# CLUMPY, version v3.0.1_ID818b0be # Parameter file to work with h2, h4, z modes (parameters to be added otherwise) # Variable name Unit Value (Format) (Comment) #------------------------------------------------------------------------------ # Cosmological parameters #------------------------------------------------------------------------------ gCOSMO_DELTA0 [-] 200 Overdensity factor at z=0;-1 for kBRYANNORMAN98 gCOSMO_FLAG_DELTA_REF [-] kRHO_CRIT Reference density of the overdensity factor #------------------------------------------------------------------------------ # Dark Matter global parameters #------------------------------------------------------------------------------ gDM_LOGCDELTA_STDDEV [-] 0 log-std. deviation of subhalo scattering gDM_RHOSAT [Msol/kpc^3] 1e+19 Dark Matter saturation density gDM_SUBS_MMIN [Msol] 1e-06 Smallest subclump mass gDM_SUBS_MMAXFRAC [-] 0.01 Biggest subclump mass, fraction of host mass gDM_SUBS_NUMBEROFLEVELS [-] 1 Number of multilevel substructures #------------------------------------------------------------------------------ # Extragalactic DM total and clump parameters (see cosmo.h and extragal.h) #------------------------------------------------------------------------------ gEXTRAGAL_FLAG_ABSORPTIONPROFILE [-] kFRANCESCHINI08 EBL absorption profile #------------------------------------------------------------------------------ # External lists with specified objects to add to simulations #------------------------------------------------------------------------------ gLIST_HALOES [-] coma.txt List of external halos definitions #------------------------------------------------------------------------------ # Universal sub-clustering properties for CLUMPY-defined external haloes, # separated into DSPH, GALAXY (but not our Galaxy!), and CLUSTER-like objects. # (N.B.: use gHALO_DPDV_RSCALE=kHOST and/or gHALO_DPDV_FLAG_PROFILE=kHOST # for the subclump distribution to follow that of the host smooth halo) #------------------------------------------------------------------------------ gDSPH_SUBS_FLAG_PROFILE [-] kHOST Halo profile of subclumps gDSPH_SUBS_SHAPE_PARAMS_0 [-] kHOST Shape parameter 1 of subclumps halo profile gDSPH_SUBS_SHAPE_PARAMS_1 [-] kHOST Shape parameter 2 of subclumps halo profile gDSPH_SUBS_SHAPE_PARAMS_2 [-] kHOST Shape parameter 3 of subclumps halo profile gDSPH_SUBS_FLAG_CDELTAMDELTA [-] kSANCHEZ14_200 Mass-concentration model of subclumps gDSPH_SUBS_DPDV_FLAG_PROFILE [-] kEINASTO dP/dV profile of subhalo distribution in host gDSPH_SUBS_DPDV_SHAPE_PARAMS_0 [-] 0.68 Shape parameter 1 of dP/dV distrib. profile gDSPH_SUBS_DPDV_SHAPE_PARAMS_1 [-] kHOST Shape parameter 2 of dP/dV distrib. profile gDSPH_SUBS_DPDV_SHAPE_PARAMS_2 [-] kHOST Shape parameter 3 of dP/dV distrib. profile gDSPH_SUBS_DPDV_RSCALE_TO_RS_HOST [-] 10 Scale radius of dP/dV profile to r_s of host gDSPH_SUBS_DPDM_SLOPE [-] 1.9 Slope of power-law subhalo mass spectrum dP/dM gDSPH_SUBS_MASSFRACTION [-] 0.2 Fraction of host halo mass bound in subhalos gGALAXY_SUBS_FLAG_PROFILE [-] kHOST Halo profile of subclumps gGALAXY_SUBS_SHAPE_PARAMS_0 [-] kHOST Shape parameter 1 of subclumps halo profile gGALAXY_SUBS_SHAPE_PARAMS_1 [-] kHOST Shape parameter 2 of subclumps halo profile gGALAXY_SUBS_SHAPE_PARAMS_2 [-] kHOST Shape parameter 3 of subclumps halo profile gGALAXY_SUBS_FLAG_CDELTAMDELTA [-] kSANCHEZ14_200 Mass-concentration model of subclumps gGALAXY_SUBS_DPDV_FLAG_PROFILE [-] kEINASTO dP/dV profile of subhalo distribution in host gGALAXY_SUBS_DPDV_SHAPE_PARAMS_0 [-] 0.68 Shape parameter 1 of dP/dV distrib. profile gGALAXY_SUBS_DPDV_SHAPE_PARAMS_1 [-] kHOST Shape parameter 2 of dP/dV distrib. profile gGALAXY_SUBS_DPDV_SHAPE_PARAMS_2 [-] kHOST Shape parameter 3 of dP/dV distrib. profile gGALAXY_SUBS_DPDV_RSCALE_TO_RS_HOST [-] 10 Scale radius of dP/dV profile to r_s of host gGALAXY_SUBS_DPDM_SLOPE [-] 1.9 Slope of power-law subhalo mass spectrum dP/dM gGALAXY_SUBS_MASSFRACTION [-] 0.2 Fraction of host halo mass bound in subhalos gCLUSTER_SUBS_FLAG_PROFILE [-] kHOST Halo profile of subclumps gCLUSTER_SUBS_SHAPE_PARAMS_0 [-] kHOST Shape parameter 1 of subclumps halo profile gCLUSTER_SUBS_SHAPE_PARAMS_1 [-] kHOST Shape parameter 2 of subclumps halo profile gCLUSTER_SUBS_SHAPE_PARAMS_2 [-] kHOST Shape parameter 3 of subclumps halo profile gCLUSTER_SUBS_FLAG_CDELTAMDELTA [-] kSANCHEZ14_200 Mass-concentration model of subclumps gCLUSTER_SUBS_DPDV_FLAG_PROFILE [-] kEINASTO dP/dV profile of subhalo distribution in host gCLUSTER_SUBS_DPDV_SHAPE_PARAMS_0 [-] 0.68 Shape parameter 1 of dP/dV distrib. profile gCLUSTER_SUBS_DPDV_SHAPE_PARAMS_1 [-] kHOST Shape parameter 2 of dP/dV distrib. profile gCLUSTER_SUBS_DPDV_SHAPE_PARAMS_2 [-] kHOST Shape parameter 3 of dP/dV distrib. profile gCLUSTER_SUBS_DPDV_RSCALE_TO_RS_HOST [-] 10 Scale radius of dP/dV profile to r_s of host gCLUSTER_SUBS_DPDM_SLOPE [-] 1.9 Slope of power-law subhalo mass spectrum dP/dM gCLUSTER_SUBS_MASSFRACTION [-] 0.2 Fraction of host halo mass bound in subhalos #------------------------------------------------------------------------------ # Particle physics parameters # N.B.: we recommend the use of kCIRELLI11 for the spectra. You then have to # select branching ratios in gPP_BR as a comma-separated # list (no space) of Br values for the 28 channels below: # 0: eL+eL- 1: eR+eR- 2: e+e- # 3: muL+muL- 4: muR+muR- 5: mu+mu- # 6: tauL+tauL- 7: tauR+tauR- 8: tau+tau- # 9: qqbar 10: ccbar 11: bbbar 12: ttbar # 13: WL+WL- 14: WT+WT- 15: W+W- # 16: ZLZL 17: ZTZT 18: ZZ # 19: gluglu 20: gammagamma 21: hh # 22: nuenue 23: numunumu 24: nutaunutau # 25: VV4e 26: VV4mu 27: VV4tau #------------------------------------------------------------------------------ gPP_BR [-] 0,0,0,0,0,0,0,0,0,0,0,1,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0, Branching channel ratio gPP_FLAG_SPECTRUMMODEL [-] kCIRELLI11_EW Spectrum model gPP_DM_ANNIHIL_DELTA [-] 2 Majorana (2) or Dirac (4) particle gPP_DM_ANNIHIL_SIGMAV_CM3PERS [cm^3/s] 3e-26 Annihilation cross section gPP_DM_IS_ANNIHIL_OR_DECAY [-] 1 Dark Matter Model (0: Decay, 1: Annihilation) gPP_DM_MASS_GEV [GeV] 100 [GeV] dark matter particle mass gPP_NUMIXING_THETA12_DEG [deg] 34 Neutrino mixing angle 1 gPP_NUMIXING_THETA13_DEG [deg] 9 Neutrino mixing angle 2 gPP_NUMIXING_THETA23_DEG [deg] 41 Neutrino mixing angle 3 #------------------------------------------------------------------------------ # Simulation parameters # Some parameters can be set to default values respectively automatically # adapted by setting to -1 (see documentation). # gSIM_OUTPUT_DIR: when set to -1, set to folder from where clumpy is executed. # gSIM_SEED: if=0, seed is chosen from computer clock (for drawing clumps) #------------------------------------------------------------------------------ gSIM_ALPHAINT_MIN_DEG [deg] 0.01 Minimum alpha_int value for 1D profile gSIM_ALPHAINT_MAX_DEG [deg] 5 Maximum alpha_int value for 1D profile gSIM_JFACTOR [variable] 6.53e+17 Input J/D-Factor for plotting flux spectrum gSIM_IS_ASTRO_OR_PP_UNITS [-] 0 Output units [Msol]&[kpc] (1) or [GeV]&[cm] (0) gSIM_REDSHIFT [-] 0.0234 Redshift of object(s) in the calculation gSIM_IS_WRITE_FLUXMAPS [-] 1 Calculate gamma-ray and/or neutrino fluxes gSIM_FLUX_IS_INTEG_OR_DIFF [-] 1 Flux either differential (0) or integrated (1) gSIM_FLUX_EMIN_GEV [GeV] 1 Lower limit for integrated flux gSIM_FLUX_EMAX_GEV [GeV] 99 Upper limit for integrated flux gSIM_FLUX_FLAG_FINALSTATE [-] kNEUTRINO Considered final state particle gSIM_FLUX_FLAG_NUFLAVOUR [-] kNUMU Considered neutrino flavour gSIM_IS_XLOG [-] 1 Evaluate and plot points in x-axis log-scale gSIM_NX [-] 100 # of points at which 1D calculation is done gSIM_XPOWER [-] 2 Multiply dependent variable with power of x val gSIM_THETA_SIZE_DEG [deg] 2.5 Grid diameter in theta-dir. gSIM_HEALPIX_NSIDE [-] 2048 Resolution parameter for HEALPix gSIM_GAUSSBEAM_GAMMA_FWHM_DEG [deg] -1 FWHM of Gaussian beam of gamma-ray telescope gSIM_GAUSSBEAM_NEUTRINO_FWHM_DEG [deg] -1 FWHM of Gaussian beam of neutrino telescope gLIST_HALONAME [-] Coma_ACO1656 Object selected out of a list of haloes gSIM_EPS [-] 0.01 Numeric precision of the simulation gSIM_IS_WRITE_ROOTFILES [-] 1 Write output additionally in ROOT format gSIM_OUTPUT_DIR [-] output/ Output directory (absolute or relative)