay=0; VWdecay=0; cleanDecayTable();
// to include processes with virtual W/Z also in co-annihilation
// VZdecay=2; VWdecay=2; cleanDecayTable();
printf("\n==== Calculation of relic density =====\n");
Omega=darkOmega(&Xf,fast,Beps);
printf("Xf=%.2e Omega=%.2e\n",Xf,Omega);
printChannels(Xf,cut,Beps,1,stdout);
VZdecay=1; VWdecay=1; cleanDecayTable(); // restore default
}
#endif
#ifdef INDIRECT_DETECTION
{
int err,i;
double Emin=1,/* Energy cut in GeV */ sigmaV;
double vcs_gz,vcs_gg;
char txt[100];
double SpA[NZ],SpE[NZ],SpP[NZ];
double FluxA[NZ],FluxE[NZ],FluxP[NZ];
double * SpNe=NULL,*SpNm=NULL,*SpNl=NULL;
double Etest=Mcdm/2;
printf("\n==== Indirect detection =======\n");
sigmaV=calcSpectrum(4,SpA,SpE,SpP,SpNe,SpNm,SpNl ,&err);
/* Returns sigma*v in cm^3/sec. SpX - calculated spectra of annihilation.
Use SpectdNdE(E, SpX) to calculate energy distribution in 1/GeV units.
First parameter 1-includes W/Z polarization
2-includes gammas for 2->2+gamma
4-print cross sections
*/
printf("sigmav=%.2E[cm^3/s] = %.2E[pb] \n", sigmaV, sigmaV/2.9979E-26);
if(SpA)
{
double fi=0.1,dfi=0.05; /* 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(FluxA,txt,Emin,Mcdm);
#endif
printf("Photon flux = %.2E[cm^2 s GeV]^{-1} for E=%.1f[GeV]\n",SpectdNdE(Etest, FluxA), Etest);
}
if(SpE)
{
posiFluxTab(Emin, sigmaV, SpE, FluxE);
#ifdef SHOWPLOTS
displaySpectrum(FluxE,"positron flux [cm^2 s sr GeV]^{-1}" ,Emin,Mcdm);
#endif
printf("Positron flux = %.2E[cm^2 sr s GeV]^{-1} for E=%.1f[GeV] \n",
SpectdNdE(Etest, FluxE), Etest);
}
if(SpP)
{
pbarFluxTab(Emin, sigmaV, SpP, FluxP );
#ifdef SHOWPLOTS
displaySpectrum(FluxP,"antiproton flux [cm^2 s sr GeV]^{-1}" ,Emin, Mcdm);
#endif
printf("Antiproton flux = %.2E[cm^2 sr s GeV]^{-1} for E=%.1f[GeV] \n",
SpectdNdE(Etest, FluxP), Etest);
}
}
#endif
#ifdef RESET_FORMFACTORS
{
/*
The user has approach to form factors which specifies quark contents
of proton and nucleon via global parametes like
<Type>FF<Nucleon><q>
where <Type> can be "Scalar", "pVector", and "Sigma";
<Nucleon> "P" or "N" for proton and neutron
<q> "d", "u","s"
calcScalarQuarkFF( Mu/Md, Ms/Md, sigmaPiN[MeV], sigmaS[MeV])
calculates and rewrites Scalar form factors
*/
printf("\n======== RESET_FORMFACTORS ======\n");
printf("protonFF (default) d %.2E, u %.2E, s %.2E\n",ScalarFFPd, ScalarFFPu,ScalarFFPs);
printf("neutronFF(default) d %.2E, u %.2E, s %.2E\n",ScalarFFNd, ScalarFFNu,ScalarFFNs);
calcScalarQuarkFF(0.46,27.5,34.,42.);
// To restore default form factors of version 2 call
// calcScalarQuarkFF(0.553,18.9,55.,243.5);
printf("protonFF (new) d %.2E, u %.2E, s %.2E\n",ScalarFFPd, ScalarFFPu,ScalarFFPs);
printf("neutronFF(new) d %.2E, u %.2E, s %.2E\n",ScalarFFNd, ScalarFFNu,ScalarFFNs);
}
#endif
#ifdef CDM_NUCLEON
{ double pA0[2],pA5[2],nA0[2],nA5[2];
double Nmass=0.939; /*nucleon mass*/
double SCcoeff;
printf("\n==== Calculation of CDM-nucleons amplitudes =====\n");
nucleonAmplitudes(CDM1,NULL, pA0,pA5,nA0,nA5);
printf("CDM[antiCDM]-nucleon micrOMEGAs amplitudes:\n");
printf("proton: SI %.3E [%.3E] SD %.3E [%.3E]\n",pA0[0], pA0[1], pA5[0], pA5[1] );
printf("neutron: SI %.3E [%.3E] SD %.3E [%.3E]\n",nA0[0], nA0[1], nA5[0], nA5[1] );
SCcoeff=4/M_PI*3.8937966E8*pow(Nmass*Mcdm/(Nmass+ Mcdm),2.);
printf("CDM[antiCDM]-nucleon cross sections[pb]:\n");
printf(" proton SI %.3E [%.3E] SD %.3E [%.3E]\n",
SCcoeff*pA0[0]*pA0[0],SCcoeff*pA0[1]*pA0[1],3*SCcoeff*pA5[0]*pA5[0],3*SCcoeff*pA5[1]*pA5[1]);
printf(" neutron SI %.3E [%.3E] SD %.3E [%.3E]\n",
SCcoeff*nA0[0]*nA0[0],SCcoeff*nA0[1]*nA0[1],3*SCcoeff*nA5[0]*nA5[0],3*SCcoeff*nA5[1]*nA5[1]);
}
#endif
#ifdef CDM_NUCLEUS
{ double dNdE[300];
double nEvents;
printf("\n======== Direct Detection ========\n");
nEvents=nucleusRecoil(Maxwell,73,Z_Ge,J_Ge73,SxxGe73,NULL,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=nucleusRecoil(Maxwell,131,Z_Xe,J_Xe131,SxxXe131,NULL,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=nucleusRecoil(Maxwell,23,Z_Na,J_Na23,SxxNa23,NULL,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=nucleusRecoil(Maxwell,127,Z_I,J_I127,SxxI127,NULL,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
#ifdef NEUTRINO
{ double nu[NZ], nu_bar[NZ],mu[NZ];
double Ntot;
int forSun=1;
double Emin=0.01;
printf("\n===============Neutrino Telescope======= for ");
if(forSun) printf("Sun\n"); else printf("Earth\n");
err=neutrinoFlux(Maxwell,forSun, nu,nu_bar);
#ifdef SHOWPLOTS
displaySpectrum(nu,"nu flux from Sun [1/Year/km^2/GeV]",Emin,Mcdm);
displaySpectrum(nu_bar,"nu-bar from Sun [1/Year/km^2/GeV]",Emin,Mcdm);
#endif
{ double Ntot;
double Emin=10; //GeV
spectrInfo(Emin/Mcdm,nu, &Ntot,NULL);
printf(" E>%.1E GeV neutrino flux %.3E [1/Year/km^2] \n",Emin,Ntot);
spectrInfo(Emin/Mcdm,nu_bar, &Ntot,NULL);
printf(" E>%.1E GeV anti-neutrino flux %.3E [1/Year/km^2]\n",Emin,Ntot);
}
/* Upward events */
muonUpward(nu,nu_bar, mu);
#ifdef SHOWPLOTS
displaySpectrum(mu,"Upward muons[1/Year/km^2/GeV]",1,Mcdm/2);
#endif
{ double Ntot;
double Emin=1; //GeV
spectrInfo(Emin/Mcdm,mu, &Ntot,NULL);
printf(" E>%.1E GeV Upward muon flux %.3E [1/Year/km^2]\n",Emin,Ntot);
}
/* Contained events */
muonContained(nu,nu_bar,1., mu);
#ifdef SHOWPLOTS
displaySpectrum(mu,"Contained muons[1/Year/km^3/GeV]",Emin,Mcdm);
#endif
{ double Ntot;
double Emin=1; //GeV
spectrInfo(Emin/Mcdm,mu, &Ntot,NULL);
printf(" E>%.1E GeV Contained muon flux %.3E [1/Year/km^3]\n",Emin,Ntot);
}
}
#endif
#ifdef DECAYS
{
txtList L;
double width,br;
char * pname;
printf("\n================= Decays ==============\n");
pname = "h";
width=pWidth(pname,&L);
printf("\n%s : total width=%.3E \n and Branchings:\n",pname,width);
printTxtList(L,stdout);
pname = "~L";
width=pWidth(pname,&L);
printf("\n%s : total width=%.3E \n and Branchings:\n",pname,width);
printTxtList(L,stdout);
}
#endif
#ifdef CROSS_SECTIONS
{ double v0=0.001, Pcm=Mcdm*v0/2,cs;
int err;
numout*cc;
cc=newProcess("~n,~N->W+,W-");
passParameters(cc);
cs=v0*cs22(cc,1,0.001*Mcdm/2,-1.,1.,&err);
printf("cs=%e\n",cs);
}
#endif
killPlots();
return 0;
}
int main(int argc,char** argv)
{ int err;
char wimpName[10];
/* to save RGE input/output files uncomment the next line */
/*delFiles(0);*/
if(argc==1)
{
printf(" Correct usage: ./omg <file with parameters> \n");
exit(1);
}
err=readVar(argv[1]);
/* err=readVarRHNM(argv[1]);*/
if(err==-1) {printf("Can not open the file\n"); exit(1);}
else if(err>0) { printf("Wrong file contents at line %d\n",err);exit(1);}
err=sortOddParticles(wimpName);
if(err) { printf("Can't calculate %s\n",wimpName); return 1;}
/*to print input parameters or model in SLHA format uncomment correspondingly*/
/*
printVar(stdout);
writeLesH("slha.out");
*/
#ifdef MASSES_INFO
{
printf("\n=== MASSES OF PARTICLES OF ODD SECTOR: ===\n");
printMasses(stdout,1);
}
#endif
#ifdef CONSTRAINTS
printf("\n================= CONSTRAINTS =================\n");
#endif
#ifdef OMEGA
{ int fast=1;
double Beps=1.E-2, cut=0.01;
double Omega,Xf;
printf("\n==== Calculation of relic density =====\n");
Omega=darkOmega(&Xf,fast,Beps);
printf("Xf=%.2e Omega=%.2e\n",Xf,Omega);
printChannels(Xf,cut,Beps,1,stdout);
}
#endif
#ifdef INDIRECT_DETECTION
{ /* See hep-ph/0607059 pages 10, 11 for complete explanation */
int err,outP;
double Mwimp,Emin,Ntot,Etot,sigmaV,v=0.001,fi,tab[250];
char txt[100];
printf("\n==== Indirect detection =======\n");
outP=0; /* 0 for gamma rays
1-positron; 2-antiproton; 3,4,5 neutrinos
(electron, muon and tau correspondinly)
*/
Emin=0.1; /* Energy cut in GeV */
fi=0; /* angle of sight in radians */
sigmaV=calcSpectrum(v,outP,tab,&err);
/* Returns sigma*v in cm^3/sec.
tab could be substituted in zInterp(z,tab) to get particle distribution
in one collision dN/dz, where z=log (E/Mwinp) */
printf("sigma*v=%.2E [cm^3/sec]\n", sigmaV);
Mwimp=lopmass_();
spectrInfo(Emin/Mwimp,tab, &Ntot,&Etot);
printf("%.2E %s with E > %.2E are generated at one collision\n",Ntot,outNames[outP],Emin);
#ifdef SHOWPLOTS
/* Spectrum of photons produced in DM annihilation. */
sprintf(txt,"%s: N=%.2e,<E/2M>=%.2f,vsc=%.2e cm^3/sec,M(%s)=%.2e",
outNames[outP],Ntot,Etot,sigmaV,wimpName,Mwimp);
displaySpectrum(tab, txt ,Emin/Mwimp);
#endif
if(outP==0)
{
printf("gamma flux for fi=%.2E[rad] is %.2E[ph/cm^2/s/sr]\n",
fi, HaloFactor(fi,rhoQisotermic)*sigmaV*Ntot/Mwimp/Mwimp);
}
/* Test of energy conservation */
/*
{ double e[6];
int i;
printf("Check of energy conservation:\n");
for(i=0;i<6;i++)
{
sigmaV=calcSpectrum(v,i,tab,&err);
spectrInfo(Emin/Mwimp,tab, NULL,e+i);
}
printf("1 = %.2f\n",e[0]+2*(e[1]+e[2]+e[3]+e[4]+e[5]) );
}
*/
}
#endif
#ifdef RESET_FORMFACTORS
{
/*
The default nucleon form factors can be completely or partially modified
by setProtonFF and setNeutronFF. For scalar form factors, one can first call
getScalarFF( Mu/Md, Ms/Md, sigmaPiN[MeV], sigma0[MeV], protonFF,neutronFF)
or set the new coefficients by directly assigning numerical values.
*/
{ double ffS0P[3]={0.033,0.023,0.26},
ffS0N[3]={0.042,0.018,0.26},
ffV5P[3]={-0.427, 0.842,-0.085},
ffV5N[3]={ 0.842,-0.427,-0.085};
printf("\n=========== Redefinition of form factors =========\n");
getScalarFF(0.553,18.9,55.,35.,ffS0P, ffS0N);
printf("protonFF d %E, u %E, s %E\n",ffS0P[0],ffS0P[1],ffS0P[2]);
printf("neutronFF d %E, u %E, s %E\n",ffS0N[0],ffS0N[1],ffS0N[2]);
/* Use NULL argument if there is no need for reassignment */
setProtonFF(ffS0P,ffV5P, NULL);
setNeutronFF(ffS0N,ffV5N,NULL);
}
/* Option to change parameters of DM velocity distribution
*/
SetfMaxwell(220.,244.4,600.);
/* arg1- defines DM velocity distribution in Galaxy rest frame:
~exp(-v^2/arg1^2)d^3v
arg2- Earth velocity with respect to Galaxy
arg3- Maximal DM velocity in Sun orbit with respect to Galaxy.
All parameters are in [km/s] units.
*/
/* In case DM has velocity distribution close to delta-function
the DM velocity V[km/s] can be defined by
*/
SetfDelta(350.);
/* To reset parameters of Fermi nucleus distribution */
SetFermi(1.23,-0.6,0.52);
/* with half-density radius for Fermi distribution:
c=arg1*A^(1/3) + arg2
and arg3 is the surface thickness.
All parameter in [fm].
*/
}
#endif
#ifdef WIMP_NUCLEON
{ double pA0[2],pA5[2],nA0[2],nA5[2];
double Nmass=0.939; /*nucleon mass*/
double SCcoeff;
double dpA0[2],dnA0[2];
printf("\n==== Calculation of WIMP-nucleons amplitudes =====\n");
nucleonAmplitudes(NULL, dpA0,pA5,dnA0,nA5);
printf("====OFF/On======\n");
nucleonAmplitudes(NULL, pA0,pA5,nA0,nA5);
dpA0[0]-=pA0[0];
dnA0[0]-=nA0[0];
printf("%s -nucleon amplitudes:\n",wimpName);
printf("proton: SI %.3E SD %.3E\n",pA0[0],pA5[0]);
printf("neutron: SI %.3E SD %.3E\n",nA0[0],nA5[0]);
SCcoeff=4/M_PI*3.8937966E8*pow(Nmass*lopmass_()/(Nmass+ lopmass_()),2.);
printf("%s-nucleon cross sections:\n",wimpName);
printf(" proton SI %.3E SD %.3E\n",SCcoeff*pA0[0]*pA0[0],3*SCcoeff*pA5[0]*pA5[0]);
printf(" neutron SI %.3E SD %.3E\n",SCcoeff*nA0[0]*nA0[0],3*SCcoeff*nA5[0]*nA5[0]);
printf(" twist-2 CS proton %.3E neutron %.3E \n",
SCcoeff*dpA0[0]*dpA0[0], SCcoeff*dnA0[0]*dnA0[0]);
printf("anti-%s -nucleon amplitudes:\n",wimpName);
printf("proton: SI %.3E SD %.3E\n",pA0[1],pA5[1]);
printf("neutron: SI %.3E SD %.3E\n",nA0[1],nA5[1]);
SCcoeff=4/M_PI*3.8937966E8*pow(Nmass*lopmass_()/(Nmass+ lopmass_()),2.);
printf("anti-%s-nucleon cross sections:\n",wimpName);
printf(" proton SI %.3E SD %.3E\n",SCcoeff*pA0[1]*pA0[1],3*SCcoeff*pA5[1]*pA5[1]);
printf(" neutron SI %.3E SD %.3E\n",SCcoeff*nA0[1]*nA0[1],3*SCcoeff*nA5[1]*nA5[1]);
}
#endif
#ifdef WIMP_NUCLEUS
{ double dNdE[200];
double nEvents;
double rho=0.3; /* DM density GeV/sm^3 */
printf("\n=========== Direct Detection ===============\n");
nEvents=nucleusRecoil(rho,fDvMaxwell,73,Z_Ge,J_Ge73,S00Ge73,S01Ge73,S11Ge73,NULL,dNdE);
/* See '../sources/micromegas.h' for description of arguments
Instead of Maxwell (DvMaxwell) one can use 'fDvDelta' Delta-function
velocity distribution.
*/
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=nucleusRecoil(rho,fDvMaxwell,131,Z_Xe,J_Xe131,S00Xe131,S01Xe131,S11Xe131,NULL,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
/* If SD form factors are not known or for spin=0 nucleus one can use */
nEvents=nucleusRecoil0(rho,fDvMaxwell,3,Z_He,J_He3,Sp_He3,Sn_He3,NULL,dNdE);
printf("\n 3^He: Total number of events=%.2E /day/kg\n",nEvents);
#ifdef SHOWPLOTS
displayRecoilPlot(dNdE,"Distribution of recoil energy of 3He",0,50);
#endif
}
#endif
#ifdef CROSS_SECTIONS
{
double Pcm=500;
numout* cc;
double cosmin=-0.99, cosmax=0.99;
double v=0.002;
printf("\n====== Calculation of widths and cross sections ====\n");
decay2Info("Z",stdout);
decay2Info("H",stdout);
/* Helicity[0]=0.45;
Helicity[1]=-0.45;
printf("Process e,E->2*x at Pcm=%.3E GeV\n",Pcm);
cc=newProcess("e%,E%->2*x","eE_2x");
if(cc)
{ int ntot,l;
char * name[4];
procInfo1(cc,&ntot,NULL,NULL);
for(l=1;l<=ntot; l++)
{ int err;
double cs;
procInfo2(cc,l,name,NULL);
printf("%3s,%3s -> %3s %3s ",name[0],name[1],name[2],name[3]);
cs= cs22(cc,l,Pcm,cosmin,cosmax,&err);
if(err) printf("Error\n");
else if(cs==0.) printf("Zero\n");
else printf("%.2E [pb]\n",cs);
}
}
*/
printf("\n WIMP annihilation at V_rel=%.2E\n",v);
cc=newProcess("",wimpAnnLib());
assignValW("Q",2*lopmass_());
if(cc)
{ int ntot,l;
char * name[4];
double mass[4];
procInfo1(cc,&ntot,NULL,NULL);
for(l=1;l<=ntot; l++)
{ int err;
double cs;
procInfo2(cc,l,name,mass);
if(l==1) { Pcm=mass[0]*v/2; printf("(Pcm=%.2E)\n",Pcm);}
printf("%3s,%3s -> %3s %3s ",name[0],name[1],name[2],name[3]);
cs= cs22(cc,l,Pcm,-1.,1.,&err);
if(err) printf("Error\n");
else if(cs==0.) printf("Zero\n");
else printf("%.2E [pb] ( sigma*v=%.2E [cm^3/sec] ) \n",cs,cs*v*2.9979E-26);
}
}
}
#endif
return 0;
}
int main(int argc,char** argv)
{ int err;
char cdmName[10];
int spin2, charge3,cdim;
ForceUG=0; /* to Force Unitary Gauge assign 1 */
/*
gauss345_arg(ff,Y,0,1,1E-5,&err);
printf("err=%d\n",err);
exit(0);
*/
VZdecay=1; VWdecay=1;
if(argc==1)
{
printf(" Correct usage: ./main <file with parameters> \n");
printf("Example: ./main data1.par\n");
exit(1);
}
err=readVar(argv[1]);
if(err==-1) {printf("Can not open the file\n"); exit(1);}
else if(err>0) { printf("Wrong file contents at line %d\n",err);exit(1);}
err=sortOddParticles(cdmName);
if(err) { printf("Can't calculate %s\n",cdmName); return 1;}
if(CDM1)
{
qNumbers(CDM1, &spin2, &charge3, &cdim);
printf("\nDark matter candidate is '%s' with spin=%d/2 mass=%.2E\n",CDM1, spin2,Mcdm1);
if(charge3) printf("Dark Matter has electric charge %d/3\n",charge3);
if(cdim!=1) printf("Dark Matter is a color particle\n");
}
if(CDM2)
{
qNumbers(CDM2, &spin2, &charge3, &cdim);
printf("\nDark matter candidate is '%s' with spin=%d/2 mass=%.2E\n",CDM2,spin2,Mcdm2);
if(charge3) printf("Dark Matter has electric charge %d/3\n",charge3);
if(cdim!=1) printf("Dark Matter is a color particle\n");
}
#ifdef MASSES_INFO
{
printf("\n=== MASSES OF HIGGS AND ODD PARTICLES: ===\n");
printHiggs(stdout);
printMasses(stdout,1);
}
#endif
#ifdef CONSTRAINTS
{ double csLim;
if(Zinvisible()) printf("Excluded by Z->invizible\n");
if(LspNlsp_LEP(&csLim)) printf("LEP excluded by e+,e- -> DM q q-\\bar Cross Section= %.2E pb\n",csLim);
}
#endif
#ifdef MONOJET
{ double CL=monoJet();
printf(" Monojet signal exclusion CL is %.3e\n", CL);
}
#endif
#if defined(HIGGSBOUNDS) || defined(HIGGSSIGNALS)
{ int NH0,NHch; // number of neutral and charged Higgs particles.
double HB_result,HB_obsratio,HS_observ,HS_chi2, HS_pval;
char HB_chan[100]={""}, HB_version[50], HS_version[50];
NH0=hbBlocksMO("HB.in",&NHch);
system("echo 'BLOCK DMASS\n 25 2 '>> HB.in");
#include "../include/hBandS.inc"
#ifdef HIGGSBOUNDS
printf("HB(%s): result=%.0f obsratio=%.2E channel= %s \n", HB_version,HB_result,HB_obsratio,HB_chan);
#endif
#ifdef HIGGSSIGNALS
printf("HS(%s): Nobservables=%.0f chi^2 = %.2E pval= %.2E\n",HS_version,HS_observ,HS_chi2, HS_pval);
#endif
}
#endif
#ifdef LILITH
{ double m2logL, m2logL_reference=0,pvalue;
int exp_ndf,n_par=0,ndf;
char call_lilith[100], Lilith_version[20];
if(LilithMO("Lilith_in.xml"))
{
#include "../include/Lilith.inc"
if(ndf)
{
printf("LILITH(DB%s): -2*log(L): %.2f; -2*log(L_reference): %.2f; ndf: %d; p-value: %.2E \n",
Lilith_version,m2logL,m2logL_reference,ndf,pvalue);
}
} else printf("LILITH: there is no Higgs candidate\n");
}
#endif
#ifdef SMODELS
{ int result=0;
double Rvalue=0;
char analysis[30]={},topology[30]={};
int LHCrun=LHC8|LHC13; // LHC8 - 8TeV; LHC13 - 13TeV;
#include "../include/SMODELS.inc"
}
#endif
#ifdef OMEGA
{ int fast=1;
double Beps=1.E-4, cut=0.01;
double Omega;
int i,err;
printf("\n==== Calculation of relic density =====\n");
if(CDM1 && CDM2)
{
Omega= darkOmega2(fast,Beps);
printf("Omega_1h^2=%.2E\n", Omega*(1-fracCDM2));
printf("Omega_2h^2=%.2E\n", Omega*fracCDM2);
} else
{ double Xf;
Omega=darkOmega(&Xf,fast,Beps,&err);
printf("Xf=%.2e Omega=%.2e\n",Xf,Omega);
if(Omega>0)printChannels(Xf,cut,Beps,1,stdout);
}
}
#endif
#ifdef FREEZEIN
{
double TR=1E10;
double omegaFi;
toFeebleList("~s0");
VWdecay=0; VZdecay=0;
omegaFi=darkOmegaFi(TR,&err);
printf("omega freeze-in=%.3E\n", omegaFi);
printChannelsFi(0,0,stdout);
}
#endif
#ifdef INDIRECT_DETECTION
{
int err,i;
double Emin=1,/* Energy cut in GeV */ sigmaV;
double vcs_gz,vcs_gg;
char txt[100];
double SpA[NZ],SpE[NZ],SpP[NZ];
double FluxA[NZ],FluxE[NZ],FluxP[NZ];
double * SpNe=NULL,*SpNm=NULL,*SpNl=NULL;
double Etest=Mcdm/2;
printf("\n==== Indirect detection =======\n");
sigmaV=calcSpectrum(1+2+4,SpA,SpE,SpP,SpNe,SpNm,SpNl ,&err);
/* Returns sigma*v in cm^3/sec. SpX - calculated spectra of annihilation.
Use SpectdNdE(E, SpX) to calculate energy distribution in 1/GeV units.
First parameter 1-includes W/Z polarization
2-includes gammas for 2->2+gamma
4-print cross sections
*/
{
double fi=0.1,dfi=0.05; /* 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 for angle of sight %.2f[rad] and cone angle %.2f[rad]",fi,2*dfi);
displayPlot(txt,"E[GeV]",Emin,Mcdm,0,1,"",0,SpectdNdE,FluxA);
#endif
printf("Photon flux = %.2E[cm^2 s GeV]^{-1} for E=%.1f[GeV]\n",SpectdNdE(Etest, FluxA), Etest);
}
{
posiFluxTab(Emin, sigmaV, SpE, FluxE);
#ifdef SHOWPLOTS
displayPlot("positron flux [cm^2 s sr GeV]^{-1}","E[GeV]",Emin,Mcdm,0,1,"",0,SpectdNdE,FluxE);
#endif
printf("Positron flux = %.2E[cm^2 sr s GeV]^{-1} for E=%.1f[GeV] \n",
SpectdNdE(Etest, FluxE), Etest);
}
{
pbarFluxTab(Emin, sigmaV, SpP, FluxP );
#ifdef SHOWPLOTS
displayPlot("antiproton flux [cm^2 s sr GeV]^{-1}","E[GeV]",Emin,Mcdm,0,1,"",0,SpectdNdE,FluxP);
#endif
printf("Antiproton flux = %.2E[cm^2 sr s GeV]^{-1} for E=%.1f[GeV] \n",
SpectdNdE(Etest, FluxP), Etest);
}
}
#endif
#ifdef RESET_FORMFACTORS
{
/*
The user has approach to form factors which specifies quark contents
of proton and nucleon via global parametes like
<Type>FF<Nucleon><q>
where <Type> can be "Scalar", "pVector", and "Sigma";
<Nucleon> "P" or "N" for proton and neutron
<q> "d", "u","s"
calcScalarQuarkFF( Mu/Md, Ms/Md, sigmaPiN[MeV], sigma0[MeV])
calculates and rewrites Scalar form factors
*/
printf("\n======== RESET_FORMFACTORS ======\n");
printf("protonFF (default) d %.2E, u %.2E, s %.2E\n",ScalarFFPd, ScalarFFPu,ScalarFFPs);
printf("neutronFF(default) d %.2E, u %.2E, s %.2E\n",ScalarFFNd, ScalarFFNu,ScalarFFNs);
// To restore default form factors of version 2 call
calcScalarQuarkFF(0.553,18.9,55.,243.5);
printf("protonFF (new) d %.2E, u %.2E, s %.2E\n",ScalarFFPd, ScalarFFPu,ScalarFFPs);
printf("neutronFF(new) d %.2E, u %.2E, s %.2E\n",ScalarFFNd, ScalarFFNu,ScalarFFNs);
// To restore default form factors current version call
// calcScalarQuarkFF(0.56,20.2,34,42);
}
#endif
#ifdef CDM_NUCLEON
{ double pA0[2],pA5[2],nA0[2],nA5[2];
double Nmass=0.939; /*nucleon mass*/
double SCcoeff;
printf("\n==== Calculation of CDM-nucleons amplitudes =====\n");
if(CDM1)
{
nucleonAmplitudes(CDM1, pA0,pA5,nA0,nA5);
printf("CDM[antiCDM]-nucleon micrOMEGAs amplitudes for %s \n",CDM1);
printf("proton: SI %.3E [%.3E] SD %.3E [%.3E]\n",pA0[0], pA0[1], pA5[0], pA5[1] );
printf("neutron: SI %.3E [%.3E] SD %.3E [%.3E]\n",nA0[0], nA0[1], nA5[0], nA5[1] );
SCcoeff=4/M_PI*3.8937966E8*pow(Nmass*Mcdm/(Nmass+ Mcdm),2.);
printf("CDM[antiCDM]-nucleon cross sections[pb]:\n");
printf(" proton SI %.3E [%.3E] SD %.3E [%.3E]\n",
SCcoeff*pA0[0]*pA0[0],SCcoeff*pA0[1]*pA0[1],3*SCcoeff*pA5[0]*pA5[0],3*SCcoeff*pA5[1]*pA5[1]);
printf(" neutron SI %.3E [%.3E] SD %.3E [%.3E]\n",
SCcoeff*nA0[0]*nA0[0],SCcoeff*nA0[1]*nA0[1],3*SCcoeff*nA5[0]*nA5[0],3*SCcoeff*nA5[1]*nA5[1]);
}
if(CDM2)
{
nucleonAmplitudes(CDM2, pA0,pA5,nA0,nA5);
printf("CDM[antiCDM]-nucleon micrOMEGAs amplitudes for %s \n",CDM2);
printf("proton: SI %.3E [%.3E] SD %.3E [%.3E]\n",pA0[0], pA0[1], pA5[0], pA5[1] );
printf("neutron: SI %.3E [%.3E] SD %.3E [%.3E]\n",nA0[0], nA0[1], nA5[0], nA5[1] );
SCcoeff=4/M_PI*3.8937966E8*pow(Nmass*Mcdm/(Nmass+ Mcdm),2.);
printf("CDM[antiCDM]-nucleon cross sections[pb]:\n");
printf(" proton SI %.3E [%.3E] SD %.3E [%.3E]\n",
SCcoeff*pA0[0]*pA0[0],SCcoeff*pA0[1]*pA0[1],3*SCcoeff*pA5[0]*pA5[0],3*SCcoeff*pA5[1]*pA5[1]);
printf(" neutron SI %.3E [%.3E] SD %.3E [%.3E]\n",
SCcoeff*nA0[0]*nA0[0],SCcoeff*nA0[1]*nA0[1],3*SCcoeff*nA5[0]*nA5[0],3*SCcoeff*nA5[1]*nA5[1]);
}
}
#endif
#ifdef CDM_NUCLEUS
{ double dNdE[300];
double nEvents;
printf("\n======== Direct Detection ========\n");
nEvents=nucleusRecoil(Maxwell,73,Z_Ge,J_Ge73,SxxGe73,NULL,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
displayPlot("Distribution of recoil energy of 73Ge","E[KeV]",0,200,0,1,"dN/dE",0,dNdERecoil,dNdE);
#endif
nEvents=nucleusRecoil(Maxwell,131,Z_Xe,J_Xe131,SxxXe131,NULL,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
displayPlot("Distribution of recoil energy of 131Xe","E[KeV]",0,200,0,1,"dN/dE",0,dNdERecoil,dNdE);
#endif
nEvents=nucleusRecoil(Maxwell,23,Z_Na,J_Na23,SxxNa23,NULL,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
displayPlot("Distribution of recoil energy of 23Na","E[KeV]",0,200,0,1,"dN/dE",0,dNdERecoil,dNdE);
#endif
nEvents=nucleusRecoil(Maxwell,127,Z_I,J_I127,SxxI127,NULL,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
displayPlot("Distribution of recoil energy of 127I","E[KeV]",0,200,0,1,"dN/dE",0,dNdERecoil,dNdE);
#endif
}
#endif
#ifdef NEUTRINO
if(!CDM1 || !CDM2)
{ double nu[NZ], nu_bar[NZ],mu[NZ];
double Ntot;
int forSun=1;
double Emin=1;
printf("\n===============Neutrino Telescope======= for ");
if(forSun) printf("Sun\n"); else printf("Earth\n");
err=neutrinoFlux(Maxwell,forSun, nu,nu_bar);
#ifdef SHOWPLOTS
displayPlot("neutrino fluxes [1/Year/km^2/GeV]","E[GeV]",Emin,Mcdm,0, 2,"dnu/dE",0,SpectdNdE,nu,"dnu_bar/dE",0,SpectdNdE,nu_bar);
#endif
{
printf(" E>%.1E GeV neutrino flux %.2E [1/Year/km^2] \n",Emin,spectrInfo(Emin,nu,NULL));
printf(" E>%.1E GeV anti-neutrino flux %.2E [1/Year/km^2]\n",Emin,spectrInfo(Emin,nu_bar,NULL));
}
/* Upward events */
muonUpward(nu,nu_bar, mu);
#ifdef SHOWPLOTS
displayPlot("Upward muons[1/Year/km^2/GeV]","E",Emin,Mcdm/2, 0,1,"mu",0,SpectdNdE,mu);
#endif
printf(" E>%.1E GeV Upward muon flux %.2E [1/Year/km^2]\n",Emin,spectrInfo(Emin,mu,NULL));
/* Contained events */
muonContained(nu,nu_bar,1., mu);
#ifdef SHOWPLOTS
displayPlot("Contained muons[1/Year/km^3/GeV]","E",Emin,Mcdm,0,1,"",0,SpectdNdE,mu);
#endif
printf(" E>%.1E GeV Contained muon flux %.2E [1/Year/km^3]\n",Emin,spectrInfo(Emin/Mcdm,mu,NULL));
}
#endif
#ifdef DECAYS
{ char* pname = pdg2name(25);
txtList L;
double width;
if(pname)
{
width=pWidth(pname,&L);
printf("\n%s : total width=%E \n and Branchings:\n",pname,width);
printTxtList(L,stdout);
}
pname = pdg2name(24);
if(pname)
{
width=pWidth(pname,&L);
printf("\n%s : total width=%E \n and Branchings:\n",pname,width);
printTxtList(L,stdout);
}
}
#endif
#ifdef CROSS_SECTIONS
{
char* next,next_;
double nextM;
next=nextOdd(1,&nextM);
if(next && nextM<1000)
{
double cs, Pcm=6500, Qren, Qfact, pTmin=0;
int nf=3;
char*next_=antiParticle(next);
Qren=Qfact=nextM;
printf("\npp > nextOdd at sqrt(s)=%.2E GeV\n",2*Pcm);
Qren=Qfact;
cs=hCollider(Pcm,1,nf,Qren, Qfact, next,next_,pTmin,1);
printf("Production of 'next' odd particle: cs(pp-> %s,%s)=%.2E[pb]\n",next,next_, cs);
}
}
#endif
#ifdef CLEAN
system("rm -f HB.* HB.* hb.* hs.* debug_channels.txt debug_predratio.txt Key.dat");
system("rm -f Lilith_* particles.py*");
system("rm -f smodels.in smodels.log smodels.out summary.*");
#endif
killPlots();
return 0;
}
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;
}
int main(int argc,char** argv)
{ int err;
char cdmName[10];
int spin2, charge3,cdim;
ForceUG=0; // to Force Unitary Gauge assign 1
if(argc==1)
{
printf(" Correct usage: ./main <file with parameters> \n");
printf("Example: ./main data1.par\n");
exit(1);
}
err=readVar(argv[1]);
if(err==-1) {
printf("Can not open the file\n");
exit(1);
}
else if(err>0) {
printf("Wrong file contents at line %d\n",err);
exit(1);
}
err=sortOddParticles(cdmName);
if(err) {
printf("Can't calculate %s\n",cdmName);
return 1;
}
qNumbers(cdmName, &spin2, &charge3, &cdim);
printf("\nDark matter candidate is '%s' with spin=%d/2\n",
cdmName, spin2);
if(charge3) {
printf("Dark Matter has electric charge %d*3\n",charge3);
exit(1);
}
if(cdim!=1) {
printf("Dark Matter ia a color particle\n");
exit(1);
}
#ifdef MASSES_INFO
{
printf("\n=== MASSES OF HIGG AND ODD PARTICLES: ===\n");
printHiggs(stdout);
printMasses(stdout,1);
}
#endif
#ifdef HIGGSBOUNDS
if(access(HIGGSBOUNDS "/HiggsBounds",X_OK )) system( "cd " HIGGSBOUNDS "; ./configure; make ");
HBblocks("HB.in");
system(HIGGSBOUNDS "/HiggsBounds LandH SLHA 1 0 HB.in HB.out > hb.stdout");
slhaRead("HB.out",1+4);
printf("HB result= %.0E obsratio=%.2E\n",slhaValFormat("HiggsBoundsResults",0.,"1 2 %lf"), slhaValFormat("HiggsBoundsResults",0.,"1 3 %lf" ) );
{ char hbInfo[100];
if(0==slhaSTRFormat("HiggsBoundsResults","1 5 ||%[^|]||",hbInfo)) printf("Channel: %s\n",hbInfo);
}
#endif
#ifdef HIGGSSIGNALS
#define DataSet " latestresults "
//#define Method " peak "
//#define Method " mass "
#define Method " both "
#define PDF " 2 " // Gaussian
//#define PDF " 1 " // box
//#define PDF " 3 " // box+Gaussia
#define dMh " 2 "
printf("HiggsSignals:\n");
if(access(HIGGSSIGNALS "/HiggsSignals",X_OK )) system( "cd " HIGGSSIGNALS "; ./configure; make ");
system("rm -f HS.in HS.out");
HBblocks("HS.in");
system(HIGGSSIGNALS "/HiggsSignals" DataSet Method PDF " SLHA 1 0 HS.in > hs.stdout");
system("grep -A 10000 HiggsSignalsResults HS.in > HS.out");
slhaRead("HS.out",1+4);
printf(" Number of observables %.0f\n",slhaVal("HiggsSignalsResults",0.,1,7));
printf(" total chi^2= %.1E\n",slhaVal("HiggsSignalsResults",0.,1,12));
printf(" HS p-value = %.1E\n", slhaVal("HiggsSignalsResults",0.,1,13));
#undef dMh
#undef PDF
#undef Method
#undef DataSet
#endif
#ifdef OMEGA
{ int fast=1;
double Beps=1.E-5, cut=0.01;
double Omega,Xf;
int i;
// to exclude processes with virtual W/Z in DM annihilation
VZdecay=0;
VWdecay=0;
cleanDecayTable();
// to include processes with virtual W/Z also in co-annihilation
// VZdecay=2; VWdecay=2; cleanDecayTable();
printf("\n==== Calculation of relic density =====\n");
Omega=darkOmega(&Xf,fast,Beps);
printf("Xf=%.2e Omega=%.2e\n",Xf,Omega);
printChannels(Xf,cut,Beps,1,stdout);
// VZdecay=1; VWdecay=1; cleanDecayTable(); // restore default
}
#endif
#ifdef INDIRECT_DETECTION
{
int err,i;
double Emin=1,/* Energy cut in GeV */ sigmaV;
double vcs_gz,vcs_gg;
char txt[100];
double SpA[NZ],SpE[NZ],SpP[NZ];
double FluxA[NZ],FluxE[NZ],FluxP[NZ];
double * SpNe=NULL,*SpNm=NULL,*SpNl=NULL;
double Etest=Mcdm/2;
printf("\n==== Indirect detection =======\n");
sigmaV=calcSpectrum(4,SpA,SpE,SpP,SpNe,SpNm,SpNl ,&err);
/* Returns sigma*v in cm^3/sec. SpX - calculated spectra of annihilation.
Use SpectdNdE(E, SpX) to calculate energy distribution in 1/GeV units.
First parameter 1-includes W/Z polarization
2-includes gammas for 2->2+gamma
4-print cross sections
*/
printf("sigmav=%.2E[cm^3/s]\n",sigmaV);
if(SpA)
{
double fi=0.1,dfi=0.05; /* 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(FluxA,txt,Emin,Mcdm);
#endif
printf("Photon flux = %.2E[cm^2 s GeV]^{-1} for E=%.1f[GeV]\n",SpectdNdE(Etest, FluxA), Etest);
}
if(SpE)
{
posiFluxTab(Emin, sigmaV, SpE, FluxE);
#ifdef SHOWPLOTS
displaySpectrum(FluxE,"positron flux [cm^2 s sr GeV]^{-1}" ,Emin,Mcdm);
#endif
printf("Positron flux = %.2E[cm^2 sr s GeV]^{-1} for E=%.1f[GeV] \n",
SpectdNdE(Etest, FluxE), Etest);
}
if(SpP)
{
pbarFluxTab(Emin, sigmaV, SpP, FluxP );
#ifdef SHOWPLOTS
displaySpectrum(FluxP,"antiproton flux [cm^2 s sr GeV]^{-1}" ,Emin, Mcdm);
#endif
printf("Antiproton flux = %.2E[cm^2 sr s GeV]^{-1} for E=%.1f[GeV] \n",
SpectdNdE(Etest, FluxP), Etest);
}
}
#endif
#ifdef RESET_FORMFACTORS
{
/*
The user has approach to form factors which specifies quark contents
of proton and nucleon via global parametes like
<Type>FF<Nucleon><q>
where <Type> can be "Scalar", "pVector", and "Sigma";
<Nucleon> "P" or "N" for proton and neutron
<q> "d", "u","s"
calcScalarFF( Mu/Md, Ms/Md, sigmaPiN[MeV], sigma0[MeV])
calculates and rewrites Scalar form factors
*/
printf("\n======== RESET_FORMFACTORS ======\n");
printf("protonFF (default) d %.2E, u %.2E, s %.2E\n",ScalarFFPd, ScalarFFPu,ScalarFFPs);
printf("neutronFF(default) d %.2E, u %.2E, s %.2E\n",ScalarFFNd, ScalarFFNu,ScalarFFNs);
// To restore default form factors of version 2 call
// calcScalarQuarkFF(0.553,18.9,55.,243.5);
calcScalarFF(0.553,18.9,70.,35.);
printf("protonFF (new) d %.2E, u %.2E, s %.2E\n",ScalarFFPd, ScalarFFPu,ScalarFFPs);
printf("neutronFF(new) d %.2E, u %.2E, s %.2E\n",ScalarFFNd, ScalarFFNu,ScalarFFNs);
}
#endif
#ifdef CDM_NUCLEON
{ double pA0[2],pA5[2],nA0[2],nA5[2];
double Nmass=0.939; /*nucleon mass*/
double SCcoeff;
int i;
printf("\n==== Calculation of CDM-nucleons amplitudes =====\n");
nucleonAmplitudes(CDM1,NULL, pA0,pA5,nA0,nA5);
printf("CDM[antiCDM]-nucleon micrOMEGAs amplitudes:\n");
printf("proton: SI %.3E [%.3E] SD %.3E [%.3E]\n",pA0[0], pA0[1], pA5[0], pA5[1] );
printf("neutron: SI %.3E [%.3E] SD %.3E [%.3E]\n",nA0[0], nA0[1], nA5[0], nA5[1] );
SCcoeff=4/M_PI*3.8937966E8*pow(Nmass*Mcdm/(Nmass+ Mcdm),2.);
printf("CDM[antiCDM]-nucleon cross sections[pb]:\n");
printf(" proton SI %.3E [%.3E] SD %.3E [%.3E]\n",
SCcoeff*pA0[0]*pA0[0],SCcoeff*pA0[1]*pA0[1],3*SCcoeff*pA5[0]*pA5[0],3*SCcoeff*pA5[1]*pA5[1]);
printf(" neutron SI %.3E [%.3E] SD %.3E [%.3E]\n",
SCcoeff*nA0[0]*nA0[0],SCcoeff*nA0[1]*nA0[1],3*SCcoeff*nA5[0]*nA5[0],3*SCcoeff*nA5[1]*nA5[1]);
}
#endif
#ifdef CDM_NUCLEUS
{ double dNdE[300];
double nEvents;
printf("\n======== Direct Detection ========\n");
nEvents=nucleusRecoil(Maxwell,73,Z_Ge,J_Ge73,SxxGe73,NULL,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=nucleusRecoil(Maxwell,131,Z_Xe,J_Xe131,SxxXe131,NULL,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=nucleusRecoil(Maxwell,23,Z_Na,J_Na23,SxxNa23,NULL,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=nucleusRecoil(Maxwell,127,Z_I,J_I127,SxxI127,NULL,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
#ifdef NEUTRINO
{ double nu[NZ], nu_bar[NZ],mu[NZ];
double Ntot;
int forSun=1;
double Emin=0.01;
printf("\n===============Neutrino Telescope======= for ");
if(forSun) printf("Sun\n");
else printf("Earth\n");
err=neutrinoFlux(Maxwell,forSun, nu,nu_bar);
#ifdef SHOWPLOTS
displaySpectrum(nu,"nu flux from Sun [1/Year/km^2/GeV]",Emin,Mcdm);
displaySpectrum(nu_bar,"nu-bar from Sun [1/Year/km^2/GeV]",Emin,Mcdm);
#endif
{ double Ntot;
double Emin=10; //GeV
spectrInfo(Emin/Mcdm,nu, &Ntot,NULL);
printf(" E>%.1E GeV neutrino flux %.3E [1/Year/km^2] \n",Emin,Ntot);
spectrInfo(Emin/Mcdm,nu_bar, &Ntot,NULL);
printf(" E>%.1E GeV anti-neutrino flux %.3E [1/Year/km^2]\n",Emin,Ntot);
}
/* Upward events */
muonUpward(nu,nu_bar, mu);
#ifdef SHOWPLOTS
displaySpectrum(mu,"Upward muons[1/Year/km^2/GeV]",1,Mcdm/2);
#endif
{ double Ntot;
double Emin=1; //GeV
spectrInfo(Emin/Mcdm,mu, &Ntot,NULL);
printf(" E>%.1E GeV Upward muon flux %.3E [1/Year/km^2]\n",Emin,Ntot);
}
/* Contained events */
muonContained(nu,nu_bar,1., mu);
#ifdef SHOWPLOTS
displaySpectrum(mu,"Contained muons[1/Year/km^3/GeV]",Emin,Mcdm);
#endif
{ double Ntot;
double Emin=1; //GeV
spectrInfo(Emin/Mcdm,mu, &Ntot,NULL);
printf(" E>%.1E GeV Contained muon flux %.3E [1/Year/km^3]\n",Emin,Ntot);
}
}
#endif
#ifdef DECAYS
{
txtList L;
double width,br;
char * pname;
printf("\n================= Decays ==============\n");
pname = "H";
width=pWidth(pname,&L);
printf("\n%s : total width=%.2E \n and Branchings:\n",pname,width);
printTxtList(L,stdout);
pname = "~W+";
width=pWidth(pname,&L);
printf("\n%s : total width=%.2E \n and Branchings:\n",pname,width);
printTxtList(L,stdout);
}
#endif
#ifdef CLEAN
system("rm -f HB.in HB.out HS.in HS.out hb.stdout hs.stdout debug_channels.txt debug_predratio.txt Key.dat");
killPlots();
#endif
return 0;
}
double spectrinfo_(double *Xmin,double*tab, double*Etot)
{ return spectrInfo(*Xmin,tab, Etot);}
int main(int argc,char** argv)
{ int err;
char cdmName[10];
int spin2, charge3,cdim;
// sysTimeLim=1000;
ForceUG=0; /* to Force Unitary Gauge assign 1 */
// nPROCSS=0; /* to switch off multiprocessor calculations */
/*
if you would like to work with superIso
setenv("superIso","./superiso_v3.1",1);
*/
#ifdef SUGRA
{
double m0,mhf,a0,tb;
double gMG1, gMG2, gMG3, gAl, gAt, gAb, sgn, gMHu, gMHd,
gMl2, gMl3, gMr2, gMr3, gMq2, gMq3, gMu2, gMu3, gMd2, gMd3;
printf("\n========= mSUGRA scenario =====\n");
PRINTRGE(RGE);
if(argc<5)
{
printf(" This program needs 4 parameters:\n"
" m0 common scalar mass at GUT scale\n"
" mhf common gaugino mass at GUT scale\n"
" a0 trilinear soft breaking parameter at GUT scale\n"
" tb tan(beta) \n");
printf(" Auxiliary parameters are:\n"
" sgn +/-1, sign of Higgsino mass term (default 1)\n"
" Mtp top quark pole mass\n"
" MbMb Mb(Mb) scale independent b-quark mass\n"
" alfSMZ strong coupling at MZ\n");
/* printf("Example: ./main 70 250 -300 10\n"); */
printf("Example: ./main 120 500 -350 10 1 173.1 \n");
exit(1);
} else
{ double Mtp,MbMb,alfSMZ;
sscanf(argv[1],"%lf",&m0);
sscanf(argv[2],"%lf",&mhf);
sscanf(argv[3],"%lf",&a0);
sscanf(argv[4],"%lf",&tb);
if(argc>5)sscanf(argv[5],"%lf",&sgn); else sgn=1;
if(argc>6){ sscanf(argv[6],"%lf",&Mtp); assignValW("Mtp",Mtp); }
if(argc>7){ sscanf(argv[7],"%lf",&MbMb); assignValW("MbMb",MbMb); }
if(argc>8){ sscanf(argv[8],"%lf",&alfSMZ); assignValW("alfSMZ",alfSMZ);}
}
/*==== simulation of mSUGRA =====*/
gMG1=mhf, gMG2=mhf,gMG3=mhf;
gAl=a0, gAt=a0, gAb=a0; gMHu=m0, gMHd=m0;
gMl2=m0, gMl3=m0, gMr2=m0, gMr3=m0;
gMq2=m0, gMq3=m0, gMu2=m0, gMd2=m0, gMu3=m0, gMd3=m0;
err= SUGRAMODEL(RGE) (tb,
gMG1, gMG2, gMG3, gAl, gAt, gAb, sgn, gMHu, gMHd,
gMl2, gMl3, gMr2, gMr3, gMq2, gMq3, gMu2, gMu3, gMd2, gMd3);
}
#elif defined(SUGRANUH)
{
double m0,mhf,a0,tb;
double gMG1, gMG2, gMG3, gAl, gAt, gAb, gMl2, gMl3, gMr2, gMr3, gMq2, gMq3, gMu2, gMu3, gMd2, gMd3,mu,MA;
printf("\n========= mSUGRA non-universal Higgs scenario =====\n");
PRINTRGE(RGE);
if(argc<7)
{
printf(" This program needs 6 parameters:\n"
" m0 common scalar mass at GUT scale\n"
" mhf common gaugino mass at GUT scale\n"
" a0 trilinear soft breaking parameter at GUT scale\n"
" tb tan(beta) \n"
" mu mu(EWSB)\n"
" MA mass of pseudoscalar Higgs\n");
printf(" Auxiliary parameters are:\n"
" Mtp top quark pole mass\n"
" MbMb Mb(Mb) scale independent b-quark mass\n"
" alfSMZ strong coupling at MZ\n");
/* printf("Example: ./main 70 250 -300 10\n"); */
printf("Example: ./main 120 500 -350 10 680 760 \n");
exit(1);
} else
{ double Mtp,MbMb,alfSMZ;
sscanf(argv[1],"%lf",&m0);
sscanf(argv[2],"%lf",&mhf);
sscanf(argv[3],"%lf",&a0);
sscanf(argv[4],"%lf",&tb);
sscanf(argv[5],"%lf",&mu);
sscanf(argv[6],"%lf",&MA);
if(argc>7){ sscanf(argv[7],"%lf",&Mtp); assignValW("Mtp",Mtp); }
if(argc>8){ sscanf(argv[8],"%lf",&MbMb); assignValW("MbMb",MbMb); }
if(argc>9){ sscanf(argv[9],"%lf",&alfSMZ); assignValW("alfSMZ",alfSMZ);}
}
/*==== simulation of mSUGRA =====*/
gMG1=mhf, gMG2=mhf,gMG3=mhf;
gAl=a0, gAt=a0, gAb=a0;
gMl2=m0, gMl3=m0, gMr2=m0, gMr3=m0;
gMq2=m0, gMq3=m0, gMu2=m0, gMd2=m0, gMu3=m0, gMd3=m0;
err= SUGRANUHMODEL(RGE) (tb,gMG1,gMG2,gMG3,gAl,gAt,gAb,gMl2,gMl3,gMr2,gMr3,gMq2,gMq3,gMu2,gMu3,gMd2,gMd3,mu,MA);
}
#elif defined(AMSB)
{
double m0,m32,sgn,tb;
printf("\n========= AMSB scenario =====\n");
PRINTRGE(RGE);
if(argc<4)
{
printf(" This program needs 3 parameters:\n"
" m0 common scalar mass at GUT scale\n"
" m3/2 gravitino mass\n"
" tb tan(beta) \n");
printf(" Auxiliary parameters are:\n"
" sgn +/-1, sign of Higgsino mass term (default 1)\n"
" Mtp top quark pole mass\n"
" MbMb Mb(Mb) scale independent b-quark mass\n"
" alfSMZ strong coupling at MZ\n");
printf("Example: ./main 450 60000 10\n");
exit(1);
} else
{ double Mtp,MbMb,alfSMZ;
sscanf(argv[1],"%lf",&m0);
sscanf(argv[2],"%lf",&m32);
sscanf(argv[3],"%lf",&tb);
if(argc>4)sscanf(argv[4],"%lf",&sgn); else sgn=1;
if(argc>5){ sscanf(argv[5],"%lf",&Mtp); assignValW("Mtp",Mtp); }
if(argc>6){ sscanf(argv[6],"%lf",&MbMb); assignValW("MbMb",MbMb); }
if(argc>7){ sscanf(argv[7],"%lf",&alfSMZ); assignValW("alfSMZ",alfSMZ);}
}
err= AMSBMODEL(RGE)(m0,m32,tb,sgn);
}
#elif defined(EWSB)
{
printf("\n========= EWSB scale input =========\n");
PRINTRGE(RGE);
if(argc <2)
{ printf("The program needs one argument:the name of file with MSSM parameters.\n"
"Example: ./main mssm1.par \n");
exit(1);
}
printf("Initial file \"%s\"\n",argv[1]);
err=readVarMSSM(argv[1]);
if(err==-1) { printf("Can not open the file\n"); exit(2);}
else if(err>0) { printf("Wrong file contents at line %d\n",err);exit(3);}
err=EWSBMODEL(RGE)();
}
#else
{
printf("\n========= SLHA file input =========\n");
if(argc <2)
{ printf("The program needs one argument:the name of SLHA input file.\n"
"Example: ./main suspect2_lha.out \n");
exit(1);
}
printf("Initial file \"%s\"\n",argv[1]);
err=lesHinput(argv[1]);
if(err) exit(2);
}
#endif
if(err==-1) { printf("Can not open the file\n"); exit(2);}
else if(err>0) { printf("Wrong file contents at line %d\n",err);exit(3);}
{ int nw;
printf("Warnings from spectrum calculator:\n");
nw=slhaWarnings(stdout);
if(nw==0) printf(" .....none\n");
}
if(err) exit(1);
err=sortOddParticles(cdmName);
if(err) { printf("Can't calculate %s\n",cdmName); return 1;}
qNumbers(cdmName,&spin2, &charge3, &cdim);
printf("\nDark matter candidate is '%s' with spin=%d/2 mass=%.2E\n",
cdmName, spin2, Mcdm);
if(charge3) { printf("Dark Matter has electric charge %d/3\n",charge3); exit(1);}
if(cdim!=1) { printf("Dark Matter is a color particle\n"); exit(1);}
if(strcmp(cdmName,"~o1")) printf(" ~o1 is not CDM\n");
else o1Contents(stdout);
#ifdef MASSES_INFO
{
printf("\n=== MASSES OF HIGGS AND SUSY PARTICLES: ===\n");
printHiggs(stdout);
printMasses(stdout,1);
}
#endif
#ifdef CONSTRAINTS
{ double SMbsg,dmunu;
printf("\n\n==== Physical Constraints: =====\n");
printf("deltartho=%.2E\n",deltarho());
printf("gmuon=%.2E\n", gmuon());
printf("bsgnlo=%.2E ", bsgnlo(&SMbsg)); printf("( SM %.2E )\n",SMbsg);
printf("bsmumu=%.2E\n", bsmumu());
printf("btaunu=%.2E\n", btaunu());
printf("dtaunu=%.2E ", dtaunu(&dmunu)); printf("dmunu=%.2E\n", dmunu);
printf("Rl23=%.3E\n", Rl23());
if(masslimits()==0) printf("MassLimits OK\n");
}
#endif
#ifdef HIGGSBOUNDS
if(access(HIGGSBOUNDS "/HiggsBounds",X_OK )) system( "cd " HIGGSBOUNDS "; ./configure; make ");
slhaWrite("HB.in");
HBblocks("HB.in");
system(HIGGSBOUNDS "/HiggsBounds LandH SLHA 3 1 HB.in HB.out > hb.stdout");
slhaRead("HB.out",1+4);
printf("HB result= %.0E obsratio=%.2E\n",slhaValFormat("HiggsBoundsResults",0.,"1 2 %lf"), slhaValFormat("HiggsBoundsResults",0.,"1 3 %lf" ) );
{ char hbInfo[100];
if(0==slhaSTRFormat("HiggsBoundsResults","1 5 ||%[^|]||",hbInfo)) printf("Channel: %s\n",hbInfo);
}
#endif
#ifdef HIGGSSIGNALS
#define DataSet " latestresults "
//#define Method " peak "
//#define Method " mass "
#define Method " both "
#define PDF " 2 " // Gaussian
//#define PDF " 1 " // box
//#define PDF " 3 " // box+Gaussia
#define dMh " 2 "
printf("HiggsSignals:\n");
if(access(HIGGSSIGNALS "/HiggsSignals",X_OK )) system( "cd " HIGGSSIGNALS "; ./configure; make ");
system("rm -f HS.in HS.out");
slhaWrite("HS.in");
HBblocks("HS.in");
system("echo 'BLOCK DMASS\n 25 " dMh " '>> HS.in");
system(HIGGSSIGNALS "/HiggsSignals" DataSet Method PDF " SLHA 3 1 HS.in > hs.stdout");
system("grep -A 10000 HiggsSignalsResults HS.in > HS.out");
slhaRead("HS.out",1+4);
printf(" Number of observables %.0f\n",slhaVal("HiggsSignalsResults",0.,1,7));
printf(" total chi^2= %.1E\n",slhaVal("HiggsSignalsResults",0.,1,12));
printf(" HS p-value = %.1E\n", slhaVal("HiggsSignalsResults",0.,1,13));
#undef dMh
#undef PDF
#undef Method
#undef DataSet
#endif
#ifdef LILITH
if(LiLithF("Lilith_in.xml"))
{ double like;
int exp_ndf;
system("python " LILITH "/run_lilith.py Lilith_in.xml -s -r Lilith_out.slha");
slhaRead("Lilith_out.slha", 1);
like = slhaVal("LilithResults",0.,1,0);
exp_ndf = slhaVal("LilithResults",0.,1,1);
printf("LILITH: -2*log(L): %f; exp ndf: %d \n", like,exp_ndf );
} else printf("LILITH: there is no Higgs candidate\n");
#endif
#ifdef SMODELS
{ int res;
smodels(4000.,5, 0.1, "smodels.in",0);
system("make -C " SMODELS);
system(SMODELS "/runTools.py xseccomputer -p -N -O -f smodels.in");
system(SMODELS "/runSModelS.py -f smodels.in -s smodels.res -particles ./ > smodels.out ");
slhaRead("smodels.res", 1);
res=slhaVal("SModelS_Exclusion",0.,2,0,0);
switch(res)
{ case -1: printf("SMODELS: no channels for testing\n");break;
case 0: printf("SMODELS: not excluded\n");break;
case 1: printf("SMODELS: excluded\n");break;
}
}
#endif
#ifdef OMEGA
{ int fast=1;
double Beps=1.E-5, cut=0.01;
double Omega,Xf;
// to exclude processes with virtual W/Z in DM annihilation
VZdecay=0; VWdecay=0; cleanDecayTable();
// to include processes with virtual W/Z also in co-annihilation
// VZdecay=2; VWdecay=2; cleanDecayTable();
printf("\n==== Calculation of relic density =====\n");
sortOddParticles(cdmName);
Omega=darkOmega(&Xf,fast,Beps);
printf("Xf=%.2e Omega=%.2e\n",Xf,Omega);
// printChannels(Xf,cut,Beps,1,stdout);
// direct access for annihilation channels
/*
if(omegaCh){
int i;
for(i=0; omegaCh[i].weight>0 ;i++)
printf(" %.2E %s %s -> %s %s\n", omegaCh[i].weight, omegaCh[i].prtcl[0],
omegaCh[i].prtcl[1],omegaCh[i].prtcl[2],omegaCh[i].prtcl[3]);
}
*/
// to restore default switches
VZdecay=1; VWdecay=1; cleanDecayTable();
}
#endif
VZdecay=0; VWdecay=0; cleanDecayTable();
#ifdef INDIRECT_DETECTION
{
int err,i;
double Emin=1,SMmev=320;/*Energy cut in GeV and solar potential in MV*/
double sigmaV;
char txt[100];
double SpA[NZ],SpE[NZ],SpP[NZ];
double FluxA[NZ],FluxE[NZ],FluxP[NZ];
double SpNe[NZ],SpNm[NZ],SpNl[NZ];
// double * SpNe=NULL,*SpNm=NULL,*SpNl=NULL;
double Etest=Mcdm/2;
/* default DarkSUSY parameters */
/*
K_dif=0.036;
L_dif=4;
Delta_dif=0.6;
Vc_dif=10;
Rdisk=30;
SMmev=320;
*/
printf("\n==== Indirect detection =======\n");
sigmaV=calcSpectrum(1+2+4,SpA,SpE,SpP,SpNe,SpNm,SpNl ,&err);
/* Returns sigma*v in cm^3/sec. SpX - calculated spectra of annihilation.
Use SpectdNdE(E, SpX) to calculate energy distribution in 1/GeV units.
First parameter 1-includes W/Z polarization
2-includes gammas for 2->2+gamma
4-print cross sections
*/
if(SpA)
{
double fi=0.1,dfi=M_PI/180.; /* angle of sight and 1/2 of cone angle in [rad] */
/* dfi corresponds to solid angle 1.E-3sr */
printf("\nPhoton flux for angle of sight f=%.2f[rad]\n"
"and spherical region described by cone with angle %.4f[rad]\n",fi,2*dfi);
gammaFluxTab(fi,dfi, sigmaV, SpA, FluxA);
printf("Photon flux = %.2E[cm^2 s GeV]^{-1} for E=%.1f[GeV]\n",SpectdNdE(Etest, FluxA), Etest);
#ifdef SHOWPLOTS
sprintf(txt,"Photon flux for angle of sight %.2f[rad] and 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);
}
if(SpE)
{
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("\nPositron flux = %.2E[cm^2 sr s GeV]^{-1} for E=%.1f[GeV] \n",
SpectdNdE(Etest, FluxE), Etest);
}
if(SpP)
{
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("\nAntiproton flux = %.2E[cm^2 sr s GeV]^{-1} for E=%.1f[GeV] \n",
SpectdNdE(Etest, FluxP), Etest);
}
}
#endif
#ifdef LoopGAMMA
{ double vcs_gz,vcs_gg;
double fi=0.,dfi=M_PI/180.; /* fi angle of sight[rad], dfi 1/2 of cone angle in [rad] */
/* dfi corresponds to solid angle pi*(1-cos(dfi)) [sr] */
if(loopGamma(&vcs_gz,&vcs_gg)==0)
{
printf("\nGamma ray lines:\n");
printf("E=%.2E[GeV] vcs(Z,A)= %.2E[cm^3/s], flux=%.2E[cm^2 s]^{-1}\n",Mcdm-91.19*91.19/4/Mcdm,vcs_gz,
gammaFlux(fi,dfi,vcs_gz));
printf("E=%.2E[GeV] vcs(A,A)= %.2E[cm^3/s], flux=%.2E[cm^2 s]^{-1}\n",Mcdm,vcs_gg,
2*gammaFlux(fi,dfi,vcs_gg));
}
}
#endif
#ifdef RESET_FORMFACTORS
{
/*
The user has approach to form factors which specifies quark contents
of proton and nucleon via global parametes like
<Type>FF<Nucleon><q>
where <Type> can be "Scalar", "pVector", and "Sigma";
<Nucleon> "P" or "N" for proton and neutron
<q> "d", "u","s"
calcScalarQuarkFF( Mu/Md, Ms/Md, sigmaPiN[MeV], sigmaS[MeV])
calculates and rewrites Scalar form factors
*/
printf("protonFF (default) d %E, u %E, s %E\n",ScalarFFPd, ScalarFFPu,ScalarFFPs);
printf("neutronFF(default) d %E, u %E, s %E\n",ScalarFFNd, ScalarFFNu,ScalarFFNs);
calcScalarQuarkFF(0.46,27.5,34.,42.);
// To restore default form factors of version 2 call
// calcScalarQuarkFF(0.553,18.9,55.,243.5);
printf("protonFF (new) d %E, u %E, s %E\n",ScalarFFPd, ScalarFFPu,ScalarFFPs);
printf("neutronFF(new) d %E, u %E, s %E\n",ScalarFFNd, ScalarFFNu,ScalarFFNs);
}
#endif
#ifdef CDM_NUCLEON
{ double pA0[2],pA5[2],nA0[2],nA5[2];
double Nmass=0.939; /*nucleon mass*/
double SCcoeff;
printf("\n==== Calculation of CDM-nucleons amplitudes =====\n");
#ifdef TEST_Direct_Detection
printf(" TREE LEVEL\n");
MSSMDDtest(0, pA0,pA5,nA0,nA5);
printf("Analitic formulae\n");
printf(" proton: SI %.3E SD %.3E\n",pA0[0],pA5[0]);
printf(" neutron: SI %.3E SD %.3E\n",nA0[0],nA5[0]);
nucleonAmplitudes(CDM1,NULL, pA0,pA5,nA0,nA5);
printf("CDM-nucleon micrOMEGAs amplitudes:\n");
printf("proton: SI %.3E SD %.3E\n",pA0[0],pA5[0]);
printf("neutron: SI %.3E SD %.3E\n",nA0[0],nA5[0]);
printf(" BOX DIAGRAMS\n");
MSSMDDtest(1, pA0,pA5,nA0,nA5);
printf("Analitic formulae\n");
printf(" proton: SI %.3E SD %.3E\n",pA0[0],pA5[0]);
printf(" neutron: SI %.3E SD %.3E\n",nA0[0],nA5[0]);
#endif
nucleonAmplitudes(CDM1,pA0,pA5,nA0,nA5);
printf("CDM-nucleon micrOMEGAs amplitudes:\n");
printf("proton: SI %.3E SD %.3E\n",pA0[0],pA5[0]);
printf("neutron: SI %.3E SD %.3E\n",nA0[0],nA5[0]);
SCcoeff=4/M_PI*3.8937966E8*pow(Nmass*Mcdm/(Nmass+ Mcdm),2.);
printf("\n==== CDM-nucleon cross sections[pb] ====\n");
printf(" proton SI %.3E SD %.3E\n",SCcoeff*pA0[0]*pA0[0],3*SCcoeff*pA5[0]*pA5[0]);
printf(" neutron SI %.3E SD %.3E\n",SCcoeff*nA0[0]*nA0[0],3*SCcoeff*nA5[0]*nA5[0]);
}
#endif
#ifdef CDM_NUCLEUS
{ double dNdE[300];
double nEvents;
printf("\n======== Direct Detection ========\n");
nEvents=nucleusRecoil(Maxwell,73,Z_Ge,J_Ge73,SxxGe73,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=nucleusRecoil(Maxwell,131,Z_Xe,J_Xe131,SxxXe131,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=nucleusRecoil(Maxwell,23,Z_Na,J_Na23,SxxNa23,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=nucleusRecoil(Maxwell,127,Z_I,J_I127,SxxI127,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
#ifdef NEUTRINO
{ double nu[NZ], nu_bar[NZ],mu[NZ];
int forSun=1;
double Emin=1;
WIMPSIM=0;
printf("\n===============Neutrino Telescope======= for ");
if(forSun) printf("Sun\n"); else printf("Earth\n");
err=neutrinoFlux(Maxwell,forSun, nu,nu_bar);
#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/anti-neutrin fluxes %.2E/%.2E [1/Year/km^2]\n",Emin,
spectrInfo(Emin,nu,NULL), spectrInfo(Emin,nu_bar,NULL));
// ICE CUBE
if(forSun)printf("IceCube22 exclusion confidence level = %.2E%%\n", 100*exLevIC22(nu,nu_bar,NULL));
/* Upward events */
muonUpward(nu,nu_bar, mu);
#ifdef SHOWPLOTS
displaySpectrum("Upward muons[1/Year/km^2/GeV]",Emin,Mcdm/2,mu);
#endif
printf(" E>%.1E GeV Upward muon flux %.2E [1/Year/km^2]\n",Emin,spectrInfo(Emin,mu,NULL));
/* Contained events */
muonContained(nu,nu_bar,1., mu);
#ifdef SHOWPLOTS
displaySpectrum("Contained muons[1/Year/km^3/GeV]",Emin,Mcdm,mu);
#endif
printf(" E>%.1E GeV Contained muon flux %.2E [1/Year/km^3]\n",Emin,spectrInfo(Emin,mu,NULL));
}
#endif
#ifdef DECAYS
{
txtList L;
double width,br;
char * pname;
printf("\n================= Decays ==============\n");
pname = "h";
width=pWidth(pname,&L);
printf("\n%s : total width=%.2E \n and Branchings:\n",pname,width);
printTxtList(L,stdout);
pname = "~o2";
width=pWidth(pname,&L);
printf("\n%s : total width=%.2E \n and Branchings:\n",pname,width);
printTxtList(L,stdout);
}
#endif
#ifdef CROSS_SECTIONS
{
double cs, Pcm=4000, Qren,Qfact=pMass("~o2"),pTmin=0;
int nf=3;
printf("pp collision at %.2E GeV\n",Pcm);
Qren=Qfact;
cs=hCollider(Pcm,1,nf,Qren, Qfact, "~o1","~o2",pTmin,1);
printf("cs(pp->~o1,~o2)=%.2E[pb]\n",cs);
}
#endif
#ifdef CLEAN
killPlots();
system("rm -f suspect2_lha.in suspect2_lha.out suspect2.out Key.dat nngg.out output.flha ");
system("rm -f HB.in HB.out HS.in HS.out hb.stdout hs.stdout debug_channels.txt debug_predratio.txt");
system("rm -f Lilith_in.xml Lilith_out.slha smodels.* summary.* particles.py");
#endif
return 0;
}
int main(int argc,char** argv)
{ int err;
char cdmName[10];
int spin2, charge3,cdim;
ForceUG=0; /* to Force Unitary Gauge assign 1 */
// sysTimeLim=1000;
/*
if you would like to work with superIso
setenv("superIso","./superiso_v3.1",1);
*/
#ifdef SUGRA
{
double m0,mhf,a0,tb;
double gMG1, gMG2, gMG3, gAl, gAt, gAb, sgn, gMHu, gMHd,
gMl2, gMl3, gMr2, gMr3, gMq2, gMq3, gMu2, gMu3, gMd2, gMd3;
printf("\n========= mSUGRA scenario =====\n");
PRINTRGE(RGE);
if(argc<5)
{
printf(" This program needs 4 parameters:\n"
" m0 common scalar mass at GUT scale\n"
" mhf common gaugino mass at GUT scale\n"
" a0 trilinear soft breaking parameter at GUT scale\n"
" tb tan(beta) \n");
printf(" Auxiliary parameters are:\n"
" sgn +/-1, sign of Higgsino mass term (default 1)\n"
" Mtp top quark pole mass\n"
" MbMb Mb(Mb) scale independent b-quark mass\n"
" alfSMZ strong coupling at MZ\n");
/* printf("Example: ./main 70 250 -300 10\n"); */
printf("Example: ./main 120 500 -350 10 1 173.1 \n");
exit(1);
} else
{ double Mtp,MbMb,alfSMZ;
sscanf(argv[1],"%lf",&m0);
sscanf(argv[2],"%lf",&mhf);
sscanf(argv[3],"%lf",&a0);
sscanf(argv[4],"%lf",&tb);
if(argc>5)sscanf(argv[5],"%lf",&sgn); else sgn=1;
if(argc>6){ sscanf(argv[6],"%lf",&Mtp); assignValW("Mtp",Mtp); }
if(argc>7){ sscanf(argv[7],"%lf",&MbMb); assignValW("MbMb",MbMb); }
if(argc>8){ sscanf(argv[8],"%lf",&alfSMZ); assignValW("alfSMZ",alfSMZ);}
}
/*==== simulation of mSUGRA =====*/
gMG1=mhf, gMG2=mhf,gMG3=mhf;
gAl=a0, gAt=a0, gAb=a0; gMHu=m0, gMHd=m0;
gMl2=m0, gMl3=m0, gMr2=m0, gMr3=m0;
gMq2=m0, gMq3=m0, gMu2=m0, gMd2=m0, gMu3=m0, gMd3=m0;
err= SUGRAMODEL(RGE) (tb,
gMG1, gMG2, gMG3, gAl, gAt, gAb, sgn, gMHu, gMHd,
gMl2, gMl3, gMr2, gMr3, gMq2, gMq3, gMu2, gMu3, gMd2, gMd3);
}
#elif defined(SUGRANUH)
{
double m0,mhf,a0,tb;
double gMG1, gMG2, gMG3, gAl, gAt, gAb, gMl2, gMl3, gMr2, gMr3, gMq2, gMq3, gMu2, gMu3, gMd2, gMd3,mu,MA;
printf("\n========= mSUGRA non-universal Higgs scenario =====\n");
PRINTRGE(RGE);
if(argc<7)
{
printf(" This program needs 6 parameters:\n"
" m0 common scalar mass at GUT scale\n"
" mhf common gaugino mass at GUT scale\n"
" a0 trilinear soft breaking parameter at GUT scale\n"
" tb tan(beta) \n"
" mu mu(EWSB)\n"
" MA mass of pseudoscalar Higgs\n");
printf(" Auxiliary parameters are:\n"
" Mtp top quark pole mass\n"
" MbMb Mb(Mb) scale independent b-quark mass\n"
" alfSMZ strong coupling at MZ\n");
/* printf("Example: ./main 70 250 -300 10\n"); */
printf("Example: ./main 120 500 -350 10 680 760 \n");
exit(1);
} else
{ double Mtp,MbMb,alfSMZ;
sscanf(argv[1],"%lf",&m0);
sscanf(argv[2],"%lf",&mhf);
sscanf(argv[3],"%lf",&a0);
sscanf(argv[4],"%lf",&tb);
sscanf(argv[5],"%lf",&mu);
sscanf(argv[6],"%lf",&MA);
if(argc>7){ sscanf(argv[7],"%lf",&Mtp); assignValW("Mtp",Mtp); }
if(argc>8){ sscanf(argv[8],"%lf",&MbMb); assignValW("MbMb",MbMb); }
if(argc>9){ sscanf(argv[9],"%lf",&alfSMZ); assignValW("alfSMZ",alfSMZ);}
}
/*==== simulation of mSUGRA =====*/
gMG1=mhf, gMG2=mhf,gMG3=mhf;
gAl=a0, gAt=a0, gAb=a0;
gMl2=m0, gMl3=m0, gMr2=m0, gMr3=m0;
gMq2=m0, gMq3=m0, gMu2=m0, gMd2=m0, gMu3=m0, gMd3=m0;
err= SUGRANUHMODEL(RGE) (tb,gMG1,gMG2,gMG3,gAl,gAt,gAb,gMl2,gMl3,gMr2,gMr3,gMq2,gMq3,gMu2,gMu3,gMd2,gMd3,mu,MA);
}
#elif defined(AMSB)
{
double m0,m32,sgn,tb;
printf("\n========= AMSB scenario =====\n");
PRINTRGE(RGE);
if(argc<4)
{
printf(" This program needs 3 parameters:\n"
" m0 common scalar mass at GUT scale\n"
" m3/2 gravitino mass\n"
" tb tan(beta) \n");
printf(" Auxiliary parameters are:\n"
" sgn +/-1, sign of Higgsino mass term (default 1)\n"
" Mtp top quark pole mass\n"
" MbMb Mb(Mb) scale independent b-quark mass\n"
" alfSMZ strong coupling at MZ\n");
printf("Example: ./main 450 60000 10\n");
exit(1);
} else
{ double Mtp,MbMb,alfSMZ;
sscanf(argv[1],"%lf",&m0);
sscanf(argv[2],"%lf",&m32);
sscanf(argv[3],"%lf",&tb);
if(argc>4)sscanf(argv[4],"%lf",&sgn); else sgn=1;
if(argc>5){ sscanf(argv[5],"%lf",&Mtp); assignValW("Mtp",Mtp); }
if(argc>6){ sscanf(argv[6],"%lf",&MbMb); assignValW("MbMb",MbMb); }
if(argc>7){ sscanf(argv[7],"%lf",&alfSMZ); assignValW("alfSMZ",alfSMZ);}
}
err= AMSBMODEL(RGE)(m0,m32,tb,sgn);
}
#elif defined(EWSB)
{
printf("\n========= EWSB scale input =========\n");
PRINTRGE(RGE);
if(argc <2)
{ printf("The program needs one argument:the name of file with MSSM parameters.\n"
"Example: ./main mssm1.par \n");
exit(1);
}
printf("Initial file \"%s\"\n",argv[1]);
err=readVarMSSM(argv[1]);
if(err==-1) { printf("Can not open the file\n"); exit(2);}
else if(err>0) { printf("Wrong file contents at line %d\n",err);exit(3);}
err=EWSBMODEL(RGE)();
}
#else
{
printf("\n========= SLHA file input =========\n");
if(argc <2)
{ printf("The program needs one argument:the name of SLHA input file.\n"
"Example: ./main suspect2_lha.out \n");
exit(1);
}
printf("Initial file \"%s\"\n",argv[1]);
err=lesHinput(argv[1]);
if(err) exit(2);
}
#endif
if(err==-1) { printf("Can not open the file\n"); exit(2);}
else if(err>0) { printf("Wrong file contents at line %d\n",err);exit(3);}
{ int nw;
printf("Warnings from spectrum calculator:\n");
nw=slhaWarnings(stdout);
if(nw==0) printf(" .....none\n");
}
if(err) exit(1);
err=sortOddParticles(cdmName);
if(err) { printf("Can't calculate %s\n",cdmName); return 1;}
qNumbers(cdmName,&spin2, &charge3, &cdim);
printf("\nDark matter candidate is '%s' with spin=%d/2 mass=%.2E\n",
cdmName, spin2, Mcdm);
if(charge3) { printf("Dark Matter has electric charge %d/3\n",charge3); exit(1);}
if(cdim!=1) { printf("Dark Matter is a color particle\n"); exit(1);}
if(strcmp(cdmName,"~o1")) printf(" ~o1 is not CDM\n");
else o1Contents(stdout);
#ifdef MASSES_INFO
{
printf("\n=== MASSES OF HIGGS AND SUSY PARTICLES: ===\n");
printHiggs(stdout);
printMasses(stdout,1);
}
#endif
#ifdef CONSTRAINTS
{ double SMbsg,dmunu;
printf("\n\n==== Physical Constraints: =====\n");
printf("deltartho=%.2E\n",deltarho());
printf("gmuon=%.2E\n", gmuon());
printf("bsgnlo=%.2E ", bsgnlo(&SMbsg)); printf("( SM %.2E )\n",SMbsg);
printf("bsmumu=%.2E\n", bsmumu());
printf("btaunu=%.2E\n", btaunu());
printf("dtaunu=%.2E ", dtaunu(&dmunu)); printf("dmunu=%.2E\n", dmunu);
printf("Rl23=%.3E\n", Rl23());
if(masslimits()==0) printf("MassLimits OK\n");
}
#endif
#ifdef SUPERISO
slhaWrite("slha.in");
system( SUPERISO "/slha.x slha.in >/dev/null");
slhaRead("output.flha",1);
unlink("slha.in");
printf("superIsoBSG=%.3E\n", slhaValFormat("FOBS",0., " 5 1 %lf 0 2 3 22"));
#endif
#ifdef HIGGSBOUNDS
if(access(HIGGSBOUNDS "/HiggsBounds",X_OK )) system( "cd " HIGGSBOUNDS "; ./configure; make ");
slhaWrite("slha.in");
system("cp slha.in HB.slha");
HBblocks("HB.slha");
System("%s/HiggsBounds LandH SLHA 3 1 HB.slha",HIGGSBOUNDS);
slhaRead("HB.slha",1+4);
printf("HB result= %.0E obsratio=%.2E\n",slhaValFormat("HiggsBoundsResults",0.,"1 2 %lf"), slhaValFormat("HiggsBoundsResults",0.,"1 3 %lf" ) );
{ char hbInfo[100];
if(0==slhaSTRFormat("HiggsBoundsResults","1 5 ||%[^|]||",hbInfo)) printf("Channel: %s\n",hbInfo);
}
slhaRead("slha.in",0);
unlink("slha.in");
#endif
#ifdef OMEGA
{ int fast=1;
double Beps=1.E-5, cut=0.01;
double Omega,Xf;
// to exclude processes with virtual W/Z in DM annihilation
VZdecay=0; VWdecay=0; cleanDecayTable();
// to include processes with virtual W/Z also in co-annihilation
// VZdecay=2; VWdecay=2; cleanDecayTable();
printf("\n==== Calculation of relic density =====\n");
sortOddParticles(cdmName);
Omega=darkOmega(&Xf,fast,Beps);
printf("Xf=%.2e Omega=%.2e\n",Xf,Omega);
printChannels(Xf,cut,Beps,1,stdout);
// direct access for annihilation channels
/*
if(omegaCh){
int i;
for(i=0; omegaCh[i].weight>0 ;i++)
printf(" %.2E %s %s -> %s %s\n", omegaCh[i].weight, omegaCh[i].prtcl[0],
omegaCh[i].prtcl[1],omegaCh[i].prtcl[2],omegaCh[i].prtcl[3]);
}
*/
// to restore VZdecay and VWdecay switches
VZdecay=1; VWdecay=1; cleanDecayTable();
}
#endif
#ifdef INDIRECT_DETECTION
{
int err,i;
double Emin=1,SMmev=320;/*Energy cut in GeV and solar potential in MV*/
double sigmaV;
double vcs_gz,vcs_gg;
char txt[100];
double SpA[NZ],SpE[NZ],SpP[NZ];
double FluxA[NZ],FluxE[NZ],FluxP[NZ];
double SpNe[NZ],SpNm[NZ],SpNl[NZ];
// double * SpNe=NULL,*SpNm=NULL,*SpNl=NULL;
double Etest=Mcdm/2;
/* default DarkSUSY parameters */
/*
K_dif=0.036;
L_dif=4;
Delta_dif=0.6;
Vc_dif=10;
Rdisk=30;
SMmev=320;
*/
printf("\n==== Indirect detection =======\n");
sigmaV=calcSpectrum( 2+4,SpA,SpE,SpP,SpNe,SpNm,SpNl ,&err);
/* Returns sigma*v in cm^3/sec. SpX - calculated spectra of annihilation.
Use SpectdNdE(E, SpX) to calculate energy distribution in 1/GeV units.
First parameter 1-includes W/Z polarization
2-includes gammas for 2->2+gamma
4-print cross sections
*/
if(SpA)
{
double fi=0.,dfi=M_PI/180.; /* angle of sight and 1/2 of cone angle in [rad] */
/* dfi corresponds to solid angle 1.E-3sr */
printf("Photon flux for angle of sight f=%.2f[rad]\n"
"and spherical region described by cone with angle %.4f[rad]\n",fi,2*dfi);
gammaFluxTab(fi,dfi, sigmaV, SpA, FluxA);
#ifdef SHOWPLOTS
sprintf(txt,"Photon flux for angle of sight %.2f[rad] and cone angle %.2f[rad]",fi,2*dfi);
displaySpectrum(FluxA,txt,Emin,Mcdm,1);
#endif
printf("Photon flux = %.2E[cm^2 s GeV]^{-1} for E=%.1f[GeV]\n",SpectdNdE(Etest, FluxA), Etest);
#ifdef LoopGAMMA
if(loopGamma(&vcs_gz,&vcs_gg)==0)
{
printf("Gamma ray lines:\n");
printf("E=%.2E[GeV] vcs(Z,A)= %.2E[cm^3/s], flux=%.2E[cm^2 s]^{-1}\n",Mcdm-91.19*91.19/4/Mcdm,vcs_gz,
gammaFlux(fi,dfi,vcs_gz));
printf("E=%.2E[GeV] vcs(A,A)= %.2E[cm^3/s], flux=%.2E[cm^2 s]^{-1}\n",Mcdm,vcs_gg,
2*gammaFlux(fi,dfi,vcs_gg));
}
#endif
}
if(SpE)
{
posiFluxTab(Emin, sigmaV, SpE, FluxE);
if(SMmev>0) solarModulation(SMmev,0.0005,FluxE,FluxE);
#ifdef SHOWPLOTS
displaySpectrum(FluxE,"positron flux [cm^2 s sr GeV]^{-1}" ,Emin,Mcdm,1);
#endif
printf("Positron flux = %.2E[cm^2 sr s GeV]^{-1} for E=%.1f[GeV] \n",
SpectdNdE(Etest, FluxE), Etest);
}
if(SpP)
{
pbarFluxTab(Emin, sigmaV, SpP, FluxP);
if(SMmev>0) solarModulation(SMmev,1,FluxP,FluxP);
#ifdef SHOWPLOTS
displaySpectrum(FluxP,"antiproton flux [cm^2 s sr GeV]^{-1}" ,Emin,Mcdm,1);
#endif
printf("Antiproton flux = %.2E[cm^2 sr s GeV]^{-1} for E=%.1f[GeV] \n",
SpectdNdE(Etest, FluxP), Etest);
}
}
#endif
#ifdef RESET_FORMFACTORS
{
/*
The user has approach to form factors which specifies quark contents
of proton and nucleon via global parametes like
<Type>FF<Nucleon><q>
where <Type> can be "Scalar", "pVector", and "Sigma";
<Nucleon> "P" or "N" for proton and neutron
<q> "d", "u","s"
calcScalarQuarkFF( Mu/Md, Ms/Md, sigmaPiN[MeV], sigmaS[MeV])
calculates and rewrites Scalar form factors
*/
printf("protonFF (default) d %E, u %E, s %E\n",ScalarFFPd, ScalarFFPu,ScalarFFPs);
printf("neutronFF(default) d %E, u %E, s %E\n",ScalarFFNd, ScalarFFNu,ScalarFFNs);
calcScalarQuarkFF(0.46,27.5,34.,42.);
// To restore default form factors of version 2 call
// calcScalarQuarkFF(0.553,18.9,55.,243.5);
printf("protonFF (new) d %E, u %E, s %E\n",ScalarFFPd, ScalarFFPu,ScalarFFPs);
printf("neutronFF(new) d %E, u %E, s %E\n",ScalarFFNd, ScalarFFNu,ScalarFFNs);
}
#endif
#ifdef CDM_NUCLEON
{ double pA0[2],pA5[2],nA0[2],nA5[2];
double Nmass=0.939; /*nucleon mass*/
double SCcoeff;
printf("\n==== Calculation of CDM-nucleons amplitudes =====\n");
#ifdef TEST_Direct_Detection
printf(" TREE LEVEL\n");
MSSMDDtest(0, pA0,pA5,nA0,nA5);
printf("Analitic formulae\n");
printf("proton: SI %.3E SD %.3E\n",pA0[0],pA5[0]);
printf("neutron: SI %.3E SD %.3E\n",nA0[0],nA5[0]);
nucleonAmplitudes(NULL, pA0,pA5,nA0,nA5);
printf("CDM-nucleon micrOMEGAs amplitudes:\n");
printf("proton: SI %.3E SD %.3E\n",pA0[0],pA5[0]);
printf("neutron: SI %.3E SD %.3E\n",nA0[0],nA5[0]);
printf(" BOX DIAGRAMS\n");
MSSMDDtest(1, pA0,pA5,nA0,nA5);
printf("Analitic formulae\n");
printf("proton: SI %.3E SD %.3E\n",pA0[0],pA5[0]);
printf("neutron: SI %.3E SD %.3E\n",nA0[0],nA5[0]);
#endif
nucleonAmplitudes(FeScLoop, pA0,pA5,nA0,nA5);
printf("CDM-nucleon micrOMEGAs amplitudes:\n");
printf("proton: SI %.3E SD %.3E\n",pA0[0],pA5[0]);
printf("neutron: SI %.3E SD %.3E\n",nA0[0],nA5[0]);
SCcoeff=4/M_PI*3.8937966E8*pow(Nmass*Mcdm/(Nmass+ Mcdm),2.);
printf("CDM-nucleon cross sections[pb]:\n");
printf(" proton SI %.3E SD %.3E\n",SCcoeff*pA0[0]*pA0[0],3*SCcoeff*pA5[0]*pA5[0]);
printf(" neutron SI %.3E SD %.3E\n",SCcoeff*nA0[0]*nA0[0],3*SCcoeff*nA5[0]*nA5[0]);
}
#endif
#ifdef CDM_NUCLEUS
{ double dNdE[300];
double nEvents;
printf("\n======== Direct Detection ========\n");
nEvents=nucleusRecoil(Maxwell,73,Z_Ge,J_Ge73,SxxGe73,FeScLoop,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=nucleusRecoil(Maxwell,131,Z_Xe,J_Xe131,SxxXe131,FeScLoop,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=nucleusRecoil(Maxwell,23,Z_Na,J_Na23,SxxNa23,FeScLoop,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=nucleusRecoil(Maxwell,127,Z_I,J_I127,SxxI127,FeScLoop,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
#ifdef NEUTRINO
{ double nu[NZ], nu_bar[NZ],mu[NZ];
double Ntot;
int forSun=1;
double Emin=0.01;
printf("\n===============Neutrino Telescope======= for ");
if(forSun) printf("Sun\n"); else printf("Earth\n");
err=neutrinoFlux(Maxwell,forSun, nu,nu_bar);
#ifdef SHOWPLOTS
displaySpectrum(nu,"nu flux from Sun [1/Year/km^2/GeV]",Emin,Mcdm,1);
displaySpectrum(nu_bar,"nu-bar from Sun [1/Year/km^2/GeV]",Emin,Mcdm,1);
#endif
{ double Ntot;
double Emin=1; //GeV
spectrInfo(Emin/Mcdm,nu, &Ntot,NULL);
printf(" E>%.1E GeV neutrino flux %.2E [1/Year/km^2] \n",Emin,Ntot);
spectrInfo(Emin/Mcdm,nu_bar, &Ntot,NULL);
printf(" E>%.1E GeV anti-neutrino flux %.2E [1/Year/km^2]\n",Emin,Ntot);
}
/* Upward events */
muonUpward(nu,nu_bar, mu);
#ifdef SHOWPLOTS
displaySpectrum(mu,"Upward muons[1/Year/km^2/GeV]",1,Mcdm/2,1);
#endif
{ double Ntot;
double Emin=1; //GeV
spectrInfo(Emin/Mcdm,mu, &Ntot,NULL);
printf(" E>%.1E GeV Upward muon flux %.2E [1/Year/km^2]\n",Emin,Ntot);
}
/* Contained events */
muonContained(nu,nu_bar,1., mu);
#ifdef SHOWPLOTS
displaySpectrum(mu,"Contained muons[1/Year/km^3/GeV]",Emin,Mcdm,1);
#endif
{ double Ntot;
double Emin=1; //GeV
spectrInfo(Emin/Mcdm,mu, &Ntot,NULL);
printf(" E>%.1E GeV Contained muon flux %.2E [1/Year/km^3]\n",Emin,Ntot);
}
}
#endif
#ifdef DECAYS
{
txtList L;
double width,br;
char * pname;
printf("\n================= Decays ==============\n");
pname = "h";
width=pWidth(pname,&L);
printf("\n%s : total width=%.2E \n and Branchings:\n",pname,width);
printTxtList(L,stdout);
pname = "~o2";
width=pWidth(pname,&L);
printf("\n%s : total width=%.2E \n and Branchings:\n",pname,width);
printTxtList(L,stdout);
}
#endif
#ifdef CROSS_SECTIONS
{
double Pcm=250, cosmin=-0.99, cosmax=0.99, cs;
numout* cc;
printf("\n====== Calculation of cross section ====\n");
printf(" e^+, e^- annihilation\n");
Pcm=250.;
Helicity[0]=0.5; /* helicity : spin projection on direction of motion */
Helicity[1]=-0.5; /* helicities ={ 0.5, -0.5} corresponds to vector state */
printf("Process e,E->2*x at Pcm=%.3E GeV\n",Pcm);
cc=newProcess("e%,E%->2*x");
if(cc)
{ int ntot,l;
char * name[4];
procInfo1(cc,&ntot,NULL,NULL);
for(l=1;l<=ntot; l++)
{ int err;
double cs;
char txt[100];
procInfo2(cc,l,name,NULL);
sprintf(txt,"%3s,%3s -> %3s %3s ",name[0],name[1],name[2],name[3]);
cs= cs22(cc,l,Pcm,cosmin,cosmax,&err);
if(err) printf("%-20.20s Error\n",txt);
else if(cs) printf("%-20.20s %.2E [pb]\n",txt,cs);
}
}
/*
{ double stot=0;
int i,j;
char * sq[25]=
{"~dL","~dR","~uL","~uR","~sL","~sR","~cL","~cR","~b1","~b2","~t1","~t2",
"~DL","~DR","~UL","~UR","~SL","~SR","~CL","~CR","~B1","~B2","~T1","~T2",
"~g"};
Pcm=4000;
for(i=0;i<25;i++) for(j=0;j<25;j++)
{double dcs=hCollider(Pcm,1,0,sq[i],sq[j]);
stot+=dcs;
printf("p,p -> %s %s %E\n", sq[i],sq[j],dcs);
}
printf("total cross section =%E (without K-factor)\n",stot);
}
*/
}
#endif
#ifdef CLEAN
killPlots();
system("rm -f suspect2_lha.in suspect2_lha.out suspect2.out HB.slha Key.dat nngg.in nngg.out output.flha ");
#endif
return 0;
}