Search arXivSearch

arXiv · 1910.12553

Pion exchange interaction in the $γp \to p e^+e^-$ reaction

Abstract

The $ρ^0-ω$ interference has been studied in the dilepton invariant mass distribution spectra in the photonuclear reaction, but that is not done for the gamma-nucleon reaction. Recent past, the $e^+e^-$ invariant mass distribution spectrum in the $γp$ reaction, i.e., $γp \to pe^+e^-$ reaction, was measured at Jefferson Laboratory to look for the $ρ^0 -ω$ interference in the multi-GeV region. To study the mechanism of this reaction, the differential cross section of the $e^+e^-$ invariant mass distribution is calculated in the quoted energy region. The reaction is assumed to proceed as $γp \to Vp$; $V \to e^+e^-$, where $V$ denotes a vector meson, i.e., either $ρ^0$ or $ω$ meson. The photoproduction of the vector meson is described by the Vector Meson Dominance (VMD) model which consists of diagonal and off-diagonal processes. The diagonal process is described as $γ\to V; ~Vp \to Vp$. The low energy $ω$ meson photoproduction data is well described by the off-diagonal process which is illustrated as $γ\to ρ^0; ~ρ^0 p \to ωp$. The reaction $ρ^0p \to ωp$ proceeds due to one pion exchange interaction. The differential cross sections of the $γp \to pe^+e^-$ reaction due to the above processes of VMD model are compared, and the significance of the pion exchange interaction is investigated in the energy region of $γ$ beam available at Jefferson Laboratory.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Swapan Das. 2019-10-28. Pion exchange interaction in the $γp \to p e^+e^-$ reaction. https://doi.org/10.1142/s021830131850057x

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Application of the Skyrme Hartree-Fock-Bogoliubov Theory to WIMP-Nucleus Interactions in 40Ar

WIMP scattering from 40Ar is investigated using a self-consistent Skyrme Hartree-Fock-Bogoliubov (HFB) approach. Nuclear form factors relevant to dark matter direct detection are calculated from the resulting one-body density matrix elements and compared with shell-model predictions. Good agreement is found for the spin-independent response, while significant differences are observed for the spin-orbit response due to variations in single-particle occupancies. The effects of particle-number projection are shown to be small for 40Ar. These results demonstrate the sensitivity of certain dark matter response channels to the underlying nuclear structure model and establish a framework for extending mean-field calculations to nuclei beyond the reach of large-scale shell-model studies.

nucl-th

Breakdown of the Plane-Wave Trojan Horse Analysis of the $^{12}\mathrm{C}+{}^{12}\mathrm{C}$ Fusion Reaction: Critical Role of Coulomb Distortions

Recently, a new Trojan Horse Method (THM) measurement of carbon-carbon fusion was reported by Li \textit{et al.} [Phys. Lett. B (2026) 140675]. The purpose of the present work is to demonstrate the breakdown of the plane-wave approximation used in the analysis of these data and the critical role of Coulomb distortions in the initial and final states. The reaction mechanism underlying the THM analysis of the $^{12}\mathrm{C}+{}^{12}\mathrm{C}$ fusion reaction using the $^{16}\mathrm{O}+{}^{12}\mathrm{C}\to α_s+α+{}^{20}\mathrm{Ne}$ reaction is investigated. Particular attention is paid to the spectator momentum distribution and to the dependence of the THM reaction amplitude on the relative carbon-carbon energy $E$. It is demonstrated that agreement with the measured spectator momentum distribution does not by itself validate the plane-wave approximation. Although the experimental momentum distribution can be reproduced, inclusion of Coulomb distortions in both the initial and final channels leads to an energy dependence of the THM amplitude that is completely different from the plane-wave result. Consequently, the energy dependence of the $^{12}\mathrm{C}+{}^{12}\mathrm{C}$ fusion cross section extracted from the THM data can be strongly distorted by the plane-wave treatment. It is concluded that the astrophysical factor extracted in the plane-wave analysis cannot be regarded as reliable and may lead to misleading conclusions concerning the low-energy $^{12}\mathrm{C}+{}^{12}\mathrm{C}$ fusion reaction.

nucl-th