Nuclear shadowing
N. Armesto
TL;DR
The article surveys nuclear shadowing at small x in deep-inelastic scattering, explaining it as a consequence of multiple scattering and reviewing three broad theoretical frameworks: Glauber-like rescatterings, Gribov inelastic shadowing, and high-density QCD. It contrasts these with DGLAP-based evolutions of nuclear parton distributions and analyzes how different models fare against available data on F2 and gluon densities, highlighting sizable uncertainties, especially for gluons at x < 0.02. The work emphasizes the relative strengths and limitations of each approach, showing that experimental constraints at very small x are still insufficient to discriminate models definitively. It also discusses the implications for high-energy nuclear collisions and the need for new data from future facilities, such as an Electron-Ion Collider or UPC measurements, to sharpen predictions and understand shadowing in nuclei.
Abstract
The phenomenon of shadowing of nuclear structure functions at small values of Bjorken-$x$ is analyzed. First, multiple scattering is discussed as the underlying physical mechanism. In this context three different but related approaches are presented: Glauber-like rescatterings, Gribov inelastic shadowing and ideas based on high-density Quantum Chromodynamics. Next, different parametrizations of nuclear partonic distributions based on fit analysis to existing data combined with Dokshitzer-Gribov-Lipatov-Altarelli-Parisi evolution, are reviewed. Finally, a comparison of the different approaches is shown, and a few phenomenological consequences of nuclear shadowing in high-energy nuclear collisions are presented.
