The choice of colliding-beam energy for polarized DY physics is important since the cross sections are small and the region in which large polarization effects are most likely to be observed is . The region, is inaccessible due to the steeply falling structure function . Optimization of the collision energy can be accomplished by reducing the DY cross section,
to the scaling form,
From Appendix A one sees that the acceptance of a spectrometer depends only on and . This means that may be measured with roughly equal acceptance at , or , ; however, from Eq. 2 the cross section at will be 16 times larger.
Finally, the luminosity of RHIC for pp collisions is expected to scale as . Thus, the event rate,