Extraction of the Pomeron Trajectory from a Global Fit to Exclusive $\rho^0$ Meson Photoproduction Data

TL;DR

This paper analyzes elastic rho0 meson photoproduction data from multiple experiments to extract the pomeron trajectory parameters, providing insights into the nature of the pomeron in high-energy physics.

Contribution

It presents a comprehensive fit to experimental data to determine the pomeron trajectory's intercept and slope, comparing results with established models.

Findings

Extracted pomeron intercept: 1.0871 ± 0.0026 (stat.) ± 0.0030 (syst.)

Pomeron slope: 0.126 ± 0.013 (stat.) ± 0.012 (syst.) GeV^{-2}

Data compatible with Donnachie-Landshoff trajectory at low |t|

Abstract

Based on data on elastic $\rho^0$ photoproduction from the H1, Omega and ZEUS collaborations, a fit has been performed to extract the value $\alpha_P (t)$ of the pomeron trajectory at fixed values of t from the W dependence of the differential $\gamma p$ cross section $d \sigma_{\gamma p} (W) / d t$. The data used in the fit cover the range of $8.3 \le W \le 94 GeV$ in $\gamma p$ centre-of-mass energy and $0.01 \le |t| \le 0.95 GeV^2$ in momentum transfer. A linear fit to the resulting values of $\alpha_P (t)$ yields $\alpha_{P,0} =1.0871 \pm 0.0026 (stat.) \pm 0.0030 (syst.)$ for the intercept and $\alpha'_P = 0.126 \pm 0.013 (stat.) \pm 0.012 (syst.) GeV^{-2}$ for the slope of the pomeron trajectory. The data are also compatible with the Donnachie-Landshoff trajectory $\alpha_P (t) = 1.0808 + 0.25 GeV^{-2}\cdot t$ at low values $|t| \lesssim 0.3 GeV^2$ and with a constant value of $\alpha_P (t)$ at larger values of $|t|$.