Search arXivSearch

arXiv · nucl-th/0411084

Modification of the pi-omega-rho vertex in nuclear medium and its influence on the dilepton production rate in relativistic heavy-ion collisions

Abstract

In this PhD thesis we analyze the medium modification of the pi-omega-rho coupling and subsequently discuss its possible influence on the dilepton production rate in relativistic heavy-ion collisions. The first part of the thesis is devoted to the medium modifications of the Dalitz decays from the omega and rho mesons in nuclear matter. We use the relativistic field theory formalism describing modifications of the coupling by one-loop Feynman diagrams with nucleons and Delta(1232) isobars. We consider cases when the decaying particle is at rest or at motion with respect to the medium. We investigate the dependence of medium effects on the dilepton invariant mass and observe a sizeable increase of the effective coupling constants compared to their vacuum values. The effect grows with density. In the second part of the thesis we apply our model to evaluate the influence of the medium effects on the dilepton production from the Dalitz decays. In the calculations of the dilepton spectrum we use the model of the hydrodynamic expansion of the fire cylinder. In our comparison to the CERES dilepton data we take into account the experimental cuts. The medium modifications enhance the effect of the Dalitz decays. It is worth to point out that in the medium the rho decay due to the isospin degeneracy becomes as important as the omega decay. The main new and original results of the thesis are: 1. Significant in-medium increase of the pi-omega-rho coupling constant. 2. Large enhancement of the Dalitz decays from the omega and rho mesons in the range 0.2-0.6 GeV of the dilepton invariant mass.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Agnieszka Bieniek. 2004-11-19. Modification of the pi-omega-rho vertex in nuclear medium and its influence on the dilepton production rate in relativistic heavy-ion collisions. https://arxiv.org/abs/nucl-th/0411084

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