int leshinput_(char *fname, int len)
{
char * cname=malloc(len+2);
int err;
fName2c(fname,cname,len);
err=lesHinput(cname);
free(cname);
return err;
}
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 */
// Check number of arguments
if(argc <2)
{ printf("The program needs one argument:the name of SLHA input file.\n"
"Example: ./main suspect2_lha.out \n");
exit(1);
}
// Read in slha
err=lesHinput(argv[1]);
if(err) exit(2);
// Check for slha warnings
slhaWarnings(stdout);
if(err) exit(1);
// Sort Particles
err=sortOddParticles(cdmName);
if(err) { printf("Can't calculate %s\n",cdmName); return 1;}
qNumbers(cdmName,&spin2, &charge3, &cdim);
// This shouldn't happen
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");
// Calculation of Omega, i.e. dark matter density
int fast=1;
double Beps=1.E-5;
double Omega,Xf;
Omega=darkOmega(&Xf,fast,Beps);
// print value
printf("[\"MastercodeTag\", \"Omega\", %f ]\n",Omega);
// Calculation of sigma_p_si
double pA0[2],pA5[2],nA0[2],nA5[2];
double Nmass=0.939; /*nucleon mass*/
double SCcoeff;
nucleonAmplitudes(FeScLoop, pA0,pA5,nA0,nA5);
SCcoeff=4/M_PI*3.8937966E8*pow(Nmass*Mcdm/(Nmass+ Mcdm),2.);
double proton_sigma_si=SCcoeff*pA0[0]*pA0[0];
// print value
printf("[\"MastercodeTag\", \"sigma_p_si\", %e ] \n",proton_sigma_si);
// if all went fine, then return 0
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;
}
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;
}
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
#ifdef OBTAIN_LSP
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);
#endif
#ifdef OBTAIN_CROSS_SECTION
{
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
*/
printf("sigmav=%.2E[cm^3/s]\n",sigmaV);
//sigma_v = Sigma_v(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);
#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 CALCULATION_OF_MU
{
#ifdef TAKE_VALUES_FROM_LSP_OF_MICROMEGAS
{
mdm = mdm_calc(Mcdm);
}
#endif
double z = pow(10,5);
printf("***************** Values used for energy calculation ********************\n");
printf("H0 - %.2e \n", H0);
printf("zeq - %.2e \n", zeq);
printf("Omega_m - %.2e \n", Omega_m);
printf("Omega_r - %.2e \n", Omega_r);
printf("Omega_Lambda - %.2e \n", Omega_Lambda);
printf("Rho_cr - %.2e \n", Rho_cr);
printf("mdm - %.2e \n", mdm);
printf("The H_z - is %.2e \n",H(z));
printf("The ndm_z is %.2e \n",ndm_z(z));
printf("The sigma_v is %.2e \n",sigma_v);
printf("The tau is %.2e \n",tau(z));
printf("*************************************************************************\n");
double value = dQdz(z) * ( exp(-tau(z))/ H(z));
printf("For redshift %.2e ", z);
printf("the energy injection is %.2e \n",value);
double value_paper = dummy_energy_injection(z)* ( exp (-tau(z))/ H(z));
printf("While the calculation as in the paper is %.2e \n", value_paper);
double z_min = 5 * pow(10,4);
double z_i = 6 * pow(10,6);
int subdivisions = 1000;
value = mu_0(z_i, z_min, subdivisions);
printf("Mu at our time is %.2e \n", value);
}
#endif
return 0;
}