“…In this case, when reducing the characteristic Breit-Wheeler energy within the range ω BW ∼ 10 ÷ 1 GeV, the maximum resonant cross-section can reach values of R * ±(1,1) ∼ 10 3 ÷ 10 6 r 2 e . The obtained results could be used to explain the narrow fluxes of high-energy ultrarelativistic positrons (electrons) in the vicinity of neutron stars, such as accretion-powered X-ray binaries [49,50], rotation-powered X/Gamma pulsars [51,52] and magnetic-fieldpowered magnetars [53,54], as well as to simulate physical processes in laser thermonuclear fusion [55].…”