Machine learning approach to pattern recognition in nuclear dynamics from the ab initio symmetry-adapted no-core shell model
Abstract
A novel machine learning approach is used to provide further insight into atomic nuclei and to detect orderly patterns amid a vast data of large-scale calculations. The method utilizes a neural network that is trained on ab initio results from the symmetry-adapted no-core shell model (SA-NCSM) for light nuclei. We show that the SA-NCSM, which expands ab initio applications up to medium-mass nuclei by using dominant symmetries of nuclear dynamics, can reach heavier nuclei when coupled with the machine learning approach. In particular, we find that a neural network trained on probability amplitudes for s- and p-shell nuclear wave functions not only predicts dominant configurations for heavier nuclei but in addition, when tested for the 20Ne ground state, accurately reproduces the probability distribution. The non-negligible configurations predicted by the network provide an important input to the SA-NCSM for reducing ultralarge model spaces to manageable sizes that can be, in turn, utilized in SA-NCSM calculations to obtain accurate observables. The neural network is capable of describing nuclear deformation and is used to track the shape evolution along the 20-42Mg isotopic chain, suggesting a shape coexistence that is more pronounced toward the very neutron-rich isotopes. We provide first descriptions of the structuremore »
- Authors:
-
- Louisiana State Univ., Baton Rouge, LA (United States)
- Louisiana State Univ., Baton Rouge, LA (United States); Yale Univ., New Haven, CT (United States). Sloane Physics Laboratory
- Louisiana State Univ., Baton Rouge, LA (United States); Academy of Sciences of the Czech Republic (Czech Republic)
- Publication Date:
- Research Org.:
- Yale Univ., New Haven, CT (United States); Univ. of California, Oakland, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC); National Science Foundation (NSF); Czech Science Foundation
- OSTI Identifier:
- 1979864
- Grant/Contract Number:
- SC0019521; AC02-05CH11231; PHY-1913728; 16-16772S; OAC-1818253
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review. C
- Additional Journal Information:
- Journal Volume: 105; Journal Issue: 3; 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; machine learning; nucleon distribution; ab initio calculations; shell model
Citation Formats
Molchanov, O. M., Launey, K. D., Mercenne, A., Sargsyan, G. H., Dytrych, T., and Draayer, J. P. Machine learning approach to pattern recognition in nuclear dynamics from the ab initio symmetry-adapted no-core shell model. United States: N. p., 2022.
Web. doi:10.1103/physrevc.105.034306.
Molchanov, O. M., Launey, K. D., Mercenne, A., Sargsyan, G. H., Dytrych, T., & Draayer, J. P. Machine learning approach to pattern recognition in nuclear dynamics from the ab initio symmetry-adapted no-core shell model. United States. https://doi.org/10.1103/physrevc.105.034306
Molchanov, O. M., Launey, K. D., Mercenne, A., Sargsyan, G. H., Dytrych, T., and Draayer, J. P. Thu .
"Machine learning approach to pattern recognition in nuclear dynamics from the ab initio symmetry-adapted no-core shell model". United States. https://doi.org/10.1103/physrevc.105.034306. https://www.osti.gov/servlets/purl/1979864.
@article{osti_1979864,
title = {Machine learning approach to pattern recognition in nuclear dynamics from the ab initio symmetry-adapted no-core shell model},
author = {Molchanov, O. M. and Launey, K. D. and Mercenne, A. and Sargsyan, G. H. and Dytrych, T. and Draayer, J. P.},
abstractNote = {A novel machine learning approach is used to provide further insight into atomic nuclei and to detect orderly patterns amid a vast data of large-scale calculations. The method utilizes a neural network that is trained on ab initio results from the symmetry-adapted no-core shell model (SA-NCSM) for light nuclei. We show that the SA-NCSM, which expands ab initio applications up to medium-mass nuclei by using dominant symmetries of nuclear dynamics, can reach heavier nuclei when coupled with the machine learning approach. In particular, we find that a neural network trained on probability amplitudes for s- and p-shell nuclear wave functions not only predicts dominant configurations for heavier nuclei but in addition, when tested for the 20Ne ground state, accurately reproduces the probability distribution. The non-negligible configurations predicted by the network provide an important input to the SA-NCSM for reducing ultralarge model spaces to manageable sizes that can be, in turn, utilized in SA-NCSM calculations to obtain accurate observables. The neural network is capable of describing nuclear deformation and is used to track the shape evolution along the 20-42Mg isotopic chain, suggesting a shape coexistence that is more pronounced toward the very neutron-rich isotopes. We provide first descriptions of the structure and deformation of 24Si and 40Mg of interest to x-ray burst nucleosynthesis, and even of the extremely heavy nuclei such as 166,168Er and 236U, that build on first-principles considerations.},
doi = {10.1103/physrevc.105.034306},
journal = {Physical Review. C},
number = 3,
volume = 105,
place = {United States},
year = {Thu Mar 03 00:00:00 EST 2022},
month = {Thu Mar 03 00:00:00 EST 2022}
}
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