Energy dependence of polarized 𝛾𝛾→𝑒+𝑒− in peripheral Au+Au collisions at √𝑠𝑁𝑁=54.4 and 200 GeV with the STAR experiment at RHIC
Resource type
Authors/contributors
- STAR Collaboration (Author)
- Finch, Evan (Contributor)
Title
Energy dependence of polarized 𝛾𝛾→𝑒+𝑒− in peripheral Au+Au collisions at √𝑠𝑁𝑁=54.4 and 200 GeV with the STAR experiment at RHIC
Abstract
We report the differential yields at mid-rapidity of the Breit-Wheeler process (𝛾𝛾→𝑒+𝑒−) in peripheral Au+Au collisions at √𝑠𝑁𝑁=54.4 and 200 GeV with the STAR experiment at the Relativistic Heavy Ion Collider (RHIC), as a function of energy √𝑠𝑁𝑁, 𝑒+𝑒− transverse momentum 𝑝T, 𝑝2T, invariant mass 𝑀𝑒𝑒, and azimuthal angle. In the invariant mass range of 0.4<𝑀𝑒𝑒<2.6GeV/𝑐2 at low transverse momentum (𝑝T<0.15GeV/𝑐), the yields increase while the pair √⟨𝑝2T⟩ decreases with increasing √𝑠𝑁𝑁, a feature that is correctly predicted by the QED calculation. The energy dependencies of the measured quantities are sensitive to the nuclear form factor, infrared divergence and photon polarization. The data are compiled and used to extract the charge radius of the Au nucleus.
Publication
Physical Review C
Publisher
American Physical Society
Date
2025-01-16
Volume
111
Issue
1
Pages
014909
Journal Abbr
Phys. Rev. C
Citation Key
starcollaborationEnergyDependencePolarized2025
Accessed
1/31/25, 6:44 PM
Library Catalog
APS
Citation
STAR Collaboration. (2025). Energy dependence of polarized 𝛾𝛾→𝑒+𝑒− in peripheral Au+Au collisions at √𝑠𝑁𝑁=54.4 and 200 GeV with the STAR experiment at RHIC. Physical Review C, 111(1), 014909. https://doi.org/10.1103/PhysRevC.111.014909
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