AbstractWe examine the East‐West asymmetry of the peak intensity in energetic storm particle (ESP) events using the improved Particle Acceleration and Transport in the Heliosphere model. We find that injection efficiency peaks east of the nose of coronal mass ejection shock where the shock exhibits a quasi‐parallel geometry. We show that the peak intensity at the eastern flank is generally larger than that at the western flank and it positively correlates with the injection efficiency. We also examine this asymmetry for heavy ions, which depends sensitively on the ion energy. Comparison between the modeling results with the measurements of ESP events at 1 au shows a reasonable agreement. We suggest that the injection efficiency can be a primary factor leading to the East‐West asymmetry of the peak intensity in ESP events. Additionally, the charge‐to‐mass (Q/A) dependence of the maximum particle energy affects this asymmetry for heavy ions.