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
Funding Sponsor
National Research Foundation of Korea
Author's Department
Chemistry Department
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https://doi.org/10.1103/PhysRevC.111.014909
Document Type
Research Article
Publication Title
Physical Review C
Publication Date
1-1-2025
doi
10.1103/PhysRevC.111.014909
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, pT2, invariant mass Mee, and azimuthal angle. In the invariant mass range of 0.4
Recommended Citation
APA Citation
Abdulhamid, M.
Aboona, B.
Adam, J.
Adams, J.
...
(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),
https://doi.org/10.1103/PhysRevC.111.014909
MLA Citation
Abdulhamid, M. I., et al.
"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, vol. 111, no. 1, 2025
https://doi.org/10.1103/PhysRevC.111.014909
