Energy Dependence of Polarized $\mathbf{γγ\rightarrow e^{+}e^{-}}$ in Peripheral Au+Au Collisions at RHIC

Fuente: arXiv
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Main Author: The STAR Collaboration
Format: Preprint
Published: 2024
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author The STAR Collaboration
author_facet The STAR Collaboration
contents We report the differential yields at mid-rapidity of the Breit-Wheeler process ($γγ\rightarrow e^{+}e^{-}$) in peripheral Au+Au collisions at $\sqrt{s_{_{\rm{NN}}}} = $ 54.4 GeV and 200 GeV with the STAR experiment at RHIC, as a function of energy $\sqrt{s_{_{\rm{NN}}}}$, $e^{+}e^{-}$ transverse momentum $p_{\rm T}$, $p_{\rm T}^{2}$, invariant mass $M_{ee}$ and azimuthal angle. In the invariant mass range of 0.4 $<$ $M_{ee}$ $<$ 2.6 GeV/$c^{2}$ at low transverse momentum ($p_{\rm T}$ $ < $0.15 GeV/$c$), the yields increase while the pair $\sqrt{\langle p_{\rm T}^{2} \rangle}$ decreases with increasing $\sqrt{s_{_{\rm{NN}}}}$, a feature 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.
format Preprint
id arxiv_https___arxiv_org_abs_2407_14821
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Energy Dependence of Polarized $\mathbf{γγ\rightarrow e^{+}e^{-}}$ in Peripheral Au+Au Collisions at RHIC
The STAR Collaboration
Nuclear Experiment
High Energy Physics - Experiment
We report the differential yields at mid-rapidity of the Breit-Wheeler process ($γγ\rightarrow e^{+}e^{-}$) in peripheral Au+Au collisions at $\sqrt{s_{_{\rm{NN}}}} = $ 54.4 GeV and 200 GeV with the STAR experiment at RHIC, as a function of energy $\sqrt{s_{_{\rm{NN}}}}$, $e^{+}e^{-}$ transverse momentum $p_{\rm T}$, $p_{\rm T}^{2}$, invariant mass $M_{ee}$ and azimuthal angle. In the invariant mass range of 0.4 $<$ $M_{ee}$ $<$ 2.6 GeV/$c^{2}$ at low transverse momentum ($p_{\rm T}$ $ < $0.15 GeV/$c$), the yields increase while the pair $\sqrt{\langle p_{\rm T}^{2} \rangle}$ decreases with increasing $\sqrt{s_{_{\rm{NN}}}}$, a feature 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.
title Energy Dependence of Polarized $\mathbf{γγ\rightarrow e^{+}e^{-}}$ in Peripheral Au+Au Collisions at RHIC
topic Nuclear Experiment
High Energy Physics - Experiment
url https://arxiv.org/abs/2407.14821