Пример #1
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;
}
Пример #2
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;
}
Пример #3
0
int main(int argc,char** argv)
{  int err;
   char cdmName[10];
   int spin2, charge3,cdim;

  ForceUG=0;  /* to Force Unitary Gauge assign 1 */
  
  if(argc==1)
  { 
      printf(" Correct usage:  ./main <file with parameters> \n");
      exit(1);
  }
                               

/*  err=readVar(argv[1]);*/
   err=readVarRHNM(argv[1]);
  if(err==-1)     {printf("Can not open the file\n"); exit(1);}
  else if(err>0)  { printf("Wrong file contents at line %d\n",err);exit(1);}


  err=sortOddParticles(cdmName);
  if(err) { printf("Can't calculate %s\n",cdmName); return 1;}
  qNumbers(cdmName, &spin2, &charge3, &cdim);
  printf("\nDark matter candidate is '%s' with spin=%d/2 \n",cdmName,spin2); 
  if(charge3) { printf("Dark Matter has electric charge %d/3\n",charge3); exit(1);}
  if(cdim!=1) { printf("Dark Matter is a color particle\n"); exit(1);}
  if(strcmp(cdmName,"~n4")) printf(" ~n4 is not CDM\n"); 
                               
#ifdef MASSES_INFO
{
  printf("\n=== MASSES OF PARTICLES OF ODD SECTOR: ===\n");
  printMasses(stdout,1);
}
#endif

#ifdef CONSTRAINTS
#endif

#ifdef OMEGA
{ int fast=1;
  double Beps=1.E-5, cut=0.01;
  double Omega,Xf; 

// to include processes with virtual W/Z in DM   annihilation      
//   VZdecay=1; VWdecay=1; cleanDecayTable(); 

// to include processes with virtual W/Z  also  in co-annihilation 
//   VZdecay=2; VWdecay=2; cleanDecayTable(); 
    
  printf("\n==== Calculation of relic density =====\n");  



  Omega=darkOmega(&Xf,fast,Beps);
  printf("Xf=%.2e Omega=%.2e\n",Xf,Omega);
  printChannels(Xf,cut,Beps,1,stdout);
}
#endif


#ifdef INDIRECT_DETECTION
{ 
  int err,i;
  double Emin=1,/* Energy cut  in GeV   */  sigmaV;
  double vcs_gz,vcs_gg;
  char txt[100];
  double SpA[NZ],SpE[NZ],SpP[NZ];
  double FluxA[NZ],FluxE[NZ],FluxP[NZ];
  double * SpNe=NULL,*SpNm=NULL,*SpNl=NULL;
  double Etest=Mcdm/2;
  
printf("\n==== Indirect detection =======\n");  

  sigmaV=calcSpectrum(1+2+4,SpA,SpE,SpP,SpNe,SpNm,SpNl ,&err);
    /* Returns sigma*v in cm^3/sec.     SpX - calculated spectra of annihilation.
       Use SpectdNdE(E, SpX) to calculate energy distribution in  1/GeV units.
       
       First parameter 1-includes W/Z polarization
                       2-includes gammas for 2->2+gamma
                       4-print cross sections             
    */
  printf("sigmav=%.2E[cm^3/s]\n",sigmaV);  


  if(SpA)
  { 
     double fi=0.1,dfi=0.05; /* angle of sight and 1/2 of cone angle in [rad] */ 

     gammaFluxTab(fi,dfi, sigmaV, SpA,  FluxA);     
     printf("Photon flux  for angle of sight f=%.2f[rad]\n"
     "and spherical region described by cone with angle %.2f[rad]\n",fi,2*dfi);
#ifdef SHOWPLOTS
     sprintf(txt,"Photon flux[cm^2 s GeV]^{1} at f=%.2f[rad], cone angle %.2f[rad]",fi,2*dfi);
     displaySpectrum(FluxA,txt,Emin,Mcdm,1);
#endif
     printf("Photon flux = %.2E[cm^2 s GeV]^{-1} for E=%.1f[GeV]\n",SpectdNdE(Etest, FluxA), Etest);       
  }

  if(SpE)
  { 
    posiFluxTab(Emin, sigmaV, SpE, FluxE);
#ifdef SHOWPLOTS     
    displaySpectrum(FluxE,"positron flux [cm^2 s sr GeV]^{-1}" ,Emin,Mcdm,1);
#endif
    printf("Positron flux  =  %.2E[cm^2 sr s GeV]^{-1} for E=%.1f[GeV] \n",
    SpectdNdE(Etest, FluxE),  Etest);           
  }
  
  if(SpP)
  { 
    pbarFluxTab(Emin, sigmaV, SpP, FluxP  ); 
#ifdef SHOWPLOTS    
     displaySpectrum(FluxP,"antiproton flux [cm^2 s sr GeV]^{-1}" ,Emin,Mcdm,1);
#endif
    printf("Antiproton flux  =  %.2E[cm^2 sr s GeV]^{-1} for E=%.1f[GeV] \n",
    SpectdNdE(Etest, FluxP),  Etest);             
  }
}  
#endif

#ifdef RESET_FORMFACTORS
{
/* 
   The user has approach to form factors  which specifies quark contents 
   of  proton and nucleon via global parametes like
      <Type>FF<Nucleon><q>
   where <Type> can be "Scalar", "pVector", and "Sigma"; 
         <Nucleon>     "P" or "N" for proton and neutron
         <q>            "d", "u","s"

   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");   

    nucleonAmplitudes(FeScLoop, pA0,pA5,nA0,nA5);
    printf("CDM[antiCDM]-nucleon micrOMEGAs amplitudes:\n");
    printf("proton:  SI  %.3E [%.3E]  SD  %.3E [%.3E]\n",pA0[0], pA0[1],  pA5[0], pA5[1] );
    printf("neutron: SI  %.3E [%.3E]  SD  %.3E [%.3E]\n",nA0[0], nA0[1],  nA5[0], nA5[1] ); 

  SCcoeff=4/M_PI*3.8937966E8*pow(Nmass*Mcdm/(Nmass+ Mcdm),2.);
    printf("CDM[antiCDM]-nucleon cross sections[pb]:\n");
    printf(" proton  SI %.3E [%.3E] SD %.3E [%.3E]\n",
       SCcoeff*pA0[0]*pA0[0],SCcoeff*pA0[1]*pA0[1],3*SCcoeff*pA5[0]*pA5[0],3*SCcoeff*pA5[1]*pA5[1]);
    printf(" neutron SI %.3E [%.3E] SD %.3E [%.3E]\n",
       SCcoeff*nA0[0]*nA0[0],SCcoeff*nA0[1]*nA0[1],3*SCcoeff*nA5[0]*nA5[0],3*SCcoeff*nA5[1]*nA5[1]);
}
#endif
  
#ifdef CDM_NUCLEUS
{ double dNdE[300];
  double nEvents;

printf("\n======== Direct Detection ========\n");    

  nEvents=nucleusRecoil(Maxwell,73,Z_Ge,J_Ge73,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=10; //GeV
  spectrInfo(Emin/Mcdm,nu, &Ntot,NULL);
    printf(" E>%.1E GeV neutrino flux       %E [1/Year/km^2] \n",Emin,Ntot);
  spectrInfo(Emin/Mcdm,nu_bar, &Ntot,NULL);
    printf(" E>%.1E GeV anti-neutrino flux  %E [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    %E [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 %E [1/Year/km^3]\n",Emin,Ntot);
  }
}
#endif

#ifdef DECAYS
{  
   txtList L;
   double width,br;
   char * pname;
   
    if(!VZdecay || !VWdecay  ){ cleanDecayTable(); VZdecay=1; VWdecay=1;}

   printf("\n Calculation of particle decays\n");
   pname = "H";
    width=pWidth(pname,&L);
    printf("\n%s :   total width=%E \n and Branchings:\n",pname,width);
    printTxtList(L,stdout);

   pname = "Zp";
    width=pWidth(pname,&L);
    printf("\n%s :   total width=%E \n and Branchings:\n",pname,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");
  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;
}
Пример #4
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;
}
Пример #5
0
static double calcSpectrum0(char *name1,char*name2, int forSun,   double *Spectranu, double *SpectraNu)
{
  int i,k;
  double vcsSum=0; 
  int ntot,err;
  double * v_cs;
  
  char name1L[10],name2L[10], lib[20],process[400];
  numout * libPtr;
  
  for(i=0;i<NZ;i++) Spectranu[i]=SpectraNu[i]=0;  

  pname2lib(name1,name1L);
  pname2lib(name2,name2L);
  sprintf(lib,"omg_%s%s",name1L,name2L);
  sprintf(process,"%s,%s->AllEven,1*x{%s",name1,name2,EvenParticles());
// Warning!!   in should be done in the same manner as annihilation libraries for Omega
  libPtr=getMEcode(0,ForceUG,process,NULL,NULL,lib);
  
  
  if(!libPtr) return 0;
  passParameters(libPtr);
  procInfo1(libPtr,&ntot,NULL,NULL); 

  
  v_cs=malloc(sizeof(double)*ntot);
  (*libPtr->interface->twidth)=0;
  
  for(k=0;k<ntot;k++)
  { double m[4];
    char *N[4];
    procInfo2(libPtr,k+1,N,m);
    if((m[2]+m[3])/(m[0]+m[1])<1)
    { 
#ifdef V0    
      v_cs[k]=V0*cs22(libPtr,k+1,V0*m[0]/2,-1.,1.,&err);
#else 
      v_cs[k]= vcs22(libPtr,k+1,&err);
#endif 
      if(v_cs[k]<0) v_cs[k]=0; 
      vcsSum+=v_cs[k];
    } else v_cs[k]=-1;
  }
   
  for(k=0;k<ntot ;k++) if(v_cs[k]>=0)
  { char * N[4];
    double m[4];
    int l, charge3[2],spin2[2],cdim[2],pdg[2];
    int PlusAok=0;

    procInfo2(libPtr,k+1,N,m);
    for(l=0;l<2;l++)  pdg[l]=qNumbers(N[2+l],spin2+l,charge3+l,NULL);

            
    if(v_cs[k]>1.E-3*vcsSum) 
    {  double tab2[NZ]; 
#ifdef PRINT
       { char txt[100];
         sprintf(txt,"%s,%s -> %s %s", N[0],N[1],N[2],N[3]);
         printf("  %-20.20s  %.2E\n",txt,v_cs[k]*2.9979E-26);
       }
#endif       
       for(l=0;l<2;l++) switch(abs(pdg[l]))  
       {  
         case 12: case 14: case 16:
         if(pdg[l]>0)
         {
           basicNuSpectra(forSun,pdg[l],1,tab2);   
           for(i=0;i<NZ;i++) Spectranu[i]+=tab2[i]*v_cs[k]/vcsSum;
         } else 
         {      
           basicNuSpectra(forSun,pdg[l],-1,tab2);
           for(i=0;i<NZ;i++) SpectraNu[i]+=tab2[i]*v_cs[k]/vcsSum;
         }  
         break;
         default:   
         basicNuSpectra(forSun,pdg[l],1,tab2);
          for(i=0;i<NZ;i++) Spectranu[i]+=0.5*tab2[i]*v_cs[k]/vcsSum;
         basicNuSpectra(forSun,pdg[l],-1,tab2);
          for(i=0;i<NZ;i++) SpectraNu[i]+=0.5*tab2[i]*v_cs[k]/vcsSum;    
       }
    } 
  }
  
  free(v_cs);
  return  vcsSum*2.9979E-26;
}
Пример #6
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;
}
Пример #7
0
int main(int argc,char** argv)
{ int err;
  char cdmName[10];
  int spin2, charge3,cdim;

  ForceUG=0;  /* to Force Unitary Gauge assign 1 */  

  if(argc==1)
  { 
      printf(" Correct usage:  ./main  <file with  parameters> \n");
      printf("Example: ./main data1.par\n");
      exit(1);
  }
                               
/*  err=readVar(argv[1]);*/
  err=readVarlHiggs(argv[1]);
  
  if(err==-1)     {printf("Can not open the file\n"); exit(1);}
  else if(err>0)  { printf("Wrong file contents at line %d\n",err);exit(1);}
           

  err=sortOddParticles(cdmName);
  if(err) { printf("Can't calculate %s\n",cdmName); return 1;}

printf("ok1\n");
  
  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,"~A")) printf(" ~A is not CDM\n");                

#ifdef MASSES_INFO
{
  printf("\n=== MASSES OF PARTICLES OF ODD SECTOR: ===\n");
  printHiggs(stdout);
  printMasses(stdout,1);
    
}
#endif

#ifdef CONSTRAINTS

#endif

#ifdef OMEGA
{ int fast=1;
  double Beps=1.E-5, cut=0.01;
  double Omega,Xf;   
  printf("\n==== Calculation of relic density =====\n");  

  Omega=darkOmega(&Xf,fast,Beps);
  printf("Xf=%.2e Omega=%.2e\n",Xf,Omega);
  printChannels(Xf,cut,Beps,1,stdout);
}
#endif

#ifdef INDIRECT_DETECTION
{ 
  int err,i;
  double Emin=1,/* Energy cut  in GeV   */  sigmaV;
  double vcs_gz,vcs_gg;
  char txt[100];
  double SpA[NZ],SpE[NZ],SpP[NZ];
  double FluxA[NZ],FluxE[NZ],FluxP[NZ];
  double * SpNe=NULL,*SpNm=NULL,*SpNl=NULL;
  double Etest=Mcdm/2;
  
printf("\n==== Indirect detection =======\n");  

  sigmaV=calcSpectrum(1+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(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]); 

  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,NULL,dNdE);

  printf("73Ge: Total number of events=%.2E /day/kg\n",nEvents);
  printf("Number of events in 10 - 50 KeV region=%.2E /day/kg\n",
                                   cutRecoilResult(dNdE,10,50));
                                                                                                         
#ifdef SHOWPLOTS
    displayRecoilPlot(dNdE,"Distribution of recoil energy of 73Ge",0,199);
#endif

  nEvents=nucleusRecoil(Maxwell,131,Z_Xe,J_Xe131,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

  nEvents=nucleusRecoil(Maxwell,23,Z_Na,J_Na23,S00Na23,S01Na23,S11Na23,NULL,dNdE);

  printf("23Na: Total number of events=%.2E /day/kg\n",nEvents);
  printf("Number of events in 10 - 50 KeV region=%.2E /day/kg\n",
                                   cutRecoilResult(dNdE,10,50));                                   
#ifdef SHOWPLOTS
    displayRecoilPlot(dNdE,"Distribution of recoil energy of 23Na",0,199);
#endif

  nEvents=nucleusRecoil(Maxwell,127,Z_I,J_I127,S00I127,S01I127,S11I127,NULL,dNdE);

  printf("I127: Total number of events=%.2E /day/kg\n",nEvents);
  printf("Number of events in 10 - 50 KeV region=%.2E /day/kg\n",
                                   cutRecoilResult(dNdE,10,50));                                   
#ifdef SHOWPLOTS
    displayRecoilPlot(dNdE,"Distribution of recoil energy of 127I",0,199);
#endif
  
}
#endif 

#ifdef DECAYS
{  
  txtList L;
   int dim;
   double width,br;
   char * pname;
   
   printf("\n Calculation of particle decays\n");
   pname = "H";
    width=pWidth(pname,&L,&dim);
    printf("%s->%d*x :   total width=%E \n and Branchings:\n",pname,dim,width);
    printTxtList(L,stdout);

   pname = "e3";
    width=pWidth(pname,&L,&dim);
    printf("%s->%d*x :   total width=%E \n and Branchings:\n",pname,dim,width);
    printTxtList(L,stdout);
    printf("Br(e1,N1,n3)= %E\n",findBr(L,"e1,N1,n3"));

   pname = "~W+";
    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;
}