In the cold underdense model, 1−vg/c≃n/(2nc) and γϕ2≃nc/n=500. A relativistic electron slips through half an accelerating sinusoidalwavelength over Ld≃γϕ2λp≃8.35 mm. For Ez=E0sinϕ and injection at the start of that half-cycle, integration over 0<ϕ<π gives