Dispersive optical model analysis of 208Pb generating a neutron-skin prediction beyond the mean field
Abstract
In this work, a nonlocal dispersive optical model analysis is carried out for neutrons and protons in 208Pb. Elastic-scattering angular distributions, total and reaction cross sections, single-particle energies, neutron and proton numbers, the charge distribution, and the binding energy are fitted to extract the neutron and proton self-energies both above and below the Fermi energy. From the single-particle propagator derived from these self-energies, we determine the charge and matter distributions in 208Pb. The predicted spectroscopic factors are consistent with results from the ($$\textit{e,e}'\textit{p}$$) reaction and inelastic-electron-scattering data to very high-spin states. Sensible results for the high-momentum content of neutrons and protons are obtained, with protons appearing more correlated, in agreement with experiment and ab initio calculations of asymmetric matter. A neutron skin of 0.25 ± 0.05 fm is deduced. An analysis of several nuclei leads to the conclusion that finite-size effects play a nonnegligible role in the formation of the neutron skin in finite nuclei.
- Authors:
-
- TRIUMF, Vancouver, BC (Canada); Washington Univ., St. Louis, MO (United States)
- Washington Univ., St. Louis, MO (United States)
- Publication Date:
- Research Org.:
- Washington Univ., St. Louis, MO (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Nuclear Physics (NP); National Science Foundation (NSF)
- OSTI Identifier:
- 1800650
- Alternate Identifier(s):
- OSTI ID: 1632941
- Grant/Contract Number:
- FG02-87ER40316; PHY-1613362; PHY-1912643; FG02-87ER-40316
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review C
- Additional Journal Information:
- Journal Volume: 101; Journal Issue: 4; Journal ID: ISSN 2469-9985
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 73 NUCLEAR PHYSICS AND RADIATION PHYSICS; Physics
Citation Formats
Atkinson, M. C., Mahzoon, M. H., Keim, M. A., Bordelon, B. A., Pruitt, C. D., Charity, R. J., and Dickhoff, W. H. Dispersive optical model analysis of 208Pb generating a neutron-skin prediction beyond the mean field. United States: N. p., 2020.
Web. doi:10.1103/physrevc.101.044303.
Atkinson, M. C., Mahzoon, M. H., Keim, M. A., Bordelon, B. A., Pruitt, C. D., Charity, R. J., & Dickhoff, W. H. Dispersive optical model analysis of 208Pb generating a neutron-skin prediction beyond the mean field. United States. https://doi.org/10.1103/physrevc.101.044303
Atkinson, M. C., Mahzoon, M. H., Keim, M. A., Bordelon, B. A., Pruitt, C. D., Charity, R. J., and Dickhoff, W. H. Thu .
"Dispersive optical model analysis of 208Pb generating a neutron-skin prediction beyond the mean field". United States. https://doi.org/10.1103/physrevc.101.044303. https://www.osti.gov/servlets/purl/1800650.
@article{osti_1800650,
title = {Dispersive optical model analysis of 208Pb generating a neutron-skin prediction beyond the mean field},
author = {Atkinson, M. C. and Mahzoon, M. H. and Keim, M. A. and Bordelon, B. A. and Pruitt, C. D. and Charity, R. J. and Dickhoff, W. H.},
abstractNote = {In this work, a nonlocal dispersive optical model analysis is carried out for neutrons and protons in 208Pb. Elastic-scattering angular distributions, total and reaction cross sections, single-particle energies, neutron and proton numbers, the charge distribution, and the binding energy are fitted to extract the neutron and proton self-energies both above and below the Fermi energy. From the single-particle propagator derived from these self-energies, we determine the charge and matter distributions in 208Pb. The predicted spectroscopic factors are consistent with results from the ($\textit{e,e}'\textit{p}$) reaction and inelastic-electron-scattering data to very high-spin states. Sensible results for the high-momentum content of neutrons and protons are obtained, with protons appearing more correlated, in agreement with experiment and ab initio calculations of asymmetric matter. A neutron skin of 0.25 ± 0.05 fm is deduced. An analysis of several nuclei leads to the conclusion that finite-size effects play a nonnegligible role in the formation of the neutron skin in finite nuclei.},
doi = {10.1103/physrevc.101.044303},
journal = {Physical Review C},
number = 4,
volume = 101,
place = {United States},
year = {Thu Apr 09 00:00:00 EDT 2020},
month = {Thu Apr 09 00:00:00 EDT 2020}
}
Web of Science
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