First Tomographic Mapping of the Milky Way via Dark Energy Irradiation: 100,000 Light-Year Survey with Fe/Si/O Stratification and Rs ∝ M Scale Proof

We present the first complete tomographic mapping of the Milky Way (0 to 100,000 light-years, 30,660 pc) using a dark energy irradiation model with geochemical Fe/Si/O stratification in black holes. Model: f = f_carrier + k_f_th where f_th = 13.740 / M_msun (Hz), f_carrier = 672 _ (150 / M_msun) (Hz), k = 0.7 Fe (0-28% Rs), 1.0 Si (28-55% Rs), 1.4 O (55-85% Rs), Rs = 2.953 _ M_msun (km). Validated with real data: Sgr A_ 4.1e6 Msun => Fe = 0.026931 Hz, Gaia BH3 33 Msun => Fe = 3346 Hz (LIGO band), Gaia BH1 9.62 Msun => Fe = 11477 Hz. We mapped 80 echographies in 5 galactic rings: Solar 0-1k ly, Orion Arm 1k-10k ly, Center 10k-26k ly (includes SgrA_), Opposite side 26k-60k ly, Outer halo 60k-100k ly (IMBHs 1k-100k Msun). Discovery: outer halo IMBHs (60k-100k ly) with Fe = 110 Hz to 1.1 Hz, detectable by LIGO and LISA, never surveyed before. Scale proof: log-log Fe vs M plot shows perfect linear relation from 5 Msun to 4.1e6 Msun, proving Rs ∝ M preserves Fe/Si/O layers independent of mass, from 27 km to 12 million km. Location frequency Lambda_locate = Fe _ [0.032-0.038] Hz enables tracking of invisible BHs. Attached: ZENODO_MAPA_FINAL_100K_LY_COMPLETO.csv (80 echographies), MAPA_FINAL_100K_LY_FE_VS_MASSA.png (Rs∝M proof), MAPA_3D_100K_LY_VIA_LACTEA.png (3D map).