High-energy photons propagating through space can convert into electron-positron pairs by scattering with cosmic microwave background (CMB) photons. Taking the average CMB temperature of 2.8 K, a typical CMB photon will have an energy of roughly 7 × 10-4 eV. Calculate the minimum energy required for the high-energy photon to produce an electron-positron pair (me = 511 keV) if A the CMB photon momentum is perpendicular to that of the high-energy photon
High-energy photons propagating through space can convert into electron-positron pairs by scattering with cosmic microwave background (CMB) photons. Taking the average CMB temperature of 2.8 K, a typical CMB photon will have an energy of roughly 7 × 10-4 eV. Calculate the minimum energy required for the high-energy photon to produce an electron-positron pair (me = 511 keV) if A the CMB photon momentum is perpendicular to that of the high-energy photon
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