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STARlight: A Monte Carlo simulation program for ultra-peripheral collisions of relativistic ions

Tool reference. 80% of classified Pith citations use this work as a method, library, or software dependency, not as a substantive claim.

13 Pith papers citing it
Method reference 80% of classified citations
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.

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Searches for GeV-Scale ALPs at RHIC

hep-ph · 2026-06-05 · unverdicted · novelty 6.0

Proposes searching for GeV-scale ALPs in ultra-peripheral collisions at RHIC via γγ → a → γγ, estimating sensitivity to m_a ~2-5 GeV and g_aγγ ≳4e-4 GeV^{-1} with existing PHENIX data.

Absorption of 1$P$-wave heavy charmonium $\chi_{c1}(1P)$ in nuclei

nucl-th · 2026-04-01 · unverdicted · novelty 3.0

Calculations of excitation functions, momentum spectra, and transparency ratios for χ_c1(1P) on 12C and 184W nuclei demonstrate sensitivity to different absorption cross-section scenarios, proposed for extraction via future CEBAF data.

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  • Absorption of 1$P$-wave heavy charmonium $\chi_{c1}(1P)$ in nuclei nucl-th · 2026-04-01 · unverdicted · none · ref 111 · internal anchor

    Calculations of excitation functions, momentum spectra, and transparency ratios for χ_c1(1P) on 12C and 184W nuclei demonstrate sensitivity to different absorption cross-section scenarios, proposed for extraction via future CEBAF data.