Exploration on $1n$ halo nucleus $^{19}$C from D-RHFB structure to reaction observables

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Hauptverfasser: An, Jia-Lin, Lu, Qi, Long, Wen Hui, Zhang, Shi-Sheng
Format: Preprint
Veröffentlicht: 2024
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author An, Jia-Lin
Lu, Qi
Long, Wen Hui
Zhang, Shi-Sheng
author_facet An, Jia-Lin
Lu, Qi
Long, Wen Hui
Zhang, Shi-Sheng
contents We utilize the axially deformed relativistic Hartree-Fock-Bogoliubov (D-RHFB) model to describe the structure of neutron-rich carbon isotopes, taking into account the continuum, pairing correlations, tensor force and their interplay. In this scheme, one- and two-neutron separation energies of neutron-rich carbon isotopes agree well with measured data, as well as the spin and parity $J^π=1/2^+$ for the ground state of $^{19}$C, which is a long-standing problem for theoretical structure models. With the structure input extracted from the microscopic D-RHFB model, the reaction observables are well described the Glauber model. In particular, this unified approach accurately reproduces the inclusive longitudinal momentum distributions of the breakup reaction $^{19}$C + $^{12}$C at 240 MeV/nucleon, which rule out the possibility of the ground state of $^{19}$C being $J^π=3/2^+$. Moreover, the continuum plays a crucial role in the formation of the halo, which is further confirmed by the reaction cross sections and longitudinal momentum distributions. However, the tensor force components carried by the $π$-coupling are not as significant as anticipated. Consequently, the D-RHFB + Glauber approach turns out to be a promising tool to search for halo candidates from the structure to the reaction.
format Preprint
id arxiv_https___arxiv_org_abs_2406_09766
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Exploration on $1n$ halo nucleus $^{19}$C from D-RHFB structure to reaction observables
An, Jia-Lin
Lu, Qi
Long, Wen Hui
Zhang, Shi-Sheng
Nuclear Theory
We utilize the axially deformed relativistic Hartree-Fock-Bogoliubov (D-RHFB) model to describe the structure of neutron-rich carbon isotopes, taking into account the continuum, pairing correlations, tensor force and their interplay. In this scheme, one- and two-neutron separation energies of neutron-rich carbon isotopes agree well with measured data, as well as the spin and parity $J^π=1/2^+$ for the ground state of $^{19}$C, which is a long-standing problem for theoretical structure models. With the structure input extracted from the microscopic D-RHFB model, the reaction observables are well described the Glauber model. In particular, this unified approach accurately reproduces the inclusive longitudinal momentum distributions of the breakup reaction $^{19}$C + $^{12}$C at 240 MeV/nucleon, which rule out the possibility of the ground state of $^{19}$C being $J^π=3/2^+$. Moreover, the continuum plays a crucial role in the formation of the halo, which is further confirmed by the reaction cross sections and longitudinal momentum distributions. However, the tensor force components carried by the $π$-coupling are not as significant as anticipated. Consequently, the D-RHFB + Glauber approach turns out to be a promising tool to search for halo candidates from the structure to the reaction.
title Exploration on $1n$ halo nucleus $^{19}$C from D-RHFB structure to reaction observables
topic Nuclear Theory
url https://arxiv.org/abs/2406.09766