Search arXivSearch

arXiv · 2409.15018

Microscopic Study of Spin Transfer in Near-Barrier Nuclear Reactions

Abstract

In quasi-fission, it is unclear what the interaction between the relative orbital angular momentum and the spin of the fragments is from a microscopic perspective. In macroscopic approaches, it is expected that the large value of the relative orbital angular momentum, of the order of 100~$\hbar$ is transferred through tangential dissipation to the fragments' intrinsic spin by sliding and rolling friction. The goal is to investigate the angular momentum transfer from the initial relative orbital angular momentum to the fragments' spin. How is the transferred spin shared between the fragments? What is the time scale associated with the different mechanisms? How does deformation play a role? A TDDFT simulation in the TDHF-Skyrme framework is used to describe several reactions at different impact parameters with increasing complexity. A method is proposed to study the evolution of the fragments' total spin as a function of time and angular velocity. The increasingly complex reaction allows for careful analysis of all the mechanisms responsible for the transfer of spin. In particular, it is shown that the transfer of nucleons, and neck formation can significantly affect the transfer of spin through tangential friction. Several mechanisms are in contradiction with previous macroscopic calculations. In particular, the spin of the fragments does not always increase during the collision which prevents it from being used to estimate the collision time of the reaction.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Guillaume Scamps. 2024-11-18. Microscopic Study of Spin Transfer in Near-Barrier Nuclear Reactions. https://doi.org/10.1103/physrevc.110.054605

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