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DM-v54.patch
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DM-v54.patch
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diff -c source/create_galaxy.cc source-dm/create_galaxy.cc
*** source/create_galaxy.cc 2021-01-24 17:16:35.580614619 +0100
--- source-dm/create_galaxy.cc 2021-01-24 17:17:44.115811067 +0100
***************
*** 32,38 ****
galaxy.init(galdef.x_min, galdef.x_max, galdef.dx,
galdef.y_min, galdef.y_max, galdef.dy,
galdef.z_min, galdef.z_max, galdef.dz);
! }
// GAS and B-FIELD DISTRIBUTION
nH_set_model(galdef.nHI_model, galdef.nH2_model, galdef.nHII_model, 0); //AWS20090814
--- 32,40 ----
galaxy.init(galdef.x_min, galdef.x_max, galdef.dx,
galdef.y_min, galdef.y_max, galdef.dy,
galdef.z_min, galdef.z_max, galdef.dz);
! }
! if(galdef.DM_gammas==2) {INFO("Exit"); return 0; } //AE20160503
!
// GAS and B-FIELD DISTRIBUTION
nH_set_model(galdef.nHI_model, galdef.nH2_model, galdef.nHII_model, 0); //AWS20090814
***************
*** 327,333 ****
// SYNCHROTRON EMISSION
! if (galdef.synchrotron >= 1) { //AWS20080229
galaxy.nu_synch_min = galdef.nu_synch_min;
galaxy.nu_synch_max = galdef.nu_synch_max;
--- 329,336 ----
// SYNCHROTRON EMISSION
! if (galdef.synchrotron >= 1) { //AWS20080229
! if (galdef.DM_int9 == 0) {
galaxy.nu_synch_min = galdef.nu_synch_min;
galaxy.nu_synch_max = galdef.nu_synch_max;
***************
*** 360,365 ****
--- 363,392 ----
}
INFO(sBuf.str());
+ } // if DM_int9 AE20140924
+
+ else {
+ galaxy.n_nu_synchgrid = galdef.DM_int9;
+ galaxy.nu_synch = new double[galaxy.n_nu_synchgrid];
+
+ ostringstream sBuf;
+ sBuf << "Synchrotron frequency grid: ";
+
+ for (int inusynch = 0; inusynch < galaxy.n_nu_synchgrid; ++inusynch) {
+
+ galaxy.nu_synch[inusynch] = galdef.DM_double3[inusynch];
+
+ sBuf << galaxy.nu_synch[inusynch] << " ";
+
+ }
+
+ galaxy.nu_synch_min = galaxy.nu_synch[0];
+ galaxy.nu_synch_max = galaxy.nu_synch[galaxy.n_nu_synchgrid-1];
+ galaxy.nu_synch_factor = 1;
+
+ INFO(sBuf.str());
+ } // else DM_int8 AE20140924
+
/* Moved to Galprop.cc Gulli20071003
if (galdef.n_spatial_dimensions == 2) {
diff -c source/create_gcr.cc source-dm/create_gcr.cc
*** source/create_gcr.cc 2021-01-24 17:16:35.703616766 +0100
--- source-dm/create_gcr.cc 2021-01-24 17:17:44.148811643 +0100
***************
*** 66,72 ****
}
if(galdef.verbose >= 1)cout<<endl<<"Number of species to create: n_species= "<<n_species<<endl<<endl;
! if(!n_species) {cout<<"create_gcr.cc: No particles specified -exit"<<endl; exit(1);}
// create a Particle array
delete[] gcr;
--- 66,72 ----
}
if(galdef.verbose >= 1)cout<<endl<<"Number of species to create: n_species= "<<n_species<<endl<<endl;
! if(!n_species && !galdef.DM_gammas) {cout<<"create_gcr.cc: No particles specified -exit"<<endl; exit(1);} // AE20160501 added "DM_gammas"
// create a Particle array
delete[] gcr;
diff -c source/Galdef.cc source-dm/Galdef.cc
*** source/Galdef.cc 2021-01-24 17:16:53.572928718 +0100
--- source-dm/Galdef.cc 2021-01-24 17:17:44.233813127 +0100
***************
*** 857,864 ****
stat= read_galdef_parameter ( filename,parstring,&DM_double1 );
strcpy ( parstring, "DM_double2" );
stat= read_galdef_parameter ( filename,parstring,&DM_double2 );
! strcpy ( parstring, "DM_double3" );
! stat= read_galdef_parameter ( filename,parstring,&DM_double3 );
strcpy ( parstring, "DM_double4" );
stat= read_galdef_parameter ( filename,parstring,&DM_double4 );
strcpy ( parstring, "DM_double5" );
--- 857,864 ----
stat= read_galdef_parameter ( filename,parstring,&DM_double1 );
strcpy ( parstring, "DM_double2" );
stat= read_galdef_parameter ( filename,parstring,&DM_double2 );
! // strcpy ( parstring, "DM_double3" );
! // stat= read_galdef_parameter ( filename,parstring,&DM_double3 );
strcpy ( parstring, "DM_double4" );
stat= read_galdef_parameter ( filename,parstring,&DM_double4 );
strcpy ( parstring, "DM_double5" );
***************
*** 893,898 ****
--- 893,902 ----
strcpy ( parstring, "DM_int9" );
stat= read_galdef_parameter ( filename,parstring,&DM_int9 );
+ DM_double3 = new double[DM_int9]; //AE20140924
+ strcpy ( parstring, "DM_double3" ); //
+ stat= read_galdef_parameter ( filename,parstring,DM_double3,DM_int9 ); //
+
//output controls
strcpy ( parstring, "skymap_format" );
stat= read_galdef_parameter ( filename,parstring,&skymap_format );
***************
*** 1585,1591 ****
cout<<" DM_double0 "<<DM_double0 <<endl;
cout<<" DM_double1 "<<DM_double1 <<endl;
cout<<" DM_double2 "<<DM_double2 <<endl;
! cout<<" DM_double3 "<<DM_double3 <<endl;
cout<<" DM_double4 "<<DM_double4 <<endl;
cout<<" DM_double5 "<<DM_double5 <<endl;
cout<<" DM_double6 "<<DM_double6 <<endl;
--- 1589,1598 ----
cout<<" DM_double0 "<<DM_double0 <<endl;
cout<<" DM_double1 "<<DM_double1 <<endl;
cout<<" DM_double2 "<<DM_double2 <<endl;
! cout<<" DM_double3 "; //<<DM_double3 <<endl;
! for (int i=0; i<DM_int9; i++)
! cout<<DM_double3[i]<<", ";
! cout<<endl; //AE20140926
cout<<" DM_double4 "<<DM_double4 <<endl;
cout<<" DM_double5 "<<DM_double5 <<endl;
cout<<" DM_double6 "<<DM_double6 <<endl;
diff -c source/Galdef.h source-dm/Galdef.h
*** source/Galdef.h 2021-01-24 17:16:53.210922398 +0100
--- source-dm/Galdef.h 2021-01-24 17:17:44.130811329 +0100
***************
*** 187,193 ****
int DM_antiprotons; // 1=compute antiprotons from DM
int DM_gammas; // 1=compute gamma rays from DM
double // user-defined params of DM (double)
! DM_double0, DM_double1, DM_double2, DM_double3, DM_double4,
DM_double5, DM_double6, DM_double7, DM_double8, DM_double9;
int // user-defined params of DM (int)
DM_int0, DM_int1, DM_int2, DM_int3, DM_int4,
--- 187,193 ----
int DM_antiprotons; // 1=compute antiprotons from DM
int DM_gammas; // 1=compute gamma rays from DM
double // user-defined params of DM (double)
! DM_double0, DM_double1, DM_double2, *DM_double3, DM_double4, //AE2014 - added pointer *
DM_double5, DM_double6, DM_double7, DM_double8, DM_double9;
int // user-defined params of DM (int)
DM_int0, DM_int1, DM_int2, DM_int3, DM_int4,
diff -c source/Galprop.h source-dm/Galprop.h
*** source/Galprop.h 2021-01-24 17:16:53.071919972 +0100
--- source-dm/Galprop.h 2021-01-24 17:17:44.115811067 +0100
***************
*** 49,56 ****
int gen_DM_source ( Particle& );
int gen_DM_emiss();
double DM_profile ( double, double, double );
! double DM_profile_av ( double,double,double,double,double );
! double DM_profile_av ( double,double,double,double,double,double,double );
int gen_DM_skymap();
int store_DM_emiss();
int store_DM_skymap();
--- 49,57 ----
int gen_DM_source ( Particle& );
int gen_DM_emiss();
double DM_profile ( double, double, double );
! double DM_profile_av ( double,double,double,double ); //AE20131218
! double DM_profile_av ( double,double,double,double,double,double ); //AE20131218
! double DM_subs_boost ( double, double, double ); //AE20131218
int gen_DM_skymap();
int store_DM_emiss();
int store_DM_skymap();
diff -c source/gen_DM_skymap.cc source-dm/gen_DM_skymap.cc
*** source/gen_DM_skymap.cc 2021-01-24 17:16:52.933917564 +0100
--- source-dm/gen_DM_skymap.cc 2021-01-24 17:17:44.069810264 +0100
***************
*** 61,66 ****
--- 61,67 ----
//**"****!****"****!****"****!****"****!****"****!****"****!****"****!****"****|
// calc. of a 2D array of g-ray emission for the given E_gammagrid for a
// particular pixel (l,b) IMOS20080114
+ // "gcr" was replaced by "galdef" AE20160501
//**"****!****"****!****"****!****"****!****"****!****"****!****"****!****"****|
int Galprop::gen_DM_skymap_pixel(const double l, const double b, vector<double> &DM){
double dtr=acos(-1.)/180.;
***************
*** 88,94 ****
double xx,yy; //IMOS20080114
// checks if we got to the Galactic boundary in 2D, if so stop integration
! if(gcr[0].n_spatial_dimensions==2)
{
// find the nearest grid points on the LEFT side of the current point
ir=(int)((RR-galaxy.r_min)/galaxy.dr);
--- 89,95 ----
double xx,yy; //IMOS20080114
// checks if we got to the Galactic boundary in 2D, if so stop integration
! if(galdef.n_spatial_dimensions==2)
{
// find the nearest grid points on the LEFT side of the current point
ir=(int)((RR-galaxy.r_min)/galaxy.dr);
***************
*** 107,113 ****
} // particle.n_spatial_dimensions==2
// checks if we got to the Galactic boundary in 3D, if so stop integration
! if(gcr[0].n_spatial_dimensions==3)
{
xx=Rsun-d*cosb*cosl; // 3D: Sun on x axis at x=+Rsun
yy= -d*cosb*sinl; // 3D: Sun at y=0; +ve long=-ve y since Z=X^Y system
--- 108,114 ----
} // particle.n_spatial_dimensions==2
// checks if we got to the Galactic boundary in 3D, if so stop integration
! if(galdef.n_spatial_dimensions==3)
{
xx=Rsun-d*cosb*cosl; // 3D: Sun on x axis at x=+Rsun
yy= -d*cosb*sinl; // 3D: Sun at y=0; +ve long=-ve y since Z=X^Y system
***************
*** 141,147 ****
{
float delta, x[8][3],f[8],y[7];
! if(gcr[0].n_spatial_dimensions==2)
{
if (ir==galaxy.n_rgrid-1 || iz==galaxy.n_zgrid-1)
delta = dd*kpc2cm *galaxy.DM_emiss.d2[ir][iz] .s[iEgamma];
--- 142,148 ----
{
float delta, x[8][3],f[8],y[7];
! if(galdef.n_spatial_dimensions==2)
{
if (ir==galaxy.n_rgrid-1 || iz==galaxy.n_zgrid-1)
delta = dd*kpc2cm *galaxy.DM_emiss.d2[ir][iz] .s[iEgamma];
***************
*** 163,169 ****
delta = dd*kpc2cm *y[2];
}
}
! if(gcr[0].n_spatial_dimensions==3)
{
if (ix==galaxy.n_xgrid-1 || iy==galaxy.n_ygrid-1 || iz==galaxy.n_zgrid-1)
delta = dd*kpc2cm *galaxy.DM_emiss.d3[ix][iy][iz].s[iEgamma];
--- 164,170 ----
delta = dd*kpc2cm *y[2];
}
}
! if(galdef.n_spatial_dimensions==3)
{
if (ix==galaxy.n_xgrid-1 || iy==galaxy.n_ygrid-1 || iz==galaxy.n_zgrid-1)
delta = dd*kpc2cm *galaxy.DM_emiss.d3[ix][iy][iz].s[iEgamma];
diff -c source/gen_DM_source.cc source-dm/gen_DM_source.cc
*** source/gen_DM_source.cc 2021-01-24 17:16:53.005918820 +0100
--- source-dm/gen_DM_source.cc 2021-01-24 17:17:44.184812272 +0100
***************
*** 3,16 ****
// * gen_DM_source.cc * galprop package * 9/09/2005
//**"****!****"****!****"****!****"****!****"****!****"****!****"****!****"****|
-
//**"****!****"****!****"****!****"****!****"****!****"****!****"****!****"****|
// The routine gen_DM_source calculates the source functions of the products of the
! // dark matter (DM) particle annihilation [cm^-3 s^-1 MeV^-1].
// The routine can be used to calculate source function of positrons, electrons,
// and antiprotons.
! // Use gen_DM_emiss to define gamma-ray emissivity (cm^-3 s^-1 MeV^-1)
! // in terms (dn/dEdt *c/4pi), where n is the number density, c is speed of light.
// The user must use the parameters DM_double0-9 and DM_int0-9 (galdef-file) to
// specify the Galactic DM profile, branching, decay channels, and spectra (see
// the template below). The DM profile is defined in the DM_profile routine.
--- 3,15 ----
// * gen_DM_source.cc * galprop package * 9/09/2005
//**"****!****"****!****"****!****"****!****"****!****"****!****"****!****"****|
//**"****!****"****!****"****!****"****!****"****!****"****!****"****!****"****|
// The routine gen_DM_source calculates the source functions of the products of the
! // dark matter (DM) particle annihilation [c/(4\pi) cm^-3 s^-1 MeV^-1].
// The routine can be used to calculate source function of positrons, electrons,
// and antiprotons.
! // Use gen_DM_emiss to define gamma-ray emissivity (cm^-3 s^-1 MeV^-1 sr^-1)
! // in terms (dn/dEdt *1/4pi), where n is the number density, c is speed of light (AE20131226 - c is removed, sr^-1 is added above - suggested typos).
// The user must use the parameters DM_double0-9 and DM_int0-9 (galdef-file) to
// specify the Galactic DM profile, branching, decay channels, and spectra (see
// the template below). The DM profile is defined in the DM_profile routine.
***************
*** 19,24 ****
--- 18,28 ----
//
// See example in Moskalenko I.V., Strong A.W. 1999, Phys. Rev. D 60, 063003
// and realization below.
+
+ // Modified, improved and updated by Andrey Egorov - 11/29/2013-... .
+
+ //Attention! - DM_profile_av function below bears in fact DM density squared average.
+
//=="====!===="====!===="====!===="====!===="====!===="====!===="====!===="====!
using namespace std;
#include"galprop_classes.h"
***************
*** 28,121 ****
#include <string.h>
//extern "C" void RHO_DARKSUSY_F77(double*,double*,double*,double*); //IMOS20060901
//**"****!****"****!****"****!****"****!****"****!****"****!****"****!****"****|
int Galprop::gen_DM_source(Particle &particle)
{
! cout<<"gen_DM_source"<<endl;
! cout<<"generating "<<particle.name<<" source function for n_spatial_dimensions="
! <<gcr[0].n_spatial_dimensions<<endl;
!
! double DMwidth,DMbranching, // annihilation product distribution
! DMsecondary_spectrum, // spectrum of secondaries from DM annihilation
! DME0, // delta function energy used for Green's function
! DMmass =galdef.DM_double2, // DM particle mass
! DMcs_v =galdef.DM_double9, // DM <cross_sec*V> -thermally overaged, cm3 s-1
! dzz=0.01; // kpc, gas averaging step
! int stat=0;
! // define the spectra of annihilation products: positrons, electrons, antiprotons
! if(strcmp(particle.name,"DM_positrons")==0)
! {
! DMwidth =galdef.DM_double3;
! DMbranching =galdef.DM_double4;
! }
! if(strcmp(particle.name,"DM_electrons")==0)
! {
! DMwidth =galdef.DM_double5;
! DMbranching =galdef.DM_double6;
! }
- if(strcmp(particle.name,"DM_antiprotons")==0)
- {
- DMwidth =galdef.DM_double7;
- DMbranching =galdef.DM_double8;
- }
// assign the source function (2D)
if(galaxy.n_spatial_dimensions==2)
{
for(int ir=0; ir<gcr[0].n_rgrid; ir++)
{
for(int iz=0; iz<gcr[0].n_zgrid; iz++)
{
for(int ip=0; ip<particle.n_pgrid; ip++)
{
- // test of electron propagation vs analytical calculations IMOS20061030
- // to run test, assign galdef.DM_int0=99, other parameters:
- // galdef.DM_double6 - the half thickness of the disk source distribution (e.g. 0.1 kpc), the source
- // distribution is uniform within the disk; normalization =1 at the normalization energy
- // galdef.DM_double7 - the photon field energy density (e.g. 1 eV/cc)
- // galdef.DM_double8 - the normalization energy of the electron spectrum (e.g. 10^3 MeV)
- // galdef.DM_double9 - the injection spectral index of electrons (e.g. 2.4)
- if(abs(galdef.DM_int0)==99 && particle.A==0)
- {
- if(strcmp(particle.name,"DM_electrons")==0) //numerical solution "DM_electrons"
- particle.secondary_source_function.d2[ir][iz].s[ip]=
- (galdef.DM_double6 <= fabs(galaxy.z[iz])) ? 0.:
- C/4./Pi*pow(particle.Ekin[ip]/galdef.DM_double8,-galdef.DM_double9);
- if(strcmp(particle.name,"DM_positrons")==0) //analytical solution "DM_positrons"
- particle.secondary_source_function.d2[ir][iz].s[ip]=0.;
- continue;
- }
- // end of the test area
if(galdef.DM_int1==9) // Green's function to work with DarkSUSY IMOS20060901
{
if(DME0<particle.Ekin[ip] || DME0/DMwidth>particle.Ekin[ip]) continue;
particle.secondary_source_function.d2[ir][iz].s[ip]
! +=pow(DM_profile_av(galaxy.r[ir], galaxy.z[iz], galaxy.dr, galaxy.dz, dzz),2)
*DMsecondary_spectrum*DMbranching/4./Pi*C;
continue;
! }
if(particle.Etot[ip]*1.e-3<=DMmass)
! particle.secondary_source_function.d2[ir][iz].s[ip]+= DMcs_v*
! pow(DM_profile_av(galaxy.r[ir], galaxy.z[iz], galaxy.dr, galaxy.dz, dzz)/DMmass,2)
! *C/4./Pi*DMbranching*exp(-pow((DMmass-particle.Etot[ip]*1.e-3)/DMwidth,2))/DMmass*1.e-3;
} // ip
} // iz
} // ir
} // particle.n_spatial_dimensions==2
// assign the source function (3D)
if(galaxy.n_spatial_dimensions==3)
{
! for(int ix=0; ix<gcr[0].n_xgrid; ix++)
{
for(int iy=0; iy<gcr[0].n_ygrid; iy++)
{
--- 32,247 ----
#include <string.h>
+ #include <ErrorLogger.h>
+ #include<sstream>
+
//extern "C" void RHO_DARKSUSY_F77(double*,double*,double*,double*); //IMOS20060901
//**"****!****"****!****"****!****"****!****"****!****"****!****"****!****"****|
int Galprop::gen_DM_source(Particle &particle)
{
! cout<<"gen_DM_source"<<endl;
! cout<<"generating "<<particle.name<<" source function for n_spatial_dimensions="<<gcr[0].n_spatial_dimensions<<endl;
! const double DMmass=galdef.DM_double2, // DM particle mass, GeV
! DMcs_v=galdef.DM_double9; // DM <cross_sec*V> -thermally averaged, cm3 s-1
! double DME0,DMwidth,DMbranching,DMsecondary_spectrum; // obsolete - needed for DarkSUSY
! int stat=0, iwm=0, SD_key=galdef.DM_int4, channel_key=galdef.DM_int2;
!
! FILE *fDM; // file with annihilation yields data for p* and ee*
! const long NsDMy=55242, NDMm=62, NsDMym=891; // for operation with yields data
! long jDMyw=0;
! double DMy[NsDMy], DMym[NsDMym];
! const double mt[NDMm] = {5.,6.,8.,10.,15.,20.,25.,30.,40.,50.,60.,70.,80.,90.,100.,110.,120.,130.,140.,150.,160.,180.,200.,220.,240.,260.,280.,300.,330.,360.,
! 400.,450.,500.,550.,600.,650.,700.,750.,800.,900.,1000.,1100.,1200.,1300.,1500.,1700.,2000.,2500.,3000.,4000.,5000.,6000.,7000.,
! 8000.,9000.,10000.,12000.,15000.,20000.,30000.,50000.,100000.}; // masses with tabulated yields
! const std::string DMDirectory = configure.fFITSDataDirectory+"DM/";
! std::string filename = DMDirectory;
! const char *str;
!
! if(strcmp(particle.name,"DM_antiprotons")==0)
! {
! SD_key=0;
! switch(channel_key)
! {
! case 1: filename += "DM-e-p.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // e^+e^- channel
! case 2: filename += "DM-mu-p.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // \mu^+\mu^- channel
! case 3: filename += "DM-tau-p.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // \tau^+\tau^- channel
! case 4: filename += "DM-q-p.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // qq* channel
! case 5: filename += "DM-c-p.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // cc* channel
! case 6: filename += "DM-b-p.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // bb* channel
! case 7: filename += "DM-t-p.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // tt* channel
! case 8: filename += "DM-g-p.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // \gamma\gamma channel
! case 9: filename += "DM-gl-p.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // gg channel
! case 10: filename += "DM-W-p.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // W^+W^- channel
! case 11: filename += "DM-Z-p.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // ZZ channel
! case 12: filename += "DM-h-p.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // hh channel
! }
! }
! if(strcmp(particle.name,"DM_electrons")==0 || strcmp(particle.name,"DM_positrons")==0)
! {
! switch(channel_key)
! {
! case 1: filename += "DM-e-e.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // e^+e^- channel
! case 2: filename += "DM-mu-e.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // \mu^+\mu^- channel
! case 3: filename += "DM-tau-e.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // \tau^+\tau^- channel
! case 4: filename += "DM-q-e.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // qq* channel
! case 5: filename += "DM-c-e.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // cc* channel
! case 6: filename += "DM-b-e.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // bb* channel
! case 7: filename += "DM-t-e.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // tt* channel
! case 8: filename += "DM-g-e.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // \gamma\gamma channel
! case 9: filename += "DM-gl-e.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // gg channel
! case 10: filename += "DM-W-e.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // W^+W^- channel
! case 11: filename += "DM-Z-e.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // ZZ channel
! case 12: filename += "DM-h-e.dat";
! str = filename.c_str();
! fDM=fopen(str,"r");
! break; // hh channel
! }
! }
! fseek(fDM, 0, SEEK_SET);
! for (long jDMy=0; jDMy<NsDMy; jDMy++)
! {
! fscanf(fDM, "%lf", &DMy[jDMy]);
! }
! fclose(fDM);
+ for(int ia=0; ia<NDMm; ia++)
+ {
+ if(DMmass==mt[ia])
+ {iwm=ia+1; // yields preparation from mass analysis
+ break;
+ }
+ }
+ if(iwm>=1)
+ {
+ for(int ib=0; ib<NsDMym; ib++) DMym[ib]=DMy[(iwm-1)*NsDMym+ib];
+ }
+ else
+ {
+ while (DMmass>mt[iwm]) iwm++;
+ for(int ic=0;ic<NsDMym;ic++) DMym[ic]=DMy[(iwm-1)*NsDMym+ic]+((DMy[iwm*NsDMym+ic]-DMy[(iwm-1)*NsDMym+ic])*(DMmass-mt[iwm-1]))/(mt[iwm]-mt[iwm-1]);
+ }
+
// assign the source function (2D)
if(galaxy.n_spatial_dimensions==2)
{
+ #pragma omp parallel for schedule(dynamic) default(shared) private(jDMyw)
for(int ir=0; ir<gcr[0].n_rgrid; ir++)
{
for(int iz=0; iz<gcr[0].n_zgrid; iz++)
{
for(int ip=0; ip<particle.n_pgrid; ip++)
{
if(galdef.DM_int1==9) // Green's function to work with DarkSUSY IMOS20060901
{
if(DME0<particle.Ekin[ip] || DME0/DMwidth>particle.Ekin[ip]) continue;
particle.secondary_source_function.d2[ir][iz].s[ip]
! +=DM_profile_av(galaxy.r[ir], galaxy.z[iz], galaxy.dr, galaxy.dz)
*DMsecondary_spectrum*DMbranching/4./Pi*C;
continue;
! } // end of DarkSUSY area
if(particle.Etot[ip]*1.e-3<=DMmass)
! {
! if(particle.Ekin[ip]*1.e-3<pow(10,-8.9)*DMmass)
! particle.secondary_source_function.d2[ir][iz].s[ip]+=0;
! else
! {
! jDMyw=lround(100.*log10(particle.Ekin[ip]/(DMmass*1000.)))+NsDMym-1;
! particle.secondary_source_function.d2[ir][iz].s[ip]+=(1.+SD_key)*(C/(4.*Pi))*0.5*DMcs_v*
! DM_profile_av(galaxy.r[ir], galaxy.z[iz], galaxy.dr, galaxy.dz)*pow(DMmass,-2.)*DM_subs_boost(galaxy.r[ir], 0., galaxy.z[iz])*DMym[jDMyw]/(log(10.)*particle.Ekin[ip]);
! } //else
! } // if
} // ip
} // iz
} // ir
+ if(galdef.verbose>=3)
+ for(int ir=0; ir<gcr[0].n_rgrid; ir++) {
+ for(int iz=0; iz<gcr[0].n_zgrid; iz++) {
+ for(int ip=0; ip<particle.n_pgrid; ip++) {
+ cout<<galaxy.r[ir]<<" r "<<galaxy.z[iz]<<" z "<<particle.Ekin[ip]<<" Ekin "<<DM_profile_av(galaxy.r[ir], galaxy.z[iz], galaxy.dr, galaxy.dz)<<" rho_{DM}_sq_av "<<DM_subs_boost(galaxy.r[ir], 0., galaxy.z[iz])<<" B(r) "<<particle.secondary_source_function.d2[ir][iz].s[ip]<<endl; }}} //test printout
} // particle.n_spatial_dimensions==2
// assign the source function (3D)
if(galaxy.n_spatial_dimensions==3)
{
! #pragma omp parallel for schedule(dynamic) default(shared) private(jDMyw)
! for(int ix=0; ix<gcr[0].n_xgrid; ix++)
{
for(int iy=0; iy<gcr[0].n_ygrid; iy++)
{
***************
*** 127,147 ****
{
if(DME0<particle.Ekin[ip] || DME0/DMwidth>particle.Ekin[ip]) continue;
particle.secondary_source_function.d3[ix][iy][iz].s[ip]
! +=pow(DM_profile_av(galaxy.r[ix], galaxy.r[iy], galaxy.z[iz], galaxy.dx, galaxy.dy, galaxy.dz, dzz),2)
*DMsecondary_spectrum*DMbranching/4./Pi*C;
continue;
! }
if(particle.Etot[ip]*1.e-3<=DMmass)
! particle.secondary_source_function.d3[ix][iy][iz].s[ip]+= DMcs_v*
! pow(DM_profile_av(galaxy.x[ix], galaxy.y[ix], galaxy.z[iz], galaxy.dx, galaxy.dy, galaxy.dz, dzz)/DMmass,2)
! *C/4./Pi*DMbranching*exp(-pow((DMmass-particle.Etot[ip]*1.e-3)/DMwidth,2))/DMmass*1.e-3;
} //ip
} // iz
} // iy
! } // ix
} // particle.n_spatial_dimensions==3
- // test printout
if(galdef.verbose>=2)
{
--- 253,286 ----
{
if(DME0<particle.Ekin[ip] || DME0/DMwidth>particle.Ekin[ip]) continue;
particle.secondary_source_function.d3[ix][iy][iz].s[ip]
! +=DM_profile_av(galaxy.r[ix], galaxy.r[iy], galaxy.z[iz], galaxy.dx, galaxy.dy, galaxy.dz)
*DMsecondary_spectrum*DMbranching/4./Pi*C;
continue;
! } // end of DarkSUSY area
!
if(particle.Etot[ip]*1.e-3<=DMmass)
! {
! if(particle.Ekin[ip]*1.e-3<pow(10,-8.9)*DMmass)
! particle.secondary_source_function.d3[ix][iy][iz].s[ip]+=0;
! else
! {
! jDMyw=lround(100.*log10(particle.Ekin[ip]/(DMmass*1000.)))+NsDMym-1;
! particle.secondary_source_function.d3[ix][iy][iz].s[ip]+=(1.+SD_key)*(C/(4.*Pi))*0.5*DMcs_v*
! DM_profile_av(galaxy.x[ix], galaxy.y[iy], galaxy.z[iz], galaxy.dx, galaxy.dy, galaxy.dz)*pow(DMmass,-2.)*DM_subs_boost(galaxy.x[ix], galaxy.y[iy], galaxy.z[iz])*DMym[jDMyw]/(log(10.)*particle.Ekin[ip]);
! } //else
! } // if
} //ip
} // iz
} // iy
! } // ix
! if(galdef.verbose>=3)
! for(int ix=0; ix<gcr[0].n_xgrid; ix++) {
! for(int iy=0; iy<gcr[0].n_ygrid; iy++) {
! for(int iz=0; iz<gcr[0].n_zgrid; iz++) {
! for(int ip=0; ip<particle.n_pgrid; ip++) {
! cout<<galaxy.x[ix]<<" x "<<galaxy.y[iy]<<" y "<<galaxy.z[iz]<<" z "<<particle.Ekin[ip]<<" Ekin "<<DM_profile_av(galaxy.x[ix], galaxy.y[iy], galaxy.z[iz], galaxy.dx, galaxy.dy, galaxy.dz)<<" rho_{DM}_sq_av "<<DM_subs_boost(galaxy.x[ix], galaxy.y[iy], galaxy.z[iz])<<" B(r) "<<particle.secondary_source_function.d3[ix][iy][iz].s[ip]<<endl; }}}} //test printout
} // particle.n_spatial_dimensions==3
if(galdef.verbose>=2)
{
***************
*** 157,220 ****
int Galprop::gen_DM_emiss()
{
cout<<"gen_DM_emiss"<<endl;
double
! DMmass =galdef.DM_double2, // DM particle mass
! DMcs_v =galdef.DM_double9, // DM <cross_sec*V> -thermally overaged, cm3 s-1
! DMbranching =0.1,
! dzz=0.01; // kpc, gas averaging step
! int stat=0;
galaxy.DM_emiss=0.;
// define the spectra of annihilation products: gammas
if(galdef.n_spatial_dimensions==2)
! {
! cout<<"generating DM emissivity for n_spatial_dimensions="<<galdef.n_spatial_dimensions<<endl;
! for(int ir=0; ir<gcr[0].n_rgrid; ir++)
{
! for(int iz=0; iz<gcr[0].n_zgrid; iz++)
{
for(int iEgamma=0; iEgamma<galaxy.n_E_gammagrid; iEgamma++)
{
! if(galaxy.E_gamma[iEgamma]*1.e-3>DMmass)
! {
! galaxy.DM_emiss.d2[ir][iz].s[iEgamma]=0;
! continue;
! }
! galaxy.DM_emiss.d2[ir][iz].s[iEgamma]= DMcs_v *DMbranching/(4.*Pi)// sr^-1 IMOS20060420
! *pow(DM_profile_av(galaxy.r[ir], galaxy.z[iz], galaxy.dr, galaxy.dz, dzz)/DMmass,2)
! /galaxy.E_gamma[iEgamma];
! }
! }
! }
! }
if(galdef.n_spatial_dimensions==3)
{
! cout<<"generating DM emissivity for n_spatial_dimensions="<<galdef.n_spatial_dimensions<<endl;
! for(int ix=0; ix<gcr[0].n_rgrid; ix++)
{
! for(int iy=0; iy<gcr[0].n_rgrid; iy++)
{
! for(int iz=0; iz<gcr[0].n_zgrid; iz++)
{
for(int iEgamma=0; iEgamma<galaxy.n_E_gammagrid; iEgamma++)
{
! if(galaxy.E_gamma[iEgamma]*1.e-3>DMmass)
! {
! galaxy.DM_emiss.d3[ix][iy][iz].s[iEgamma]=0;
! continue;
! }
! galaxy.DM_emiss.d3[ix][iy][iz].s[iEgamma]= DMcs_v *DMbranching/(4.*Pi) // sr^-1 IMOS20060420
! *pow(DM_profile_av(galaxy.x[ix], galaxy.y[ix], galaxy.z[iz], galaxy.dx, galaxy.dy, galaxy.dz, dzz)/DMmass,2)
! /galaxy.E_gamma[iEgamma];
! }
! }
! }
! }
! }
cout<<" <<<< gen_DM_emiss"<<endl;
! return(stat);
}
//**"****!****"****!****"****!****"****!****"****!****"****!****"****!****"****|
--- 296,467 ----
int Galprop::gen_DM_emiss()
{
cout<<"gen_DM_emiss"<<endl;
+ cout<<"generating DM prompt gamma emissivity for n_spatial_dimensions="<<galdef.n_spatial_dimensions<<endl;
+
double
! DMmass =galdef.DM_double2, // DM particle mass, GeV
! DMcs_v =galdef.DM_double9; // DM <cross_sec*V> -thermally overaged, cm3 s-1
! int stat=0, iwm=0, channel_key=galdef.DM_int2; // last one sets annihilation channel
!
! FILE *fDMg; //file with annihilation yields data for gammas
! const long NsDMy=55242, NDMm=62, NsDMym=891; // for operation with yields data
! long jDMyw=0;
! double DMy[NsDMy], DMym[NsDMym];
! const double mt[NDMm]={5.,6.,8.,10.,15.,20.,25.,30.,40.,50.,60.,70.,80.,90.,100.,110.,120.,130.,140.,150.,160.,180.,200.,220.,240.,260.,280.,300.,330.,360.,
! 400.,450.,500.,550.,600.,650.,700.,750.,800.,900.,1000.,1100.,1200.,1300.,1500.,1700.,2000.,2500.,3000.,4000.,5000.,6000.,7000.,
! 8000.,9000.,10000.,12000.,15000.,20000.,30000.,50000.,100000.}; // masses with tabulated yields
! const std::string DMDirectory = configure.fFITSDataDirectory+"DM/";
! std::string filename = DMDirectory;
! const char *str;
!
!
! switch(channel_key)
! {
! case 1: filename += "DM-e-g.dat";
! str = filename.c_str();
! fDMg=fopen(str,"r");
! break; // e^+e^- channel
! case 2: filename += "DM-mu-g.dat";
! str = filename.c_str();
! fDMg=fopen(str,"r");
! break; // \mu^+\mu^- channel
! case 3: filename += "DM-tau-g.dat";
! str = filename.c_str();
! fDMg=fopen(str,"r");
! break; // \tau^+\tau^- channel
! case 4: filename += "DM-q-g.dat";
! str = filename.c_str();
! fDMg=fopen(str,"r");
! break; // qq* channel
! case 5: filename += "DM-c-g.dat";
! str = filename.c_str();
! fDMg=fopen(str,"r");
! break; // cc* channel
! case 6: filename += "DM-b-g.dat";
! str = filename.c_str();
! fDMg=fopen(str,"r");
! break; // bb* channel
! case 7: filename += "DM-t-g.dat";
! str = filename.c_str();
! fDMg=fopen(str,"r");
! break; // tt* channel
! case 8: filename += "DM-g-g.dat";
! str = filename.c_str();
! fDMg=fopen(str,"r");
! break; // \gamma\gamma channel
! case 9: filename += "DM-gl-g.dat";
! str = filename.c_str();
! fDMg=fopen(str,"r");
! break; // gg channel
! case 10: filename += "DM-W-g.dat";
! str = filename.c_str();
! fDMg=fopen(str,"r");
! break; // W^+W^- channel
! case 11: filename += "DM-Z-g.dat";
! str = filename.c_str();
! fDMg=fopen(str,"r");
! break; // ZZ channel
! case 12: filename += "DM-h-g.dat";
! str = filename.c_str();
! fDMg=fopen(str,"r");
! break; // hh channel
! }
!
! fseek(fDMg, 0, SEEK_SET);
! for (long jDMy=0; jDMy<NsDMy; jDMy++)
! {
! fscanf(fDMg, "%lf", &DMy[jDMy]);
! }
! fclose(fDMg);
!
!
! for(int ia=0; ia<NDMm; ia++)
! {
! if(DMmass==mt[ia])
! {iwm=ia+1; // yields preparation from mass analysis
! break;
! }
! }
! if(iwm>=1)
! {
! for(int ib=0; ib<NsDMym; ib++) DMym[ib]=DMy[(iwm-1)*NsDMym+ib];
! }
! else
! {
! while (DMmass>mt[iwm]) iwm++;
! for(int ic=0;ic<NsDMym;ic++) DMym[ic]=DMy[(iwm-1)*NsDMym+ic]+((DMy[iwm*NsDMym+ic]-DMy[(iwm-1)*NsDMym+ic])*(DMmass-mt[iwm-1]))/(mt[iwm]-mt[iwm-1]);
! }
galaxy.DM_emiss=0.;
// define the spectra of annihilation products: gammas
if(galdef.n_spatial_dimensions==2)
! {
! #pragma omp parallel for schedule(dynamic) default(shared) private(jDMyw)
! for(int ir=0; ir<galaxy.n_rgrid; ir++)
{
! for(int iz=0; iz<galaxy.n_zgrid; iz++)
{
for(int iEgamma=0; iEgamma<galaxy.n_E_gammagrid; iEgamma++)
{
! if(galaxy.E_gamma[iEgamma]*1.e-3<=DMmass)
! {
! if(galaxy.E_gamma[iEgamma]*1.e-3<pow(10,-8.9)*DMmass)
! galaxy.DM_emiss.d2[ir][iz].s[iEgamma]+=0;
! else
! {
! jDMyw=lround(100.*log10(galaxy.E_gamma[iEgamma]/(DMmass*1000.)))+NsDMym-1;
! galaxy.DM_emiss.d2[ir][iz].s[iEgamma]+=(1/(4.*Pi))*0.5*DMcs_v*
! DM_profile_av(galaxy.r[ir], galaxy.z[iz], galaxy.dr, galaxy.dz)*pow(DMmass,-2.)*DM_subs_boost(galaxy.r[ir], 0., galaxy.z[iz])*DMym[jDMyw]/(log(10.)*galaxy.E_gamma[iEgamma]);
! } // else
! } // if
! } // iEgamma
! } // iz
! } // ir
! if(galdef.verbose>=3)
! for(int ir=0; ir<galaxy.n_rgrid; ir++) {
! for(int iz=0; iz<galaxy.n_zgrid; iz++) {
! for(int iEgamma=0; iEgamma<galaxy.n_E_gammagrid; iEgamma++) {
! cout<<galaxy.r[ir]<<" r "<<galaxy.z[iz]<<" z "<<galaxy.E_gamma[iEgamma]<<" Egamma "<<DM_profile_av(galaxy.r[ir], galaxy.z[iz], galaxy.dr, galaxy.dz)<<" rho_{DM}_sq_av "<<DM_subs_boost(galaxy.r[ir], 0., galaxy.z[iz])<<" B(r) "<<galaxy.DM_emiss.d2[ir][iz].s[iEgamma]<<endl; }}} //test printout
! } // if n_sp._dim.
!
if(galdef.n_spatial_dimensions==3)
{
! #pragma omp parallel for schedule(dynamic) default(shared) private(jDMyw)
! for(int ix=0; ix<galaxy.n_xgrid; ix++)
{
! for(int iy=0; iy<galaxy.n_ygrid; iy++)
{
! for(int iz=0; iz<galaxy.n_zgrid; iz++)
{
for(int iEgamma=0; iEgamma<galaxy.n_E_gammagrid; iEgamma++)
{
! if(galaxy.E_gamma[iEgamma]*1.e-3<=DMmass)
! {
! if(galaxy.E_gamma[iEgamma]*1.e-3<pow(10,-8.9)*DMmass)
! galaxy.DM_emiss.d3[ix][iy][iz].s[iEgamma]+=0;
! else
! {
! jDMyw=lround(100.*log10(galaxy.E_gamma[iEgamma]/(DMmass*1000.)))+NsDMym-1;
! galaxy.DM_emiss.d3[ix][iy][iz].s[iEgamma]+=(1/(4.*Pi))*0.5*DMcs_v*
! DM_profile_av(galaxy.x[ix], galaxy.y[iy], galaxy.z[iz], galaxy.dx, galaxy.dy, galaxy.dz)*pow(DMmass,-2.)*DM_subs_boost(galaxy.x[ix], galaxy.y[iy], galaxy.z[iz])*DMym[jDMyw]/(log(10.)*galaxy.E_gamma[iEgamma]);
! } // else
! } // if
! } // iEgamma
! } // iz
! } // iy
! } // ix
! if(galdef.verbose>=3)
! for(int ix=0; ix<galaxy.n_xgrid; ix++) {
! for(int iy=0; iy<galaxy.n_ygrid; iy++) {
! for(int iz=0; iz<galaxy.n_zgrid; iz++) {
! for(int iEgamma=0; iEgamma<galaxy.n_E_gammagrid; iEgamma++) {
! cout<<galaxy.x[ix]<<" x "<<galaxy.y[iy]<<" y "<<galaxy.z[iz]<<" z "<<galaxy.E_gamma[iEgamma]<<" Egamma "<<DM_profile_av(galaxy.x[ix], galaxy.y[iy], galaxy.z[iz], galaxy.dx, galaxy.dy, galaxy.dz)<<" rho_{DM}_sq_av "<<DM_subs_boost(galaxy.x[ix], galaxy.y[iy], galaxy.z[iz])<<" B(r) "<<galaxy.DM_emiss.d3[ix][iy][iz].s[iEgamma]<<endl; }}}} //test printout
! } // if n_sp._dim.
cout<<" <<<< gen_DM_emiss"<<endl;
!
! return stat;
}
//**"****!****"****!****"****!****"****!****"****!****"****!****"****!****"****|
***************
*** 222,294 ****
double Galprop::DM_profile(double Xkpc, double Ykpc, double Zkpc)
{
double R=sqrt(Xkpc*Xkpc+Ykpc*Ykpc+Zkpc*Zkpc),
! Rsun =8.5, //kpc, galactocentric distance of the solar system
! Rc =galdef.DM_double0, //core radius
! rho0 =galdef.DM_double1; //local DM mass density
int profile_key =galdef.DM_int0; //profile type
switch(profile_key)
{
! case 0: //NFW profile
! return(rho0*Rc/R*pow(1.+R/Rc,-2));
! case 1: //isothermal profile
! return(rho0*(pow(Rc,2)+pow(Rsun,2))/(pow(Rc,2)+pow(R,2)));
! case 2: //Evans profile
! return(rho0*pow(pow(Rc,2)+pow(Rsun,2),2)/(3.*pow(Rc,2)+pow(Rsun,2))
! *(3.*pow(Rc,2)+pow(R,2))/pow(pow(Rc,2)+pow(R,2),2));
! case 3: //alternative profile
! return(rho0*pow(Rc+Rsun,2)/pow(Rc+R,2));
case 9: //DarkSUSY profile (use only if the DarkSUSY and GALPROP combined) IMOS20060901
RHO_DARKSUSY_F77(&Xkpc,&Ykpc,&Zkpc,&rho0);
-
if(rho0<0.)
{
cout<<"gen_DM_source: rho_darksusy() function is not defined"<<endl;
exit(0);
}
return(rho0);
! default:
! return(rho0);
}
}
!
- //**.****|****.****|****.****|****.****|****.****|****.****|****.****|****.****|
! double Galprop::DM_profile_av(double r,double z,double dr,double dz,double dzz)
{
! double DM_profile_av_=0.0;
! int nuse=0;
!
! for (double zz=z-dz/2.; zz<=z+dz/2.; zz+=dzz)
! for (double rr=r-dr/2.; rr<=r+dr/2.; rr+=dr/10.)
! {
! if (rr<0.) continue;
! DM_profile_av_+=DM_profile(rr,0,zz);
! nuse++;
! }
! return (DM_profile_av_/nuse);
! }
//**.****|****.****|****.****|****.****|****.****|****.****|****.****|****.****|
! double Galprop::DM_profile_av(double x,double y,double z,double dx,double dy,double dz,double dzz)
! {
! double DM_profile_av_=0.0;
! int nuse=0;
!
! for (double zz=z-dz/2.; zz<=z+dz/2.; zz+=dzz)
! for (double xx=x-dx/2.; xx<=x+dx/2.; xx+=dx/10.)
! for (double yy=y-dy/2.; yy<=y+dy/2.; yy+=dy/10.)
! {
! DM_profile_av_+=DM_profile(xx,yy,zz);
! nuse++;