STARlight: A Monte Carlo simulation program for ultra-peripheral collisions of relativistic ions
Spencer R. Klein, Joakim Nystrand, Janet Seger, Yuri Gorbunov, Joey, Butterworth

TL;DR
STARlight is a Monte Carlo simulation tool designed to calculate cross-sections and generate events for ultra-peripheral relativistic ion collisions, aiding in the study of electromagnetic interactions at RHIC and LHC.
Contribution
It introduces a comprehensive Monte Carlo program for simulating ultra-peripheral collisions, including cross-section calculations and event generation for various final states.
Findings
Provides accurate cross-section calculations for UPCs.
Enables detailed event simulation for detector efficiency studies.
Supports analysis of photonuclear and two-photon interactions.
Abstract
Ultra-peripheral collisions (UPCs) have been a significant source of study at RHIC and the LHC. In these collisions, the two colliding nuclei interact electromagnetically, via two-photon or photonuclear interactions, but not hadronically; they effectively miss each other. Photonuclear interactions produce vector meson states or more general photonuclear final states, while two-photon interactions can produce lepton or meson pairs, or single mesons. In these interactions, the collision geometry plays a major role. We present a program, STARlight, that calculates the cross-sections for a variety of UPC final states and also creates, via Monte Carlo simulation, events for use in determining detector efficiency.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
