This analysis derives a formula for Bhabha scattering cross-section, suggesting refined estimates for particle interactions in colliders.
A simple analytical formula is derived for the total rate of small angle radiative Bhabha scattering, using the no-recoil approximation. This expression illustrates how radiative processes soften the forward angle singularity so that the cross-section for all electrons which have radiated an energy larger that a given amount ΔE, is only logarithmically divergent as m_e→0. Estimate of the total integrated rate at a \φ-factory are given, and a comparison is made with existing calculations.
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Pancheri G. (1993) studied this question.
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