Ultra-Peripheral Collisions with gold ions in STAR
  In 2010, the STAR Collaboration collected 38 million low-multiplicity triggers for ultra-peripheral collision studies. We present new results involving photonuclear interactions in ultra-peripheral relativistic heavy ion collisions (UPCs), based on an analysis of 384,000 photoproduced pion pairs, from $\rho$, $\omega$ and direct $\pi^+\pi^-$ pair production.The $\omega$ component is clearly visible through its interference with the $\rho$ peak. The relative amplitudes of the three components have been measured, along with the phase angle between the $\rho$ and $\omega$ components.   Using a two-year (2010 and 2011) dataset, we explore higher mass final states, and observe a $\pi^+\pi^-$ state with a mass of $1653 \pm 10$ MeV and a width of $164\pm 15$ MeV (statistical errors only). The state is at least roughly compatible with the $\rho_3(1690)$.   The $\rho^0$ squared momentum transfer ($t$) spectrum exhibits a spectrum with both coherent and incoherent prodution. The coherent component shows two characteristic diffraction minima, with positions that are sensitive to the hadronic radius of the gold nucleus. 
Spencer R. Klein (for the STAR Collaboration)
nucl-ex hep-ex