int nmssmSUGRA(double m0,double mhf, double a0,double tb, double sgn,
double Lambda, double aLambda, double aKappa)
{ int err;
int del=getdelfilesstat_();
err=sugraLesH("inpsp.dat", m0,mhf,a0,tb, sgn,Lambda, aLambda, aKappa);
if(err) return -1;
err=runTools("nmspec","spectrsp.dat");
assignValW("Au",findValW("At"));
assignValW("Ad",findValW("Ab"));
if(del) system("rm -f inpsp.dat spectrsp.dat omegasp.dat decaysp.dat outsp.dat");
return err;
}
static void CharginoZM(void)
{
double M2=NMassM[1][1];
double mu=-NMassM[2][3];
double g2v1= -NMassM[1][3]*sqrt(2.);
double g2v2= NMassM[1][2]*sqrt(2.);
double offQ=g2v1*g2v1+g2v2*g2v2;
double TrX2=offQ +M2*M2+mu*mu;
double detX=mu*M2 - g2v1*g2v2;
double D=TrX2*TrX2 - 4.*detX*detX;
double tU=(g2v2*g2v2-g2v1*g2v1-M2*M2+mu*mu-sqrt(D))/2./(M2*g2v2+mu*g2v1);
double tV=(g2v1*g2v1-g2v2*g2v2-M2*M2+mu*mu-sqrt(D))/2./(M2*g2v1+mu*g2v2);
double CU=cos(atan(tU));
double SU=sin(atan(tU));
double CV=cos(atan(tV));
double SV=sin(atan(tV));
double mc[2],Zv_[2][2],Zu_[2][2];
char name[10];
int i,j;
Zu_[0][0]=CU;
Zu_[0][1]=SU;
Zu_[1][0]=-SU;
Zu_[1][1]=CU;
Zv_[0][0]=CV;
Zv_[0][1]=SV;
Zv_[1][0]=-SV;
Zv_[1][1]=CV;
for(i=0;i<2;i++) mc[i]=g2v1*Zu_[i][0]*Zv_[i][1]
+g2v2*Zu_[i][1]*Zv_[i][0]
+ M2*Zu_[i][0]*Zv_[i][0]
+ mu*Zu_[i][1]*Zv_[i][1];
for(i=1;i<=2;i++)
{ sprintf(name,"MC%d",i);
assignValW(name,mc[i-1]);
for(j=1;j<=2;j++)
{
sprintf(name,"Zu%d%d",i,j);
assignValW(name,Zu_[i-1][j-1]);
sprintf(name,"Zv%d%d",i,j);
assignValW(name,Zv_[i-1][j-1]);
}
}
}
static void fillNeutralinoMassMatrix(void)
{ int i,j,k;
double M[5];
M[0]=findValW("MNE1");
M[1]=findValW("MNE2");
M[2]=findValW("MNE3");
M[3]=findValW("MNE4");
M[4]=findValW("MNE5");
for(i=0;i<5;i++) for(j=0;j<5;j++) for(k=0,NMassM[i][j]=0;k<5;k++)
NMassM[i][j]+=Zn_[k][i]*M[k]*Zn_[k][j];
assignValW("NMM55", NMassM[4][4]);
assignValW("NMM34", NMassM[2][3]);
assignValW("NMM35", NMassM[2][4]);
assignValW("NMM45", NMassM[3][4]);
assignValW("NMM13", NMassM[0][2]);
assignValW("NMM14", NMassM[0][3]);
assignValW("NMM23", NMassM[1][2]);
assignValW("NMM24", NMassM[1][3]);
CharginoZM();
}
int readVarMSSM(char * fname)
{ int rdCode;
char*vlist[32]={
"alfEMZ","alfSMZ","SW","MZ","Ml","MbMb","Mtp","tb","MG1","MG2",
"MG3","Am","Al","At","Ab","Au","Ad","MH3","mu","Ml2",
"Ml3","Mr2","Mr3","Mq2","Mq3","Mu2","Mu3","Md2","Md3","wt",
"wZ","wW"};
rdCode = readVarSpecial(fname,32,vlist);
assignValW("Ml1",findValW("Ml2"));
assignValW("Mr1",findValW("Mr2"));
assignValW("Mq1",findValW("Mq2"));
assignValW("Mu1",findValW("Mu2"));
assignValW("Md1",findValW("Md2"));
return rdCode;
}
static double higgspotent_(void)
{ int i,j;
double ee,sw,cw,lmax;
double MZ,alfEMZ,tb,At,Ab;
char name[10];
MZ=findValW("MZ");
alfEMZ=findValW("alfEMZ");
At=findValW("At");
Ab=findValW("Ab");
tb=findValW("tb");
for(i=1;i<=2;i++) for(j=1;j<=2;j++)
{ sprintf(name,"Pa%d%d",i,j); Pa_[i-1][j-1]=findValW(name);}
for(i=1;i<=3;i++) for(j=1;j<=3;j++)
{ sprintf(name,"Zh%d%d",i,j); Zh_[i-1][j-1]=findValW(name);}
for(i=1;i<=5;i++) for(j=1;j<=5;j++)
{ sprintf(name,"Zn%d%d",i,j); Zn_[i-1][j-1]=findValW(name);}
extpar.tb = findValW("tb");
extpar.Lambda = findValW("Lambda");
extpar.Kappa = findValW("Kappa");
extpar.aLambda = findValW("aLmbd0");
extpar.vev=findValW("vev");
ee=sqrt(4*M_PI*alfEMZ);
sw=sin(asin(extpar.vev*sqrt(2.0)*ee/MZ)/2);
cw=sqrt(1.0-sw*sw);
extpar.mw=MZ*cw;
extpar.g2=ee*ee/(sw*cw)/(sw*cw)/2;
extpar.aLambda=min1(extpar.aLambda-1, extpar.aLambda+1, varAlam);
varAlam(extpar.aLambda);
assignValW("mu",extpar.mu);
assignValW("aLmbda",extpar.aLambda);
assignValW("aKappa",extpar.aKappa);
fillNeutralinoMassMatrix();
for(i=1;i<=5;i++) {sprintf(name,"la%d",i); assignValW(name, La[i]);}
for(i=1;i<=2;i++) {sprintf(name,"la%ds",i); assignValW(name,Las[i]);}
assignValW("lass", Lass);
lmax=0;
for(i=0;i<10;i++)
{ if(lmax<fabs(La[i]))lmax=fabs(La[i]);
if(lmax<fabs(Las[i]))lmax=fabs(Las[i]);
}
if(lmax<fabs(Lass))lmax=fabs(Lass);
if(nCall>2000) return -1;
else return lmax;
}
int hbBlocksMDL(char*fname,int*nHch)
{ FILE * f=fopen(fname,"w");
double tb,sb,cb,Q;
if(!f) return 0;
Q=findValW("Q");
fprintf(f,"Block Mass\n 25 %E # Higgs Mass\n\n",findValW("Mh"));
slhaDecayPrint("h", 0,f);
slhaDecayPrint("t", 0,f);
slhaDecayPrint("~H+",0,f);
// MbSM=findValW("Mb");
fprintf(f,"Block HiggsBoundsInputHiggsCouplingsBosons\n");
fprintf(f,"# Effective coupling normalised to SM one and squared\n");
fprintf(f,"# For (*) normalized on Sin(2*W)\n");
fprintf(f," %12.4E 3 25 24 24 # higgs-W-W \n", 1. );
fprintf(f," %12.4E 3 25 23 23 # higgs-Z-Z \n", 1. );
fprintf(f," %12.4E 3 25 25 23 # higgs-higgs-Z \n", 0. );
{ double vev = findValW("V"),
Mh = findValW("Mh"),
aQCD=alphaQCD(Mh)/M_PI,
LGGSM=lGGhSM(Mh,aQCD, findValW("Mcp"),findValW("Mbp"),findValW("Mtp"),vev),
LAASM=lAAhSM(Mh,aQCD, findValW("Mcp"),findValW("Mbp"),findValW("Mtp"),vev);
fprintf(f," %12.4E 3 25 21 21 # higgs-gluon-gluon\n", 1. );
fprintf(f," %12.4E 3 25 22 22 # higgs-gamma-gamma\n", SQR(findValW("LAAh")/LAASM) );
}
fprintf(f,"Block HiggsBoundsInputHiggsCouplingsFermions\n");
fprintf(f,"# Effective coupling normalised to SM one and squared\n");
fprintf(f," %12.4E %12.4E 3 25 5 5 # higgs-b-b \n" ,1.,0.);
fprintf(f," %12.4E %12.4E 3 25 6 6 # higgs-top-top \n",1.,0.);
fprintf(f," %12.4E %12.4E 3 25 15 15 # higgs-tau-tau \n",1.,0.);
assignValW("Q",Q);
calcMainFunc();
fclose(f);
if(nHch) *nHch=1;
return 1;
}
int HBblocks(char * fname)
{ FILE * f=fopen(fname,"w");
double tb,sb,cb,Q;
if(!f) return 1;
Q=findValW("Q");
fprintf(f,"Block Mass\n 25 %E # Higgs Mass\n\n",findValW("Mh"));
slhaDecayPrint("h",f);
slhaDecayPrint("t",f);
slhaDecayPrint("~H+",f);
// MbSM=findValW("Mb");
fprintf(f,"Block HiggsBoundsInputHiggsCouplingsBosons\n");
fprintf(f,"# Effective coupling normalised to SM one and squared\n");
fprintf(f,"# For (*) normalized on Sin(2*W)\n");
fprintf(f," %12.4E 3 25 24 24 # higgs-W-W \n", 1. );
fprintf(f," %12.4E 3 25 23 23 # higgs-Z-Z \n", 1. );
fprintf(f," %12.4E 3 25 25 23 # higgs-higgs-Z \n", 0. );
{ assignVal("Q",pMass("h"));
calcMainFunc();
fprintf(f," %12.4E 3 25 21 21 # higgs-gluon-gluon\n", 1. );
fprintf(f," %12.4E 3 25 22 22 # higgs-gamma-gamma\n", SQR(findValW("LAAh")/findValW("LAAhSM")) );
}
fprintf(f,"Block HiggsBoundsInputHiggsCouplingsFermions\n");
fprintf(f,"# Effective coupling normalised to SM one and squared\n");
fprintf(f," %12.4E %12.4E 3 25 5 5 # higgs-b-b \n" ,1.,0.);
fprintf(f," %12.4E %12.4E 3 25 6 6 # higgs-top-top \n",1.,0.);
fprintf(f," %12.4E %12.4E 3 25 15 15 # higgs-tau-tau \n",1.,0.);
assignValW("Q",Q);
calcMainFunc();
fclose(f);
return 0;
}
void assignvalw_(char* f_name, double * val, int len)
{ char buff[20];
fName2c(f_name,buff,len);
assignValW(buff, *val);
}
int readlesh_(char *f_name,int len)
{
FILE *f;
char buff[100], name[20];
int n1,n2,i,err=0;
double val;
char fname[100];
char Zf[3][3]={"Zb","Zt","Zl"};
int MG1ok=0, MG2ok=0, AmOK=0;
fName2c(f_name,fname,len);
f=fopen(fname,"r");
if(f==NULL) return -2;
for(;;)
{ if(fscanf(f,"%s", buff)== EOF) break;
if(buff[0]=='#') { fscanf(f,"%*[^\n]\n"); continue;}
for(i=0;buff[i];i++) buff[i]=toupper(buff[i]);
if(strcmp(buff,"BLOCK")==0)
{ char rest[200];
char *c;
fscanf(f,"%s",buff);
if(fscanf(f,"%[^\n]",rest))
{ c=strchr(rest,'#');
if(c) c[0]=0;
c=strchr(rest,'=');
if(c && 1==sscanf(c+1,"%lf",&val))assignValW("QSUSY",val);
}
fscanf(f,"%*c");
for(i=0;buff[i];i++) buff[i]=toupper(buff[i]);
if(strcmp(buff,"MODSEL")==0)
{
for(;nfscanf(f,&n1,NULL,&val)==2;)
if(n1==1) assignValW("model",val);
}
else if(strcmp(buff,"SMINPUTS")==0)
{
for(;nfscanf(f,&n1,NULL,&val)==2;)
{
switch(n1)
{
case 1 : assignValW("alfEMZ", 1/val); break;
case 2 : assignValW("GF",val); break;
case 3 : assignValW("alfSMZ", val); break;
case 4 : assignValW("MZ", val); break;
case 5 : assignValW("MbMb",val); break;
case 6 : assignValW("Mtp",val); break;
case 7 : assignValW("Ml",val); break;
}
}
}
else if(strcmp(buff,"MINPAR")==0)
{ int model=findValW("model")+0.1;
while(2==nfscanf(f,&n1,NULL,&val))
switch(model)
{ case 0: if(n1==3) assignValW("tb",val); break;
case 1: switch(n1)
{ case 1: assignValW("M0",val);
assignValW("gMHu",val); assignValW("gMHd",val);
assignValW("gMl2",val); assignValW("gMl3",val);
assignValW("gMr2",val); assignValW("gMr3",val);
assignValW("gMq2",val); assignValW("gMq3",val);
assignValW("gMu2",val); assignValW("gMd2",val);
assignValW("gMu3",val); assignValW("gMd3",val);
break;
case 2: assignValW("Mhlf",val);
assignValW("gMG1",val); assignValW("gMG2",val); assignValW("gMG3",val);
break;
case 3: assignValW("tb",val); break;
case 4: assignValW("sgn",val); break;
case 5: assignValW("A0", val);
assignValW("gAl",val); assignValW("gAt",val); assignValW("gAb",val);
break;
} break;
case 2: switch(n1)
{ case 1: assignValW("Lambda",val); break;
case 2: assignValW("Mmess",val); break;
case 3: assignValW("tb",val); break;
case 4: assignValW("sgn",val); break;
case 5: assignValW("N5",val);
assignValW("N5_1",val);
assignValW("N5_2",val);
assignValW("N5_3",val); break;
case 6:
assignValW("Cgrav",val); break;
} break;
case 3: switch(n1)
{ case 1: assignValW("M0",val); break;
case 2: assignValW("M32",val); break;
case 3: assignValW("tb",val); break;
case 4: assignValW("sgn",val); break;
} break;
}
}
else if(strcmp(buff,"EXTPAR")==0) while(2==nfscanf(f,&n1,NULL,&val))
switch(n1)
{
case 1 : assignValW("gMG1" , val); break;
case 2 : assignValW("gMG2" , val); break;
case 3 : assignValW("gMG3" , val); break;
case 11 : assignValW("gAt" , val); break;
case 12 : assignValW("gAb" , val); break;
case 13 : assignValW("gAl" , val); break;
case 21 : if(val>0) assignValW("gMHd",sqrt(val));
else assignValW("gMHd",-sqrt(-val));
break;
case 22 : if(val>0)assignValW("gMHu", sqrt(val));
else assignValW("gMHu", -sqrt(-val));break;
case 23 : assignValW("mu", val); break;
case 26 : assignValW("MH3", val); break;
case 31 : assignValW("gMl1" , val); break;
case 32 : assignValW("gMl2" , val); break;
case 33 : assignValW("gMl3" , val); break;
case 34 : assignValW("gMr1" , val); break;
case 35 : assignValW("gMr2" , val); break;
case 36 : assignValW("gMr3" , val); break;
case 41 : assignValW("gMq1" , val); break;
case 42 : assignValW("gMq2" , val); break;
case 43 : assignValW("gMq3" , val); break;
case 44 : assignValW("gMu1" , val); break;
case 45 : assignValW("gMu2" , val); break;
case 46 : assignValW("gMu3" , val); break;
case 47 : assignValW("gMd1" , val); break;
case 48 : assignValW("gMd2" , val); break;
case 49 : assignValW("gMd3" , val); break;
case 51 : assignValW("N5_1" , val); break;
case 52 : assignValW("N5_2" , val); break;
case 53 : assignValW("N5_3" , val); break;
}
}
}
fclose(f);
return err;
}
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;
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 FillVal(int mode)
{
double Q=0.;
if(mode)
{ assignValW("MG1",slhaVal("EXTPAR", Q, 1, 1));
assignValW("MG2",slhaVal("EXTPAR", Q, 1, 2));
assignValW("MG3",slhaVal("EXTPAR", Q, 1, 3));
assignValW("At", slhaVal("EXTPAR", Q, 1, 11));
assignValW("Ab", slhaVal("EXTPAR", Q, 1, 12));
assignValW("Al", slhaVal("EXTPAR", Q, 1, 13));
assignValW("Ml2",slhaVal("EXTPAR", Q, 1, 32));
assignValW("Ml3",slhaVal("EXTPAR", Q, 1, 33));
assignValW("Mr2",slhaVal("EXTPAR", Q, 1, 35));
assignValW("Mr3",slhaVal("EXTPAR", Q, 1, 36));
assignValW("Mq2",slhaVal("EXTPAR", Q, 1, 42));
assignValW("Mq3",slhaVal("EXTPAR", Q, 1, 43));
assignValW("Mu2",slhaVal("EXTPAR", Q, 1, 45));
assignValW("Mu3",slhaVal("EXTPAR", Q, 1, 46));
assignValW("Md2",slhaVal("EXTPAR", Q, 1, 48));
assignValW("Md3",slhaVal("EXTPAR", Q, 1, 49));
assignValW("Mn2",slhaVal("EXTPAR", Q, 1, 58));
assignValW("Mnlr",slhaVal("EXTPAR", Q, 1,59));
assignValW("Alda",slhaVal("EXTPAR", Q, 1,63));
assignValW("mu", slhaVal("EXTPAR", Q, 1, 65));
assignValW("MZ2",slhaVal("EXTPAR", Q, 1,101));
assignValW("aZZ",slhaVal("EXTPAR", Q, 1,102));
assignValW("MK", slhaVal("EXTPAR", Q, 1,103));
assignValW("M1p",slhaVal("EXTPAR", Q, 1,104));
assignValW("tE6",slhaVal("EXTPAR", Q, 1,105));
}
if(mode>1)
{
assignValW("alfSMZ",slhaVal("SMINPUTS",Q,1,3) );
assignValW("MbMb", slhaVal("SMINPUTS",Q,1,5) );
assignValW("Mtp", slhaVal("SMINPUTS",Q,1,6) );
assignValW("Ml", slhaVal("SMINPUTS",Q,1,7) );
}
}
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;
}
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;
}
void FillVal(int mode)
{
double Q=91.;
if(mode)
{ assignValW("MH3",slhaVal("MASS", Q, 1, 36));
assignValW("mu", slhaVal("HMIX", Q, 1, 1) );
assignValW("MG1",slhaVal("MSOFT", Q, 1, 1));
assignValW("MG2",slhaVal("MSOFT", Q, 1, 2));
assignValW("MG3",slhaVal("MSOFT", Q, 1, 3));
assignValW("Ml1",slhaVal("MSOFT", Q, 1, 31));
assignValW("Ml2",slhaVal("MSOFT", Q, 1, 32));
assignValW("Ml3",slhaVal("MSOFT", Q, 1, 33));
assignValW("Mr1",slhaVal("MSOFT", Q, 1, 34));
assignValW("Mr2",slhaVal("MSOFT", Q, 1, 35));
assignValW("Mr3",slhaVal("MSOFT", Q, 1, 36));
assignValW("Mq1",slhaVal("MSOFT", Q, 1, 41));
assignValW("Mq2",slhaVal("MSOFT", Q, 1, 42));
assignValW("Mq3",slhaVal("MSOFT", Q, 1, 43));
assignValW("Mu1",slhaVal("MSOFT", Q, 1, 44));
assignValW("Mu2",slhaVal("MSOFT", Q, 1, 45));
assignValW("Mu3",slhaVal("MSOFT", Q, 1, 46));
assignValW("Md1",slhaVal("MSOFT", Q, 1, 47));
assignValW("Md2",slhaVal("MSOFT", Q, 1, 48));
assignValW("Md3",slhaVal("MSOFT", Q, 1, 49));
assignValW("At", slhaVal("Au", Q, 2, 3, 3) );
assignValW("Ab", slhaVal("Ad", Q, 2, 3, 3) );
assignValW("Al", slhaVal("Ae", Q, 2, 3, 3) );
assignValW("Am", slhaValExists("Ae",2,2,2)>0 ? slhaVal("Ae",Q,2,2,2):slhaVal("Al",Q,2,3,3));
assignValW("Ad", slhaValExists("Ad",2,2,2)>0 ? slhaVal("Ad",Q,2,2,2):slhaVal("Ad",Q,2,3,3));
assignValW("At", slhaVal("Au",Q,2,3,3));
assignValW("Au", slhaValExists("Au",2,2,2)>0 ? slhaVal("Au",Q,2,2,2):slhaVal("Au",Q,2,3,3));
}
if(mode>1)
{
assignValW("alfSMZ",slhaVal("SMINPUTS",Q,1,3) );
assignValW("MbMb", slhaVal("SMINPUTS",Q,1,5) );
assignValW("Mtp", slhaVal("SMINPUTS",Q,1,6) );
assignValW("Ml", slhaVal("SMINPUTS",Q,1,7) );
}
}
int main(int argc,char** argv)
{ int err;
char mess[10];
double dMb,dMd;
double (*LF)(double,double,double,double);
struct { char *lbl; double m0,mhf,A0,tb,sgn;}
testPoints[4]=
{
{"BP", 70, 250,-300,10, 1},
{"KP", 2500, 550, -80,40,-1},
{"IP", 180, 350, 0,35, 1},
{"NUH", 250, 530, 0,30, 1}
};
int I, K;
/* to save RGE input/output files uncomment the next line */
/*delFiles(0);*/
for(I=0;I<5;I++)
{
if(I==4)
{
printf("================================================ MSSM1 ======\n");
err=readVarMSSM("mssm1.par");
if(err==0)err=EWSBMODEL(RGE)();
}else
{
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");
printf("================================================ %s ======\n",testPoints[I].lbl);
PRINTRGE(RGE);
m0=testPoints[I].m0;
mhf=testPoints[I].mhf;
a0=testPoints[I].A0;
tb=testPoints[I].tb;
sgn=testPoints[I].sgn;
/*==== 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;
if(I==3){
/*==== Non universal SUGRA====*/
gMHu=2.*m0, gMHd=-0.6*m0;
}
err= SUGRAMODEL(RGE) (tb,
gMG1, gMG2, gMG3, gAl, gAt, gAb, sgn, gMHu, gMHd,
gMl2, gMl3, gMr2, gMr3, gMq2, gMq3, gMu2, gMu3, gMd2, gMd3);
if(err>0){ printf(" non fatal problems in RGE\n");err=0;}
}
if(err)
{ printf("Problem with RGE solution or spectrum calculation\n");
exit(1);
}
err=sortOddParticles(mess);
if(err) { printf("Can't calculate %s\n",mess); return 1;}
dMb=findValW("dMb");
dMd=findValW("dMd");
printf("dMb=%.2E dMd=dMs=%.2E \n", dMb, dMd);
for(K=1;K<=5;K++)
{
switch(K)
{
case 1: printf("================= Tree level \n");
QCDcorrections=0;
assignValW("dMb",0.);
assignValW("dMd",0.);
assignValW("dMs",0.); break;
case 2: printf("================= QCD \n");
QCDcorrections=1;
assignValW("dMb",0.);
assignValW("dMd",0.);
assignValW("dMs",0.);
break;
case 3: printf("================= dMb \n");
QCDcorrections=0;
assignValW("dMb",dMb);
assignValW("dMd",dMd);
assignValW("dMs",dMd);
break;
case 4: printf("================= QCD+dMb \n");
QCDcorrections=1;
assignValW("dMb",dMb);
assignValW("dMd",dMd);
assignValW("dMs",dMd);
break;
case 5: printf("================= box+QCD+dMb\n");
QCDcorrections=1;
assignValW("dMb",dMb);
assignValW("dMd",dMd);
assignValW("dMs",dMd);
break;
}
{ double pA0[2],pA5[2],nA0[2],nA5[2];
double Nmass=0.939; /*nucleon mass*/
double SCcoeff;
//printf("\n==== Calculation of WIMP-nucleons amplitudes =====\n");
if(K==5) LF=FeScLoop; else LF=NULL;
nucleonAmplitudes(LF, pA0,pA5,nA0,nA5);
// printf("WIMP-nucleon 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*lopmass_()/(Nmass+ lopmass_()),2.);
// printf("WIMP-nucleon cross sections:\n");
printf(" proton SI %.3E neutron SI %.3E\n",SCcoeff*pA0[0]*pA0[0],SCcoeff*nA0[0]*nA0[0]);
// printf(" neutron SI %.3E SD %.3E\n",SCcoeff*nA0[0]*nA0[0],SCcoeff*nA5[0]*nA5[0]);
}
}
}
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,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 HBblocks(char * fname)
{ FILE * f=fopen(fname,"a");
double tb,sb,cb,alpha,sa,ca,ta,samb,camb,dMb,MbHl,MbSM,MbH,MbH3,Q;
if(!f) return 1;
Q=findValW("Q");
if(slhaDecayExists(pNum("h")) <0) slhaDecayPrint("h", f);
if(slhaDecayExists(pNum("H")) <0) slhaDecayPrint("H", f);
if(slhaDecayExists(pNum("H3"))<0) slhaDecayPrint("H3",f);
if(slhaDecayExists(pNum("t")) <0) slhaDecayPrint("t", f);
if(slhaDecayExists(pNum("H+"))<0) slhaDecayPrint("H+",f);
tb=findValW("tB");
sb=tb/sqrt(1+tb*tb);
cb=1/sqrt(1+tb*tb);
alpha=findValW("alpha");
sa=sin(alpha);
ca=cos(alpha);
ta=sa/ca;
samb=sa*cb-ca*sb;
camb=ca*cb+sa*sb;
dMb=findValW("dMb");
MbSM=findValW("Mb");
MbH= MbSM/(1+dMb)*(1+dMb*ta/tb);
MbH3=MbSM/(1+dMb)*(1-dMb/tb/tb);
MbHl=MbSM/(1+dMb)*(1-dMb/ta/tb);
fprintf(f,"Block HiggsBoundsInputHiggsCouplingsBosons\n");
fprintf(f,"# Effective coupling normalised to SM one and squared\n");
fprintf(f,"# For (*) normalized on Sin(2*W)\n");
fprintf(f," %12.4E 3 25 24 24 # higgs-W-W \n", SQR(samb) );
fprintf(f," %12.4E 3 25 23 23 # higgs-Z-Z \n", SQR(samb) );
fprintf(f," %12.4E 3 25 25 23 # higgs-higgs-Z \n", 0. );
{ assignVal("Q",pMass("h"));
calcMainFunc();
fprintf(f," %12.4E 3 25 21 21 # higgs-gluon-gluon\n", SQR(findValW("LGGh")/findValW("LGGSM")) );
fprintf(f," %12.4E 3 25 22 22 # higgs-gamma-gamma\n", SQR(findValW("LAAh")/findValW("LAASM")) );
}
fprintf(f," %12.4E 3 35 24 24 # higgs-W-W \n", SQR(camb) );
fprintf(f," %12.4E 3 35 23 23 # higgs-Z-Z \n", SQR(camb) );
fprintf(f," %12.4E 3 35 25 23 # higgs-higgs-Z \n", 0. );
fprintf(f," %12.4E 3 35 35 23 # higgs-higgs-Z \n", 0. );
{ assignVal("Q",pMass("H"));
calcMainFunc();
fprintf(f," %12.4E 3 35 21 21 # higgs-gluon-gluon\n",SQR(findValW("LGGH")/findValW("LGGSM")) );
fprintf(f," %12.4E 3 35 22 22 # higgs-gamma-gamma\n",SQR(findValW("LAAH")/findValW("LAASM")) );
}
fprintf(f," %12.4E 3 36 24 24 # higgs-W-W \n", 0. );
fprintf(f," %12.4E 3 36 23 23 # higgs-Z-Z \n", 0. );
{ assignVal("Q",pMass("H3"));
calcMainFunc();
fprintf(f," %12.4E 3 36 21 21 # higgs-gluon-gluon\n",SQR(findValW("LGGH3")/2/findValW("LGGSM")) );
fprintf(f," %12.4E 3 36 22 22 # higgs-gamma-gamma\n",SQR(findValW("LAAH3")/2/findValW("LAASM")) );
}
fprintf(f," %12.4E 3 36 25 23 #*higgs-higgs-Z \n", SQR(camb) );
fprintf(f," %12.4E 3 36 35 23 #*higgs-higgs-Z \n", SQR(samb) );
fprintf(f," %12.4E 3 36 36 23 #* higgs-higgs-Z \n", 0. );
fprintf(f,"Block HiggsBoundsInputHiggsCouplingsFermions\n");
fprintf(f,"# Effective coupling normalised to SM one and squared\n");
fprintf(f," %12.4E %12.4E 3 25 5 5 # higgs-b-b \n" ,SQR((sa/cb)*(MbHl/MbSM)),0.);
fprintf(f," %12.4E %12.4E 3 25 6 6 # higgs-top-top \n",SQR(ca/sb) ,0.);
fprintf(f," %12.4E %12.4E 3 25 15 15 # higgs-tau-tau \n",SQR(sa/cb) ,0.);
fprintf(f," %12.4E %12.4E 3 35 5 5 # higgs-b-b \n" ,SQR((ca/cb)*(MbH/MbSM)) ,0.);
fprintf(f," %12.4E %12.4E 3 35 6 6 # higgs-top-top \n",SQR(sa/sb) ,0.);
fprintf(f," %12.4E %12.4E 3 35 15 15 # higgs-tau-tau \n",SQR(ca/cb) ,0.);
fprintf(f," %12.4E %12.4E 3 36 5 5 # higgs-b-b \n" ,0.,SQR(tb*(MbH3/MbSM)));
fprintf(f," %12.4E %12.4E 3 36 6 6 # higgs-top-top \n",0.,SQR(1/tb) );
fprintf(f," %12.4E %12.4E 3 36 15 15 # higgs-tau-tau \n",0.,SQR(tb) );
assignValW("Q",Q);
calcMainFunc();
fclose(f);
return 0;
}