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| Formato: | Preprint |
| Publicado: |
2026
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| Acceso en línea: | https://arxiv.org/abs/2604.22184 |
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| _version_ | 1866913058934226944 |
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| author | STAR Collaboration |
| author_facet | STAR Collaboration |
| contents | In this paper, a study of cold nuclear matter (CNM) effects is reported based on the new STAR measurement of inclusive $J/ψ$ production in $p+p$ and $p+\text{Au}$ collisions at $\sqrt{s_\text{NN}}$ = 200 GeV, and a combined $J/ψ\rightarrow e^{+}e^{-}$ cross section in $p+p$ collisions at $\sqrt{s}$ = 200 GeV is provided. Given the long-established presumption that the energy density and the temperature produced in proton-nucleon collisions are insufficient to form QGP droplets, CNM effects in $p+\text{Au}$ collisions are quantified by the nuclear modification factor ($R_{p\text{Au}}$), defined as the ratio of the yield of the inclusive $J/ψ$ in $p+\text{Au}$ collisions to that in $p+p$ collisions, scaled by the average number of binary nucleon-nucleon collisions. The $R_{p\text{Au}}$ is derived as a function of transverse momentum ($p_\text{T}$) in the range 4--12 GeV/$c$ and is averaged within the rapidity ($y$) and azimuthal angle ($φ$) coverage of $|y|<1$, $0 \leq φ< 2π$. The result is consistent with unity, suggesting negligible modification of the yield by CNM effects in this kinematic region. Various model calculations are in agreement with the $R_{p\text{Au}}$ measurement, yet the same calculations are less satisfactory in describing the individual invariant yields from $p+p$ and $p+\text{Au}$ collisions. In the covered kinematic region, this analysis has improved the precision of cross-section and invariant-yield measurements in $p+p$ and $p+\text{Au}$ collisions, respectively, and consequently the $R_{p\text{Au}}$. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2604_22184 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Cold Nuclear Matter Effects on Inclusive $J/ψ$ Production in $p+\text{Au}$ Collisions at $\sqrt{s_\text{NN}}$ = 200 GeV with the STAR Experiment STAR Collaboration Nuclear Experiment In this paper, a study of cold nuclear matter (CNM) effects is reported based on the new STAR measurement of inclusive $J/ψ$ production in $p+p$ and $p+\text{Au}$ collisions at $\sqrt{s_\text{NN}}$ = 200 GeV, and a combined $J/ψ\rightarrow e^{+}e^{-}$ cross section in $p+p$ collisions at $\sqrt{s}$ = 200 GeV is provided. Given the long-established presumption that the energy density and the temperature produced in proton-nucleon collisions are insufficient to form QGP droplets, CNM effects in $p+\text{Au}$ collisions are quantified by the nuclear modification factor ($R_{p\text{Au}}$), defined as the ratio of the yield of the inclusive $J/ψ$ in $p+\text{Au}$ collisions to that in $p+p$ collisions, scaled by the average number of binary nucleon-nucleon collisions. The $R_{p\text{Au}}$ is derived as a function of transverse momentum ($p_\text{T}$) in the range 4--12 GeV/$c$ and is averaged within the rapidity ($y$) and azimuthal angle ($φ$) coverage of $|y|<1$, $0 \leq φ< 2π$. The result is consistent with unity, suggesting negligible modification of the yield by CNM effects in this kinematic region. Various model calculations are in agreement with the $R_{p\text{Au}}$ measurement, yet the same calculations are less satisfactory in describing the individual invariant yields from $p+p$ and $p+\text{Au}$ collisions. In the covered kinematic region, this analysis has improved the precision of cross-section and invariant-yield measurements in $p+p$ and $p+\text{Au}$ collisions, respectively, and consequently the $R_{p\text{Au}}$. |
| title | Cold Nuclear Matter Effects on Inclusive $J/ψ$ Production in $p+\text{Au}$ Collisions at $\sqrt{s_\text{NN}}$ = 200 GeV with the STAR Experiment |
| topic | Nuclear Experiment |
| url | https://arxiv.org/abs/2604.22184 |