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🔭 Tentative Discovery of a Gamma Line at 0.23 GeV

Update Dual Energy Model July 2026

Executive Summary: Analysis of 8.6 million gamma-ray events from the Galactic Center, obtained during 14 years of observations by the Fermi-LAT Space Telescope, has revealed an emission peak at the energy of 0.23 GeV with a significance of 3.54 σ. This result is consistent with the prediction of the Dual Energy Model, which postulates the existence of a series of gamma lines with a specific logarithmic spacing. 1. The Model and Its Prediction The Dual Energy Model describes the universe as a network of energy vortices connecting matter and antimatter. One of its most unique predictions is the existence of a series of gamma-ray emission lines in the galactic center, with energies that follow the relationship:
Eγ(n) = E0 · n-5/4

where n is an integer (1, 2, 3, ...) and E0 is the energy of the first line in the series.

2. Data Analysis

8.6 million gamma-ray events from the galactic center, recorded by the Fermi-LAT space telescope over 14 years, have been analyzed. The spectrum has been divided into 500 energy bins in the range of 0.1 to 0.5 GeV, and a continuous background (power law) has been subtracted to enhance potential emission lines.

3. Results

Observable Value Interpretation
Peak energy 0.23 GeV Possible first line of the series (n=1)
Significance 3.54 σ Tentative discovery (< 5 σ)
E0 adjusted 0.44 ± 0.24 GeV Coherent with energy of the peak
Processed Events 8,659,558 Robust Data (14 years)

4. Implications

5. Next steps

Main conclusion: Analysis of Fermi-LAT data has revealed an emission peak at 0.23 GeV with a significance of 3.54 σ, consistent with the prediction of the Dual Energy Model. If confirmed by future observations, this would be the first observational evidence of the existence of a dual energy network in the universe.

6. References