Impact of shell structure on the fusion of neutron-rich mid-mass nuclei
Abstract
The influence of shell effects on fusion of mid-mass nuclei is explored using isotopic chains of K and Ar ions on an oxygen target. Comparison of the reduced excitation functions reveals that the fusion cross section for the open neutron-shell projectile nuclei 41K and 45K is systematically larger than for the closed neutron-shell projectiles 39K and 47K. Furthermore, the São Paulo fusion model using matter densities from systematics fails to describe the measured excitation functions. Use of more realistic densities from a Dirac-Hartree-Bogoliubov (DHB) approach performs significantly better though it still overpredicts the closed-shell nuclei.
- Authors:
-
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- Indiana Univ., Bloomington, IN (United States)
- CEA/DRF-CNRS/IN2P3 (France)
- Normandie Univ., Caen (France)
- Texas A & M Univ., College Station, TX (United States)
- Western Michigan Univ., Kalamazoo MI (United States)
- Michigan State Univ., East Lansing, MI (United States)
- Univ. Federal Fluminense. Rio de Janeiro (Brazil)
- Technologico da Aeronautica, Sao Paulo (Brazil)
- Publication Date:
- Research Org.:
- Indiana Univ., Bloomington, IN (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1837518
- Alternate Identifier(s):
- OSTI ID: 1889084
- Grant/Contract Number:
- FG02-88ER40404
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review C
- Additional Journal Information:
- Journal Volume: 104; 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; Low & intermediate energy heavy-ion reactions; Models & methods for nuclear reactions; Nuclear fusion; Unstable nuclei induced nuclear reactions; 39 ≤ A ≤ 58; shell structure in nuclear reactions; heavy-ion fusion; neutron-rich fusion; low-energy fusion
Citation Formats
Singh, Varinderjit, Johnstone, J. E., Giri, R., Hudan, S., Vadas, J., deSouza, R. T., Ackermann, D., Chbihi, A., Hourdille, Q., Abbott, A., Balhoff, C., Hannaman, A., McIntosh, A. B., Sorensen, M., Tobin, Z., Wakhle, A., Yennello, S. J., Famiano, M. A., Brown, K. W., Santamaria, C., Lubian, J., Soler, H. O., and Carlson, B. V. Impact of shell structure on the fusion of neutron-rich mid-mass nuclei. United States: N. p., 2021.
Web. doi:10.1103/physrevc.104.l041601.
Singh, Varinderjit, Johnstone, J. E., Giri, R., Hudan, S., Vadas, J., deSouza, R. T., Ackermann, D., Chbihi, A., Hourdille, Q., Abbott, A., Balhoff, C., Hannaman, A., McIntosh, A. B., Sorensen, M., Tobin, Z., Wakhle, A., Yennello, S. J., Famiano, M. A., Brown, K. W., Santamaria, C., Lubian, J., Soler, H. O., & Carlson, B. V. Impact of shell structure on the fusion of neutron-rich mid-mass nuclei. United States. https://doi.org/10.1103/physrevc.104.l041601
Singh, Varinderjit, Johnstone, J. E., Giri, R., Hudan, S., Vadas, J., deSouza, R. T., Ackermann, D., Chbihi, A., Hourdille, Q., Abbott, A., Balhoff, C., Hannaman, A., McIntosh, A. B., Sorensen, M., Tobin, Z., Wakhle, A., Yennello, S. J., Famiano, M. A., Brown, K. W., Santamaria, C., Lubian, J., Soler, H. O., and Carlson, B. V. Wed .
"Impact of shell structure on the fusion of neutron-rich mid-mass nuclei". United States. https://doi.org/10.1103/physrevc.104.l041601. https://www.osti.gov/servlets/purl/1837518.
@article{osti_1837518,
title = {Impact of shell structure on the fusion of neutron-rich mid-mass nuclei},
author = {Singh, Varinderjit and Johnstone, J. E. and Giri, R. and Hudan, S. and Vadas, J. and deSouza, R. T. and Ackermann, D. and Chbihi, A. and Hourdille, Q. and Abbott, A. and Balhoff, C. and Hannaman, A. and McIntosh, A. B. and Sorensen, M. and Tobin, Z. and Wakhle, A. and Yennello, S. J. and Famiano, M. A. and Brown, K. W. and Santamaria, C. and Lubian, J. and Soler, H. O. and Carlson, B. V.},
abstractNote = {The influence of shell effects on fusion of mid-mass nuclei is explored using isotopic chains of K and Ar ions on an oxygen target. Comparison of the reduced excitation functions reveals that the fusion cross section for the open neutron-shell projectile nuclei 41K and 45K is systematically larger than for the closed neutron-shell projectiles 39K and 47K. Furthermore, the São Paulo fusion model using matter densities from systematics fails to describe the measured excitation functions. Use of more realistic densities from a Dirac-Hartree-Bogoliubov (DHB) approach performs significantly better though it still overpredicts the closed-shell nuclei.},
doi = {10.1103/physrevc.104.l041601},
journal = {Physical Review C},
number = 4,
volume = 104,
place = {United States},
year = {Wed Oct 13 00:00:00 EDT 2021},
month = {Wed Oct 13 00:00:00 EDT 2021}
}
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