https://github.com/a-e-egorov/GALPROP_DM
Tip revision: 3e42307006508424bc7beadd0708f6c240029339 authored by Andrei Egorov on 02 February 2024, 16:17:56 UTC
Update DM-v57_w_M31.patch
Update DM-v57_w_M31.patch
Tip revision: 3e42307
galdef_54_testDM
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Title = example of DM run for v54
# DARK MATTER =====================================================
DM_double2 = 2000 DM particle mass, GeV - must be in the range [5..100000] AND greater than the rest mass of the primary products (DM_int2)
DM_int2 = 9 DM annihilation channel: 1=e^+e^-, 2=\mu^+\mu^-,3=\tau^+\tau^-,4=qq*, 5=cc*, 6=bb*, 7=tt*, 8=\gamma\gamma, 9=gg, 10=W^+W^-, 11=ZZ, 12=hh
DM_double6 = 1.2 \gamma parameter for the generalized NFW profile (1.0 gives the canonical NFW)
DM_double1 = 0.17 scale density of the DM profile, GeV cm^-3
DM_double0 = 23 scale radius of the DM density profile, kpc
DM_double8 = 0.05 truncation radius for the NFW profile, below which the DM density stays constant, kpc. It's strictly NOT recommended to set it lower than ~0.01 kpc, since the gNFW profile steeply
blows up near the central point, which may lead to unphysical source term value in the central cell; DM numerical simulations anyway don't resolve anything below such a limit.
DM_double7 = 0.17 \alpha parameter for the Einasto DM density profile
DM_int0 = 0 DM density profile (according to PPPC review): 0=generalized NFW, 1=Isothermal, 2=Einasto, 3=Burkert, 9=DarkSUSY
DM_int3 = 1 Substructure presense: 0=no, 1=based on Kamionkowski et al., Phys.Rev.D 81, 043532 (2010).
DM_int4 = 1 1=doubles lepton source function (0=no) in order to save comp. time by propagating only one specie; if turned on, requires either one of DM_positrons or DM_electrons to be 0; should be a good approximation
DM_positrons = 1 1=compute DM positrons
DM_electrons = 0 1=compute DM electrons
DM_antiprotons = 1 1=compute DM antiprotons
DM_gammas = 1 1=compute DM gammas, 2=compute DM gammas ONLY AND NOTHING else (doesn't allow other switches)
gamma_rays = 1 1=compute gamma rays, 2=compute HI,H2 skymaps separately
pi0_decay = 0 1= old formalism 2=Blattnig et al. 3=Kamae et al.
IC_isotropic = 0 1,2= compute isotropic IC: 1=compute full, 2=store skymap components
IC_anisotropic = 0 1,2,3= compute anisotropic IC: 1=full, 2=approx., 3=isotropic
bremss = 0 1=compute bremsstrahlung
synchrotron = 2 2,3=compute synchrotron using B_field_name and B_field_parameters. 2=total only, 3= all Stokes
free_free_absorption = 0 0=no absorption 1 free-free absorption of synchrotron 2=replace synch total with free-free
DM_double9 = 3.0e-26 DM thermally averaged annihilation cross section, cm^3 s^-1
DM_int9 = 3 0=fixed increment synchrotron frequency grid, >0=# of arbitrary frequencies (DM_double3)
DM_double3 = 0.1e9,1.0e9,30.0e9 #120.0e6,240.0e6,325.0e6,610.0e6,1.4e9,2.3e9,4.8e9,12.0e9,23.0e9,28.0e9 list of arbitrary synchrotron frequencies (Hz)
DM_int8 = 1 not used
DM_int5 = 1
DM_int6 = 1
DM_int7 = 1
DM_int1 = 1 9=DarkSUSY DM source
DM_double4 = 50.
DM_double5 = 40.
# MAGNETIC FIELD ================================================
B_field_name = galprop_original 3D models:han .... galprop_original: exponential model as in original (parameters Bo, rscale, zscale)
n_B_field_parameters = 10 number of B-field parameters (number is free, depends on model)
# B0 R- z-scale
B_field_parameters = 6.0e-6, 4.0, 2.7, 0.0,0.0,0.0,0.0,0.0,0.0,0.0 parameters for 3D models galprop_original
# PROPAGATION ===================================================
z_min = -5.4 min z, kpc
z_max = +5.4 max z, kpc
D0_xx = 5.4e28 diffusion coefficient in x at reference rigidity in cm^2/s
D_g_1 = 0.31 diffusion coefficient index below reference rigidity
D_g_2 = 0.31 diffusion coefficient index above reference rigidity
diff_reacc = 1 0=no reacc.; 1,2=incl.diff.reacc.; -1==beta^3 Dxx; 11=Kolmogorov+damping; 12=Kraichnan+damping
v_Alfven = 38.0 Alfven speed in km s-1
D_rigid_br = 1.0e3 reference rigidity for diffusion coefficient in MV
damping_p0 = 1.e6 MV -some rigidity (where CR density is low)
damping_const_G = 0.02 a const derived from fitting B/C
damping_max_path_L = 3.e21 Lmax~1 kpc, max free path
Diffusion_aniso = 0 0=isotropic 1=anisotropic diffusion
D0_zz = 5.80e27 diffusion coefficient in z at reference rigidity, for Diffusion_aniso=1
convection = 0 1,2,3 =include convection for various models
v0_conv = 0. km s-1 convection=1: v_conv=v0_conv+dvdz_conv*dz
dvdz_conv = 7. km s-1 kpc-1 convection=1: v_conv=v0_conv+dvdz_conv*dz
z0_conv = 3.0 convection=2: v=0 for |z|<z0 ; v=v0_conv+dvdz_conv*(z-z0) z>z0, similar for z<-z0; convection=3: tanh function
# ================================================================
n_spatial_dimensions = 2
dz = 0.3 delta z, kpc
x_min = -15.0 min x
x_max = +15.0 max x
dx = 1.0 delta x
y_min = -15.0 min y
y_max = +15.0 max y
dy = 1.0 delta y
r_min = 0.0 min r
r_max = 20.0 max r
dr = 1.0 delta r
p_min = 1000 min momentum (MV)
p_max = 4000 max momentum
p_factor = 1.50 momentum factor
Ekin_min = 2.0 min kinetic energy per nucleon (MeV); not only the region of interest must be covered, but also the region of production
Ekin_max = 4.0e8 max kinetic energy per nucleon (MeV); not only the region of interest must be covered, but also the region of production
Ekin_factor = 2.0 kinetic energy per nucleon grid factor
p_Ekin_grid = Ekin p||Ekin alignment
E_gamma_min = 1. min gamma-ray energy (MeV)
E_gamma_max = 1000. max gamma-ray energy (MeV)
E_gamma_factor = 3.0 gamma-ray energy factor
integration_mode = 0 integr.over part.spec.: =1-old E*logE; =0-PL analyt.
nu_synch_min = 28.0e9 min synchrotron frequency (Hz)
nu_synch_max = 29.0e9 max synchrotron frequency (Hz)
nu_synch_factor = 1.5 synchrotron frequency factor
long_min = 0 gamma-ray intensity skymap longitude minimum (deg); 0 -automatic binning required to get correct results!
long_max = 360 gamma-ray intensity skymap longitude maximum (deg); 360 -automatic binning
lat_min = -90 gamma-ray intensity skymap latitude minimum (deg); -90 -automatic binning
lat_max = +90 gamma-ray intensity skymap latitude maximum (deg); +90 -automatic binning
d_long = 4.0 gamma-ray intensity skymap longitude binsize (deg)
d_lat = 4.0 gamma-ray intensity skymap latitude binsize (deg)
lat_substep_number = 1 latitude bin splitting (0,1=no split, 2=split in 2...)
LoS_step = 0.05 kpc, Line of Sight (LoS) integration step
LoS_substep_number = 1 number of substeps per LoS integration step (0,1=no substeps)
nuc_rigid_br = 9.0e3 reference rigidity for nucleus injection index in MV
nuc_g_1 = 1.98 nucleus injection index below reference rigidity
nuc_g_2 = 2.42 nucleus injection index index above reference rigidity
inj_spectrum_type = rigidity rigidity||beta_rig||Etot nucleon injection spectrum type
electron_g_0 = 1.60 electron injection index below electron_rigid_br0
electron_rigid_br0 = 4.0e3 reference rigidity0 for electron injection index in MV
electron_g_1 = 2.42 electron injection index below reference rigidity
electron_rigid_br = 1.0e9 reference rigidity for electron injection index in MV
electron_g_2 = 5.0 electron injection index index above reference rigidity
positron_g_0 = 1.70 positron injection index below positron_rigid_br0
positron_rigid_br0 = 4.2e3 reference rigidity0 for positron injection index in MV
positron_g_1 = 2.5 positron injection index below reference rigidity
positron_rigid_br = 2.0e9 reference rigidity for positron injection index in MV
positron_g_2 = 4.0 positron injection index index above reference rigidity
He_H_ratio = 0.11 He/H of ISM, by number
n_X_CO = 9 an option to select functional dependence of X_CO=X_CO(R) 0=constant as below, 9=standard variation as in A&A 2004 paper 10=an exponential
X_CO = 1.9E20 conversion factor from CO integrated temperature to H2 column density
nHI_model = 1 selection of HI gas density model (not yet implemented)
nH2_model = 1 selection of H2 gas density model (not yet implemented)
nHII_model = 3 selection of HII gas density model 1=Cordes et al 1991 2, 3 = other models
HII_Te = 7000 free electron temperature (K) for free-free absorption
HII_clumping_factor = 1 free electron clumping factor for free-free absorption
COR_filename = rbands_co10mm_v3_2001_hdeg.fits.gz
HIR_filename = rbands_hi12_v5_hdeg_zmax1_Ts125.fits.gz
ISRF_file = ISRF/Standard/Standard.dat see manual
ISRF_filetype = 3 0=CMB only,1=obsolete, 2=standard FITS, 3=healpix with angular dependence - see manual
ISRF_healpixOrder = 3 for output of ISRF skymaps
ISRF_factors = 1.0,1.0,1.0 ISRF factors for IC calculation: optical, FIR, CMB
fragmentation = 0 1=include fragmentation
momentum_losses = 1 1=include momentum losses
hadronic_losses = 1 1=include hadronic (pionic) losses
hadronic_loss_model = 2 0=simple test model, 1,2,3=Krakau&Schlickeiser 2015 model, 1=protons only, 2= A=1-4, 3= all A (caution!), 10= as 3 but *10 for test
radioactive_decay = 0 1=include radioactive decay
K_capture = 0 1=include K-capture
ionization_rate = 0 1=compute ionization rate
start_timestep = 2.0e8
end_timestep = 1.0e1
timestep_factor = 0.5
timestep_repeat = 50 number of repeats per timestep in timetep_mode=1 - must be integer! - this set gives about 2500 steps in total
timestep_repeat2 = 0 number of timesteps in timetep_mode=2
timestep_print = 1000000000 number of timesteps between printings
timestep_diagnostics = 100 number of timesteps between diagnostics
control_diagnostics = 0 control detail of diagnostics
solution_method = 1 1=Crank-Nicolson, 2=fully time explicit, 21=fully time explicit turbo
solution_convergence = 1 1=use convergence test
network_iterations = 1 number of iterations of protons
network_iter_compl = 1 number of iterations of entire network (default 1 if absent)
prop_r = 1 1=propagate in r (2D)
prop_x = 1 1=propagate in x (2D,3D)
prop_y = 1 1=propagate in y (3D)
prop_z = 1 1=propagate in z (3D)
prop_p = 1 1=propagate in momentum
use_symmetry = 0 0=no symmetry, 1=optimized symmetry, 2=xyz symmetry by copying(3D)
spatial_bound_conds = 2 spatial boundary conditions. 1:CR=0 at boundaries (default), 2: free escape at boundaries
source_specification = 0 2D::1:r,z=0 2:z=0 3D::1:x,y,z=0 2:z=0 3:x=0 4:y=0
source_model = 1 0=zero 1=parameterized 2=Case&B 3=pulsars 4= 5=S&Mattox 6=S&Mattox with cutoff 7=Gaussian 8=user-defined values source model for nuclei
source_parameters_0 = 0.2 model 1:zscale, kpc
source_parameters_1 = 0.475063 1.25 2.35 model 1:alpha model 7: Gaussian mean, kpc from GC
source_parameters_2 = 2.16570 3.56 5.56283 model 1:beta model 7: Gaussian width, kpc
source_parameters_3 = 15 model 1, 7 :rmax: set to zero beyond this radius, kpc from GC
source_parameters_4 = 10 model 1, 7: rconst: set to value at rconst for rconst<r<rmax, kpc from GC
source_parameters_5 = 0.0 not yet used
source_model_elec = 1 source model for electrons (parameter values default to nuclei values if they are absent)
source_pars_elec_1 = 0.485063 1.25 2.35 model 1:alpha model 7: Gaussian mean, kpc from GC
source_pars_elec_2 = 2.17570 3.56 5.56283 model 1:beta model 7: Gaussian width, kpc
source_pars_elec_3 = 16.0 model 1, 7 :rmax: set to zero beyond this radius, kpc from GC
source_pars_elec_4 = 11.0 model 1, 7: rconst: set to value at rconst for rconst<r<rmax, kpc from GC
source_pars_elec_5 = 0.0 not yet used
source_model_posi = 1 source model for positrons (parameter values default to nuclei values if they are absent)
source_pars_posi_1 = 0.495063 1.25 2.35 model 1:alpha model 7: Gaussian mean, kpc from GC
source_pars_posi_2 = 2.18570 3.56 5.56283 model 1:beta model 7: Gaussian width, kpc
source_pars_posi_3 = 17.0 model 1, 7 :rmax: set to zero beyond this radius, kpc from GC
source_pars_posi_4 = 12.0 model 1, 7: rconst: set to value at rconst for rconst<r<rmax, kpc from GC
source_pars_posi_5 = 1.0 not yet used
n_source_values = 0 model 8: number of points for CR source distribution
source_radius = 0,1,2,3,4,5,6,7,8,9,10,20 model 8: radius for points for CR source distribution, kpc from GC
source_values = 2,3,4,5,6,7,6,5,4,3,02,01 model 8: values at points for CR source distribution
n_cr_sources = 0 number of pointlike cosmic-ray sources 3D only!
cr_source_x_01 = 10.0 x position of cosmic-ray source 1 (kpc)
cr_source_y_01 = 10.0 y position of cosmic-ray source 1
cr_source_z_01 = 0.1 z position of cosmic-ray source 1
cr_source_w_01 = 0.1 sigma width of cosmic-ray source 1
cr_source_L_01 = 1.0 luminosity of cosmic-ray source 1
cr_source_x_02 = 3.0 x position of cosmic-ray source 2
cr_source_y_02 = 4.0 y position of cosmic-ray source 2
cr_source_z_02 = 0.2 z position of cosmic-ray source 2
cr_source_w_02 = 2.4 sigma width of cosmic-ray source 2
cr_source_L_02 = 2.0 luminosity of cosmic-ray source 2
SNR_events = 0 handle stochastic SNR events
SNR_interval = 1.0e4 time interval in years between SNR in 1 kpc^-3 volume
SNR_livetime = 1.0e4 CR-producing live-time in years of an SNR
SNR_electron_sdg = 0.00 delta electron source index Gaussian sigma
SNR_nuc_sdg = 0.00 delta nucleus source index Gaussian sigma
SNR_electron_dgpivot = 5.0e3 delta electron source index pivot rigidity (MeV)
SNR_nuc_dgpivot = 5.0e3 delta nucleus source index pivot rigidity (MeV)
proton_norm_Ekin = 1.00e+5 proton kinetic energy for normalization (MeV)
proton_norm_flux = 5.75e-9 6.75e-9 5.75e-9 5.00e-9 to renorm nuclei/flux of protons at norm energy (cm^-2 sr^-1 s^-1 MeV^-1)
electron_norm_Ekin = 3.45e4 electron kinetic energy for normalization (MeV)
electron_norm_flux = 0.32e-9 0.56e-9 0.32e-9 0.4e-9 0.6e-9 0.40e-9 flux of electrons at normalization energy (cm^-2 sr^-1 s^-1 MeV^-1)
positron_norm_Ekin = 3.55e4 positron kinetic energy for normalization (MeV)
positron_norm_flux = 0.42e-9 0.56e-9 0.32e-9 0.4e-9 0.6e-9 0.40e-9 flux of positrons at normalization energy (cm^-2 sr^-1 s^-1 MeV^-1)
max_Z = 0 the largest atomic number (Z) in the nuclear reaction network
use_Z_1 = 1
use_Z_2 = 1
use_Z_3 = 1
use_Z_4 = 1
use_Z_5 = 1
use_Z_6 = 1
use_Z_7 = 1
use_Z_8 = 1
use_Z_9 = 1
use_Z_10 = 1
use_Z_11 = 1
use_Z_12 = 1
use_Z_13 = 1
use_Z_14 = 1
use_Z_15 = 1
use_Z_16 = 1
use_Z_17 = 1
use_Z_18 = 1
use_Z_19 = 1
use_Z_20 = 1
use_Z_21 = 1
use_Z_22 = 1
use_Z_23 = 1
use_Z_24 = 1
use_Z_25 = 1
use_Z_26 = 1
use_Z_27 = 1
use_Z_28 = 1
use_Z_29 = 0
use_Z_30 = 0
iso_abundance_01_001 = 1.06e+06 H
iso_abundance_01_002 = 0. 34.8
iso_abundance_02_003 = 9.033 He
iso_abundance_02_004 = 7.199e+04
iso_abundance_03_006 = 0 Li
iso_abundance_03_007 = 0
iso_abundance_04_009 = 0 Be
iso_abundance_05_010 = 0 B
iso_abundance_05_011 = 0
iso_abundance_06_012 = 2819 C
iso_abundance_06_013 = 5.268e-07
iso_abundance_07_014 = 182.8 N
iso_abundance_07_015 = 5.961e-05
iso_abundance_08_016 = 3822 O
iso_abundance_08_017 = 6.713e-07
iso_abundance_08_018 = 1.286
iso_abundance_09_019 = 2.664e-08 F
iso_abundance_10_020 = 312.5 Ne
iso_abundance_10_021 = 0.003556
iso_abundance_10_022 = 100.1
iso_abundance_11_023 = 22.84 Na
iso_abundance_12_024 = 658.1 Mg
iso_abundance_12_025 = 82.5
iso_abundance_12_026 = 104.7
iso_abundance_13_027 = 76.42 Al
iso_abundance_14_028 = 725.7 Si
iso_abundance_14_029 = 35.02
iso_abundance_14_030 = 24.68
iso_abundance_15_031 = 4.242 P
iso_abundance_16_032 = 89.12 S
iso_abundance_16_033 = 0.3056
iso_abundance_16_034 = 3.417
iso_abundance_16_036 = 0.0004281
iso_abundance_17_035 = 0.7044 Cl
iso_abundance_17_037 = 0.001167
iso_abundance_18_036 = 9.829 Ar
iso_abundance_18_038 = 0.6357
iso_abundance_18_040 = 0.001744
iso_abundance_19_039 = 1.389 K
iso_abundance_19_040 = 3.022
iso_abundance_19_041 = 0.0003339
iso_abundance_20_040 = 51.13 Ca
iso_abundance_20_041 = 1.974
iso_abundance_20_042 = 1.134e-06
iso_abundance_20_043 = 2.117e-06
iso_abundance_20_044 = 9.928e-05
iso_abundance_20_048 = 0.1099
iso_abundance_21_045 = 1.635 Sc
iso_abundance_22_046 = 5.558 Ti
iso_abundance_22_047 = 8.947e-06
iso_abundance_22_048 = 6.05e-07
iso_abundance_22_049 = 5.854e-09
iso_abundance_22_050 = 6.083e-07
iso_abundance_23_050 = 1.818e-05 V
iso_abundance_23_051 = 5.987e-09
iso_abundance_24_050 = 2.873 Cr
iso_abundance_24_052 = 8.065
iso_abundance_24_053 = 0.003014
iso_abundance_24_054 = 0.4173
iso_abundance_25_053 = 6.499 Mn
iso_abundance_25_055 = 1.273
iso_abundance_26_054 = 49.08 Fe
iso_abundance_26_056 = 697.7
iso_abundance_26_057 = 21.67
iso_abundance_26_058 = 3.335
iso_abundance_27_059 = 2.214 Co
iso_abundance_28_058 = 28.88 Ni
iso_abundance_28_060 = 11.9
iso_abundance_28_061 = 0.5992
iso_abundance_28_062 = 1.426
iso_abundance_28_064 = 0.3039
total_cross_section = 2 total cross section option: 0=L83 1=WA96 2=BP01
cross_section_option = 022 100*i+j i=1: use Heinbach-Simon C,O->B j=kopt j=11=Webber, 21=ST
t_half_limit = 1.0e4 year - lower limit on radioactive half-life for explicit inclusion
primary_electrons = 0 1=compute primary electrons
primary_positrons = 0 1=compute primary positrons
secondary_electrons = 0 1=compute secondary electrons
secondary_positrons = 0 1=compute secondary positrons
knock_on_electrons = 0 1,2 1=compute knock-on electrons (p,He) 2= use factor 1.75 to scale pp,pHe
pairproduction = 0 1=compute pair production on ISRF
secondary_antiproton = 0 1,2= calculate: 1=uses nuclear scaling; 2=uses nuclear factors (Simon et al 1998) NB parameter name changed at r548
tertiary_antiproton = 0 1=compute tertiary antiprotons NB parameter name changed at r548
secondary_protons = 0 1=compute secondary protons
globalLuminosities = 0 1=compute global luminosities, 0=don't (default)
skymap_format = 3 fitsfile format: 0=old format (the default), 1=mapcube for glast science tools, 2=both, 3=healpix
healpix_order = 7 order for healpix skymaps. 7 gives ~0.5 deg and it changes by an order of 2
output_gcr_full = 0 output full galactic cosmic ray array
warm_start = 0 read in nuclei file and continue run
GCR_data_filename = GCR_data_5.dat
verbose = 0 -456 -455 -454 -453 verbosity: 0=min,10=max <0: selected debugs
test_suite = 0 run test suite instead of normal run
rigid_min = 0.0 min rigidity for sources
rigid_max = 1.0E38 max rigidity for sources
