int main(int argc,char** argv)
{ int err,nw;
char cdmName[10];
int spin2, charge3,cdim;
double laMax;
delFiles=0; /* switch to save/delete NMSSMTools input/output */
ForceUG=0; /* to Force Unitary Gauge assign 1 */
#ifdef SUGRA
{
double m0,mhf,a0,tb;
double Lambda, aLambda,aKappa,sgn;
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"
" Lambda Lambda parameter at SUSY\n"
" aKappa aKappa parameter at GUT\n"
);
printf(" Auxiliary parameters are:\n"
" sgn +/-1, sign of Higgsino mass term (default 1)\n"
" aLambda at GUT (default aLambda=a0)\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 320 600 -1300 2 0.5 -1400\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",&Lambda);
sscanf(argv[6],"%lf",&aKappa);
if(argc>7) sscanf(argv[7],"%lf",&sgn); else sgn=1;
if(argc>8) sscanf(argv[8],"%lf",&aLambda); else aLambda=a0;
if(argc>9){ sscanf(argv[9],"%lf",&Mtp); assignValW("Mtp",Mtp); }
if(argc>10){ sscanf(argv[10],"%lf",&MbMb); assignValW("MbMb",MbMb); }
if(argc>11){ sscanf(argv[11],"%lf",&alfSMZ); assignValW("alfSMZ",alfSMZ);}
}
err=nmssmSUGRA( m0,mhf, a0,tb, sgn, Lambda, aLambda, aKappa);
}
#elif defined(EWSB)
{
if(argc!=2)
{
printf(" Correct usage: ./main <file with NMSSM parameters> \n");
printf(" Example : ./main data1.par \n");
exit(1);
}
err=readVarNMSSM(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=nmssmEWSB();
}
#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 spectr.dat \n");
exit(1);
}
printf("Initial file \"%s\"\n",argv[1]);
err=readSLHA(argv[1]);
if(err) exit(2);
}
#endif
slhaWarnings(stdout);
if(err) exit(1);
//assignValW("Ms2GeV",0.14);
err=sortOddParticles(cdmName);
if(err) { printf("Can't calculate %s\n",cdmName); return 1;}
laMax=findValW("laMax");
printf("Largest coupling of Higgs self interaction %.1E\n",laMax);
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 is a color particle\n"); exit(1);}
if(strcmp(cdmName,"~o1")) printf(" ~o1 is not CDM\n");
else o1Contents(stdout);
/* printVar(stdout); */
#ifdef MASSES_INFO
{
printf("\n=== MASSES OF HIGGS AND SUSY PARTICLES: ===\n");
printHiggs(stdout);
printMasses(stdout,1);
}
#endif
#ifdef CONSTRAINTS
{ double constr0,constrM, constrP;
printf("\n\n==== Physical Constraints: =====\n");
constr0=bsgnlo(&constrM,&constrP);
printf("B->s,gamma = %.2E (%.2E , %.2E ) \n",constr0,constrM, constrP );
constr0= bsmumu(&constrM,&constrP);
printf("Bs->mu,mu = %.2E (%.2E , %.2E ) \n",constr0,constrM, constrP );
constr0=btaunu(&constrM,&constrP);
printf("B+->tau+,nu= %.2E (%.2E , %.2E ) \n",constr0, constrM, constrP );
constr0=deltaMd(&constrM,&constrP);
printf("deltaMd = %.2E (%.2E , %.2E ) \n",constr0,constrM, constrP );
constr0=deltaMs(&constrM,&constrP);
printf("deltaMs = %.2E (%.2E , %.2E ) \n",constr0,constrM, constrP );
constr0=gmuon(&constrM,&constrP);
printf("(g-2)/BSM = %.2E (%.2E , %.2E ) \n",constr0,constrM, constrP );
}
#endif
#ifdef OMEGA
{ int fast=1;
double Beps=1.E-5, 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
{
int err,i;
double Emin=0.1,/* 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 SpNe[NZ],SpNm[NZ],SpNl[NZ];
double Etest=Mcdm/2;
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
*/
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,1);
#endif
printf("Photon flux = %.2E[cm^2 s GeV]^{-1} for E=%.1f[GeV]\n",SpectdNdE(Etest, SpA), Etest);
}
if(SpE)
{
posiFluxTab(Emin, sigmaV, SpE, 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 );
#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"
calcScalarFF( Mu/Md, Ms/Md, sigmaPiN[MeV], sigma0[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);
calcScalarFF(0.553,18.9,70.,35.);
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);
/* Option to change parameters of DM velocity distribution */
SetfMaxwell(220.,600.);
/*
dN ~ exp(-v^2/arg1^2)*Theta(v-arg2) d^3v
Earth velocity with respect to Galaxy defined by 'Vearth' parameter.
All parameters are in [km/s] units.
*/
}
#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(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,S00Ge73,S01Ge73,S11Ge73,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,S00Xe131,S01Xe131,S11Xe131,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,S00Na23,S01Na23,S11Na23,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,S00I127,S01I127,S11I127,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 DECAYS
{
txtList L;
int dim;
double width,br;
char * pname;
printf("\nParticle decays\n");
pname = "h1";
width=pWidth(pname,&L,&dim);
printf("%s->%d*x : total width=%E \n and Branchings:\n",pname,dim,width);
printTxtList(L,stdout);
pname = "l";
width=pWidth(pname,&L,&dim);
printf("%s->%d*x : total width=%E \n and Branchings:\n",pname,dim,width);
printTxtList(L,stdout);
printf("Br(e,Ne,nl)= %E\n",findBr(L,"e,Ne,nl"));
pname = "~o2";
width=pWidth(pname,&L,&dim);
printf("%s->%d*x : total width=%E \n and Branchings:\n",pname,dim,width);
printTxtList(L,stdout);
}
#endif
#ifdef CROSS_SECTIONS
{
double Pcm=500, cosmin=-0.99, cosmax=0.99, cs;
numout* cc;
printf("\n====== Calculation of cross section ====\n");
printf(" e^+, e^- annihilation\n");
Pcm=500.;
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","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;
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);
}
}
}
#endif
killPlots();
return 0;
}
int main(int argc,char** argv)
{ int err;
char cdmName[10];
int spin2, charge3,cdim;
delFiles=0; /* switch to save/delete RGE input/output */
ForceUG=0; /* to Force Unitary Gauge assign 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(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
{ 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
{ printf("\n\n==== Physical Constraints: =====\n");
printf("deltartho=%.2E\n",deltarho());
printf("gmuon=%.2E\n", gmuon());
printf("bsgnlo=%.2E\n", bsgnlo());
printf("bsmumu=%.2E\n", bsmumu());
printf("btaunu=%.2E\n", btaunu());
if(masslimits()==0) printf("MassLimits OK\n");
}
#endif
#ifdef OMEGA
{ int fast=1;
double Beps=1.E-5, 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
{
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( 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
*/
printf("sigmav=%.2E[cm^3/s]\n",sigmaV);
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);
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));
}
}
if(SpE)
{
posiFluxTab(Emin, sigmaV, SpE, FluxE);
if(SMmev>0) solarModulation(SMmev,0.0005,FluxE,FluxE);
#ifdef SHOWPLOTS
displaySpectrum(SpE,"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"
calcScalarFF( Mu/Md, Ms/Md, sigmaPiN[MeV], sigma0[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);
calcScalarFF(0.553,18.9,70.,35.);
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);
/* Option to change parameters of DM velocity distribution */
SetfMaxwell(220.,600.);
/*
dN ~ exp(-v^2/arg1^2)*Theta(v-arg2) d^3v
Earth velocity with respect to Galaxy defined by 'Vearth' parameter.
All parameters are in [km/s] units.
*/
}
#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,S00Ge73,S01Ge73,S11Ge73,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,S00Xe131,S01Xe131,S11Xe131,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,S00Na23,S01Na23,S11Na23,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,S00I127,S01I127,S11I127,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 DECAYS
{
txtList L;
int dim;
double width,br;
char * pname;
pname = "h";
width=pWidth(pname,&L,&dim);
printf("%s->%d*x : total width=%E \n and Branchings:\n",pname,dim,width);
printTxtList(L,stdout);
pname = "l";
width=pWidth(pname,&L,&dim);
printf("%s->%d*x : total width=%E \n and Branchings:\n",pname,dim,width);
printTxtList(L,stdout);
printf("Br(e,Ne,nl)= %E\n",findBr(L,"e,Ne,nl"));
pname = "~o2";
width=pWidth(pname,&L,&dim);
printf("%s->%d*x : total width=%E \n and Branchings:\n",pname,dim,width);
printTxtList(L,stdout);
pname = "~g";
width=pWidth(pname,&L,&dim);
printf("%s->%d*x : total width=%E \n and Branchings:\n",pname,dim,width);
printTxtList(L,stdout);
}
#endif
#ifdef CROSS_SECTIONS
{
double Pcm=500, cosmin=-0.99, cosmax=0.99, cs;
numout* cc;
printf("\n====== Calculation of cross section ====\n");
printf(" e^+, e^- annihilation\n");
Pcm=500.;
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","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;
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);
}
}
}
#endif
killPlots();
return 0;
}
void setfmaxwell_(double *DV,double *vmax)
{ SetfMaxwell(*DV,*vmax);}
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 */
if(argc==1)
{
printf(" Correct usage: ./main <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(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 is a color particle\n"); exit(1);}
if(strcmp(cdmName,"~n4")) printf(" ~n4 is not CDM\n");
#ifdef MASSES_INFO
{
printf("\n=== MASSES OF PARTICLES OF ODD SECTOR: ===\n");
printMasses(stdout,1);
}
#endif
#ifdef CONSTRAINTS
#endif
#ifdef OMEGA
{ int fast=1;
double Beps=1.E-5, 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
{
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
*/
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,1);
#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,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 );
#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"
calcScalarFF( Mu/Md, Ms/Md, sigmaPiN[MeV], sigma0[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);
calcScalarFF(0.553,18.9,70.,35.);
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);
/* Option to change parameters of DM velocity distribution */
SetfMaxwell(220.,600.);
/*
dN ~ exp(-v^2/arg1^2)*Theta(v-arg2) d^3v
Earth velocity with respect to Galaxy defined by 'Vearth' parameter.
All parameters are in [km/s] units.
*/
}
#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(FeScLoop, 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,S00Ge73,S01Ge73,S11Ge73,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,S00Xe131,S01Xe131,S11Xe131,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,S00Na23,S01Na23,S11Na23,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,S00I127,S01I127,S11I127,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 DECAYS
{
txtList L;
int dim;
double width,br;
char * pname;
printf("\n Calculation of particle decays\n");
pname = "H";
width=pWidth(pname,&L,&dim);
printf("%s->%d*x : total width=%E \n and Branchings:\n",pname,dim,width);
printTxtList(L,stdout);
pname = "l";
width=pWidth(pname,&L,&dim);
printf("%s->%d*x : total width=%E \n and Branchings:\n",pname,dim,width);
printTxtList(L,stdout);
printf("Br(e,Ne,nl)= %E\n",findBr(L,"e,Ne,nl"));
pname = "Zp";
width=pWidth(pname,&L,&dim);
printf("%s->%d*x : total width=%E \n and Branchings:\n",pname,dim,width);
printTxtList(L,stdout);
}
#endif
#ifdef CROSS_SECTIONS
{
double Pcm=500, cosmin=-0.99, cosmax=0.99, cs;
numout* cc;
printf("\n====== Calculation of cross section ====\n");
printf(" e^+, e^- annihilation\n");
Pcm=500.;
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","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;
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);
}
}
}
#endif
killPlots();
return 0;
}
