Quenching of the quantum p-strength in light exotic nuclei

One-nucleon spectroscopic overlaps, their strength or spectroscopic factors (SFs), and nucleon removal cross sections for light nuclei in the mass range A≤12 were evaluated using the fully correlated Quantum Monte Carlo (QMC) wave functions (WFs). Harder (AV18+UX) and softer (NV2+3) bare interaction...

Full description

Saved in:
Bibliographic Details
Main Authors: E. Cravo, R.B. Wiringa, R. Crespo, A. Arriaga, A. Deltuva, M. Piarulli
Format: Article
Language:English
Published: Elsevier 2024-12-01
Series:Physics Letters B
Subjects:
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269324006452
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1850218925330006016
author E. Cravo
R.B. Wiringa
R. Crespo
A. Arriaga
A. Deltuva
M. Piarulli
author_facet E. Cravo
R.B. Wiringa
R. Crespo
A. Arriaga
A. Deltuva
M. Piarulli
author_sort E. Cravo
collection DOAJ
description One-nucleon spectroscopic overlaps, their strength or spectroscopic factors (SFs), and nucleon removal cross sections for light nuclei in the mass range A≤12 were evaluated using the fully correlated Quantum Monte Carlo (QMC) wave functions (WFs). Harder (AV18+UX) and softer (NV2+3) bare interactions were used providing consistent results. The SFs were also taken from simple Shell Model (SM) calculations. This structure information was incorporated in the standard three-body Faddeev/Alt-Grassberger-Sandhas reaction formalism to evaluate the (p,pN) cross sections. The results further our understanding of the quenching of the quantum p-shell strength obtained from structure and reactions. We have found the ratios of the total QMC sums of SFs to the SM ones to be uniform and ∼ 3/4. The corresponding ratios of the sums Below Particle Threshold (BPT) of SFs, as well as of total cross sections, deviate strikingly from the uniform trend in some special cases. We find these ratios to be close to unit for Li9→8Li+n and C9→8B+p. In contrast, they are strongly reduced for C11→10C+n and B11→10Be+p mirror transitions, resulting from the quenching of the strength for low-lying 2+ final state transitions. The QMC theoretical cross section BPT for C11(p,pn) is about two times smaller than the experimental data.
format Article
id doaj-art-bb65c276b0e8415eb49de02e387b4583
institution OA Journals
issn 0370-2693
language English
publishDate 2024-12-01
publisher Elsevier
record_format Article
series Physics Letters B
spelling doaj-art-bb65c276b0e8415eb49de02e387b45832025-08-20T02:07:34ZengElsevierPhysics Letters B0370-26932024-12-0185913908710.1016/j.physletb.2024.139087Quenching of the quantum p-strength in light exotic nucleiE. Cravo0R.B. Wiringa1R. Crespo2A. Arriaga3A. Deltuva4M. Piarulli5Centro de Física Teórica e Computacional, Faculdade de Ciências, Universidade de Lisboa, Campo Grande, 1749-016 Lisboa, Portugal; Departamento de Física, Faculdade de Ciências, Universidade de Lisboa, Campo Grande, 1749-016 Lisboa, PortugalPhysics Division, Argonne National Laboratory, Argonne, IL 60439, USADepartamento de Física, Instituto Superior Técnico, Universidade de Lisboa, Av. Rovisco Pais 1, 1049-001, Lisboa, Portugal; Centro de Ciências e Tecnologias Nucleares, Universidade de Lisboa, Estrada Nacional 10, 2695-066 Bobadela, Portugal; Corresponding author at: Departamento de Física, Instituto Superior Técnico, Universidade de Lisboa, Av. Rovisco Pais 1, 1049-001, Lisboa, Portugal.Departamento de Física, Faculdade de Ciências, Universidade de Lisboa, Campo Grande, 1749-016 Lisboa, PortugalInstitute of Theoretical Physics and Astronomy, Vilnius University, Saulėtekio al. 3, LT-10257 Vilnius, LithuaniaDepartment of Physics, Washington University in Saint Louis, Saint Louis, MO 63130, USA; McDonnell Center for the Space Sciences at Washington University in St. Louis, MO 63130, USAOne-nucleon spectroscopic overlaps, their strength or spectroscopic factors (SFs), and nucleon removal cross sections for light nuclei in the mass range A≤12 were evaluated using the fully correlated Quantum Monte Carlo (QMC) wave functions (WFs). Harder (AV18+UX) and softer (NV2+3) bare interactions were used providing consistent results. The SFs were also taken from simple Shell Model (SM) calculations. This structure information was incorporated in the standard three-body Faddeev/Alt-Grassberger-Sandhas reaction formalism to evaluate the (p,pN) cross sections. The results further our understanding of the quenching of the quantum p-shell strength obtained from structure and reactions. We have found the ratios of the total QMC sums of SFs to the SM ones to be uniform and ∼ 3/4. The corresponding ratios of the sums Below Particle Threshold (BPT) of SFs, as well as of total cross sections, deviate strikingly from the uniform trend in some special cases. We find these ratios to be close to unit for Li9→8Li+n and C9→8B+p. In contrast, they are strongly reduced for C11→10C+n and B11→10Be+p mirror transitions, resulting from the quenching of the strength for low-lying 2+ final state transitions. The QMC theoretical cross section BPT for C11(p,pn) is about two times smaller than the experimental data.http://www.sciencedirect.com/science/article/pii/S0370269324006452Many-body ab initio structureFew-body reaction(p,pN) reactions
spellingShingle E. Cravo
R.B. Wiringa
R. Crespo
A. Arriaga
A. Deltuva
M. Piarulli
Quenching of the quantum p-strength in light exotic nuclei
Physics Letters B
Many-body ab initio structure
Few-body reaction
(p,pN) reactions
title Quenching of the quantum p-strength in light exotic nuclei
title_full Quenching of the quantum p-strength in light exotic nuclei
title_fullStr Quenching of the quantum p-strength in light exotic nuclei
title_full_unstemmed Quenching of the quantum p-strength in light exotic nuclei
title_short Quenching of the quantum p-strength in light exotic nuclei
title_sort quenching of the quantum p strength in light exotic nuclei
topic Many-body ab initio structure
Few-body reaction
(p,pN) reactions
url http://www.sciencedirect.com/science/article/pii/S0370269324006452
work_keys_str_mv AT ecravo quenchingofthequantumpstrengthinlightexoticnuclei
AT rbwiringa quenchingofthequantumpstrengthinlightexoticnuclei
AT rcrespo quenchingofthequantumpstrengthinlightexoticnuclei
AT aarriaga quenchingofthequantumpstrengthinlightexoticnuclei
AT adeltuva quenchingofthequantumpstrengthinlightexoticnuclei
AT mpiarulli quenchingofthequantumpstrengthinlightexoticnuclei