Modeling spectral lags in active galactic nucleus flares in the context of Lorentz invariance violation searches

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Fig. 11.

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Time delay vs. energy for different initial maximum energy for electron γ_c, 0 values with B₀ = 65 mG (left) and B₀ = 90 mG (right). All other parameters are unchanged (Table 1). The two cases in bold in the legend correspond to the situation discussed in Sect. 4.2.

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