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Fermi Diffuse Emission at Intermediate Galactic Latitudes https://galprop.stanford.edu/forum/viewtopic.php?f=4&t=102 |
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Author: | christian [ Wed Sep 22, 2010 2:16 am ] | ||
Post subject: | Fermi Diffuse Emission at Intermediate Galactic Latitudes | ||
Hi, I'm trying to reproduce the diffuse emission spectra from GALPROP used in the Fermi paper http://arxiv.org/pdf/0912.0973 "Fermi Large Area Telescope Measurement of the Diffuse Gamma-Ray Emission at Intermediate Galactic Latitudes ". Therefore I copied the datapoints for the GALPROP prediction in Fig. 2, page 5 in the cited paper and tried to reproduce these points with the Galprop webrun v54. For pion decay and bremsstrahlung it looks very fine. However for IC the fermi model is a factor 2 above the prediction of the conventional model I use (see attached plot). Can you think of any reason for this? How can it be that the bremsstrahlung emission is the same for both models but the IC isn't? Can this have something to do with another ISRF model used by the Fermi people? A typical GALDEF file that I'm using is attached. Many thanks, Gerrit n_spatial_dimensions = 2 r_min = 00.0 r_max = 20.00 dr = 1.0 z_min = -4.0 z_max = +4.0 dz = 0.1 x_min = 0.0 x_max = +15.0 dx = 0.2 y_min = 0.0 y_max = +15.0 dy = 0.2 p_Ekin_grid = Ekin p_min = 1000 p_max = 4000 p_factor = 1.3 Ekin_min = 1.0e1 Ekin_max = 1.0e10 Ekin_factor = 1.3 gamma_rays = 1 pi0_decay = 1 IC_isotropic = 1 IC_anisotropic = 0 bremss = 1 integration_mode = 0 E_gamma_min = 1.0e1 E_gamma_max = 1.0e6 E_gamma_factor = 1.3 ISRF_factors = 1.0,1.0,1.0 synchrotron = 0 nu_synch_min = 1.0e6 nu_synch_max = 1.0e10 nu_synch_factor = 2.0 long_min = 0.50 long_max = 359.50 lat_min = -90.0 lat_max = -10.0 d_long = 1.0 d_lat = 1.0 healpix_order = 6 lat_substep_number = 1 LoS_step = 0.01 LoS_substep_number = 1 DM_positrons = 0 DM_electrons = 0 DM_antiprotons = 0 DM_gammas = 0 D0_xx = 5.75e28 D_rigid_br = 4.0e3 D_g_1 = 0.34 D_g_2 = 0.34 diff_reacc = 1 v_Alfven = 36. damping_p0 = 1.e6 damping_const_G = 0.02 damping_max_path_L = 3.e21 convection = 0 v0_conv = 0. dvdz_conv = 10. nuc_rigid_br = 9.0e3 nuc_g_1 = 1.82 nuc_g_2 = 2.36 inj_spectrum_type = rigidity electron_g_0 = 1.60 electron_rigid_br0 = 4.0e3 electron_g_1 = 2.50 electron_rigid_br = 1.0e9 electron_g_2 = 5.0 He_H_ratio = 0.11 n_X_CO = 9 X_CO = 1.9E20 X_CO_parameters_0 = 1.0E20 X_CO_parameters_1 = 1 X_CO_parameters_2 = 0 X_CO_parameters_3 = 0 n_HI_model = 1 n_H2_model = 1 n_HII_model = 1 COR_filename = r HIR_filename = r fragmentation = 1 momentum_losses = 1 radioactive_decay = 1 K_capture = 1 ionization_rate = 0 start_timestep = 1.0e9 end_timestep = 1.0e1 timestep_factor = 0 timestep_repeat = 20 timestep_repeat2 = 0 timestep_print = 10000 timestep_diagnostics = 10000 control_diagnostics = 0 network_iterations = 2 network_iter_compl = 2 network_iter_sec = 1 prop_r = 1 prop_x = 1 prop_y = 1 prop_z = 1 prop_p = 1 use_symmetry = 0 vectorized = 0 source_specification = 0 source_model = 1 source_parameters_1 = 0.5 source_parameters_2 = 1.0 source_parameters_3 = 20.0 source_parameters_4 = 20.0 source_parameters_5 = 0.0 n_cr_sources = 0 cr_source_x_01 = 10.0 cr_source_y_01 = 10.0 cr_source_z_01 = 0.1 cr_source_w_01 = 0.1 cr_source_L_01 = 1.0 cr_source_x_02 = 3.0 cr_source_y_02 = 4.0 cr_source_z_02 = 0.2 cr_source_w_02 = 2.4 cr_source_L_02 = 2.0 cr_source_x_03 = 0.0 cr_source_y_03 = 0.0 cr_source_z_03 = 0.0 cr_source_w_03 = 0.0 cr_source_L_03 = 0.0 cr_source_x_04 = 0.0 cr_source_y_04 = 0.0 cr_source_z_04 = 0.0 cr_source_w_04 = 0.0 cr_source_L_04 = 0.0 cr_source_x_05 = 0.0 cr_source_y_05 = 0.0 cr_source_z_05 = 0.0 cr_source_w_05 = 0.0 cr_source_L_05 = 0.0 SNR_events = 0 SNR_interval = 1.0e4 SNR_livetime = 1.0e4 SNR_electron_sdg = 0.0 SNR_nuc_sdg = 0.0 SNR_electron_dgpivot = 5.0e3 SNR_nuc_dgpivot = 5.0e3 ISRF_file = ISRF/Standard/Standard.dat ISRF_filetype = 3 ISRF_healpixOrder = 3 B_field_model = 050100020 proton_norm_Ekin = 1.00e+5 proton_norm_flux = 4.90e-9 electron_norm_Ekin = 34.5e3 electron_norm_flux = .40e-9 max_Z = 28 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 = 1 use_Z_30 = 1 iso_abundance_01_001 = 1.06e+06 iso_abundance_01_002 = 34.8 iso_abundance_02_003 = 9.033 iso_abundance_02_004 = 7.199e+04 iso_abundance_03_006 = 0 iso_abundance_03_007 = 0 iso_abundance_04_007 = 0.0 iso_abundance_04_009 = 0 iso_abundance_04_010 = 0.0 iso_abundance_05_010 = 0 iso_abundance_05_011 = 0 iso_abundance_06_012 = 2819 iso_abundance_06_013 = 5.268e-07 iso_abundance_07_014 = 182.8 iso_abundance_07_015 = 5.961e-05 iso_abundance_08_016 = 3822 iso_abundance_08_017 = 6.713e-07 iso_abundance_08_018 = 1.286 iso_abundance_09_019 = 2.664e-08 iso_abundance_10_020 = 312.5 iso_abundance_10_021 = 0.003556 iso_abundance_10_022 = 100.1 iso_abundance_11_023 = 22.84 iso_abundance_12_024 = 658.1 iso_abundance_12_025 = 82.5 iso_abundance_12_026 = 104.7 iso_abundance_13_027 = 76.42 iso_abundance_14_028 = 725.7 iso_abundance_14_029 = 35.02 iso_abundance_14_030 = 24.68 iso_abundance_15_031 = 4.242 iso_abundance_16_032 = 89.12 iso_abundance_16_033 = 0.3056 iso_abundance_16_034 = 3.417 iso_abundance_16_036 = 0.0004281 iso_abundance_17_035 = 0.7044 iso_abundance_17_037 = 0.001167 iso_abundance_18_036 = 9.829 iso_abundance_18_038 = 0.6357 iso_abundance_18_040 = 0.001744 iso_abundance_19_039 = 1.389 iso_abundance_19_040 = 3.022 iso_abundance_19_041 = 0.0003339 iso_abundance_20_040 = 51.13 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 iso_abundance_22_046 = 5.558 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 iso_abundance_23_051 = 5.987e-09 iso_abundance_24_050 = 2.873 iso_abundance_24_051 = 0 iso_abundance_24_052 = 8.065 iso_abundance_24_053 = 0.003014 iso_abundance_24_054 = 0.4173 iso_abundance_25_053 = 6.499 iso_abundance_25_055 = 1.273 iso_abundance_26_054 = 49.08 iso_abundance_26_055 = 0 iso_abundance_26_056 = 697.7 iso_abundance_26_057 = 21.67 iso_abundance_26_058 = 3.335 iso_abundance_27_059 = 2.214 iso_abundance_28_058 = 28.88 iso_abundance_28_059 = 0 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 cross_section_option = 012 t_half_limit = 1.0e4 primary_electrons = 1 secondary_electrons = 1 knock_on_electrons = 0 secondary_positrons = 1 secondary_protons = 1 secondary_antiproton = 2 tertiary_antiproton = 1 skymap_format = 0 output_gcr_full = 0 warm_start = 0 verbose = 0 test_suite = 0
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Author: | strong [ Wed Sep 29, 2010 7:59 am ] |
Post subject: | Re: Fermi Diffuse Emission at Intermediate Galactic Latitude |
the ISRF did indeed change, but I did not expect the difference to be a factor 2. Did you include all the components (CMB, FIR, optical) if you used the ISRF components file ? I cannot open your attachments by the way. |
Author: | avladim [ Wed Sep 29, 2010 1:09 pm ] |
Post subject: | Re: Fermi Diffuse Emission at Intermediate Galactic Latitude |
The attachment shows now, my bad. |
Author: | strong [ Wed Sep 29, 2010 11:16 pm ] |
Post subject: | Re: Fermi Diffuse Emission at Intermediate Galactic Latitude |
I expect the difference is in the electron injection spectral slope - you have 2.50 but we used 2.42 I think in the Fermi paper. this does not affect the bremss which comes from low energy electrons but has a big effect on IC from higher energies. You can see this clearly since the IC slope is flatter in the Fermi than yours. |
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