Nuclear $\text{C}(e,e^{\prime }p)$ Transparencies in a Relativistic Glauber Model

Abstract

In light of the recent Jefferson Laboratory (JLab) data for the nuclear ${}^{12}\text{C}(e,e^{\prime }p)$ transparencies, calculations, obtained in a relativistic multiple scattering Glauber approximation, are discussed. The shell-separated ${}^{12}$C transparencies are shown and it is concluded that the $p$-shell nucleons are 75\% more transparent than the $s$-shell ones. The presented comparisons between the calculations made here and the current ${}^{12}\text{C}(e,e^{\prime }p)$ data show no clear indication for the onset of color transparency when implemented within the color diffusion model with standard parameters.

arXiv comment5 pages, 2 figures. Matches published version in Special Issue "The Future of Color Transparency, Hadronization and Short-Range Nucleon-Nucleon Correlation Studies". Based on a talk given at the workshop "The Future of Color Transparency and Hadronization Studies at Jefferson Lab and Beyond"

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Cited by in corpus (1)

• Searching for an Enhanced Signal of the onset of Color Transparency in Baryons with D(e,e'p)n scattering