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Title: Theory of nuclear fission

Abstract

Atomic nuclei are quantum many-body systems of protons and neutrons held together by strong nuclear forces. Under the proper conditions, nuclei can break into two (sometimes three) fragments which will subsequently decay by emitting particles. This phenomenon is called nuclear fission. Since different fission events may produce different fragmentations, the end-products of all fissions that occurred in a small chemical sample of matter comprise hundreds of different isotopes, including α particles, together with a large number of emitted neutrons, photons, electrons and antineutrinos. The extraordinary complexity of this process, which happens at length scales of the order of a femtometer, mostly takes less than a femtosecond but is not entirely over until all the lingering β decays have completed – which can take years – is a fascinating window into the physics of atomic nuclei. While fission may be more naturally known in the context of its technological applications, it also plays a crucial role in the synthesis of heavy elements in astrophysical environments. In both cases, simulations are needed for the many systems or energies inaccessible to experiments in the laboratory. In this context, the level of accuracy and precision required poses formidable challenges to nuclear theory. Overall, themore » goal of this article is to provide a comprehensive overview of the theoretical methods employed in the description of nuclear fission.« less

Authors:
ORCiD logo [1]; ORCiD logo [2]
  1. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
  2. Alternative Energies and Atomic Energy Commission (CEA, DAM, DIF), Arpajon (France); Univ. Paris-Saclay, Bruyères-le-Châtel (France)
Publication Date:
Research Org.:
Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
Sponsoring Org.:
USDOE National Nuclear Security Administration (NNSA)
OSTI Identifier:
1873225
Alternate Identifier(s):
OSTI ID: 1960974
Report Number(s):
LLNL-JRNL-830603
Journal ID: ISSN 0146-6410; 1046287; TRN: US2306983
Grant/Contract Number:  
AC52-07NA27344; SC0018223
Resource Type:
Accepted Manuscript
Journal Name:
Progress in Particle and Nuclear Physics
Additional Journal Information:
Journal Volume: 125; Journal ID: ISSN 0146-6410
Publisher:
Elsevier
Country of Publication:
United States
Language:
English
Subject:
73 NUCLEAR PHYSICS AND RADIATION PHYSICS; fission; fission fragment yields; cross sections; prompt fission spectrum; large-amplitude collective motion; energy density functional theory

Citation Formats

Schunck, Nicolas, and Regnier, David. Theory of nuclear fission. United States: N. p., 2022. Web. doi:10.1016/j.ppnp.2022.103963.
Schunck, Nicolas, & Regnier, David. Theory of nuclear fission. United States. https://doi.org/10.1016/j.ppnp.2022.103963
Schunck, Nicolas, and Regnier, David. Tue . "Theory of nuclear fission". United States. https://doi.org/10.1016/j.ppnp.2022.103963. https://www.osti.gov/servlets/purl/1873225.
@article{osti_1873225,
title = {Theory of nuclear fission},
author = {Schunck, Nicolas and Regnier, David},
abstractNote = {Atomic nuclei are quantum many-body systems of protons and neutrons held together by strong nuclear forces. Under the proper conditions, nuclei can break into two (sometimes three) fragments which will subsequently decay by emitting particles. This phenomenon is called nuclear fission. Since different fission events may produce different fragmentations, the end-products of all fissions that occurred in a small chemical sample of matter comprise hundreds of different isotopes, including α particles, together with a large number of emitted neutrons, photons, electrons and antineutrinos. The extraordinary complexity of this process, which happens at length scales of the order of a femtometer, mostly takes less than a femtosecond but is not entirely over until all the lingering β decays have completed – which can take years – is a fascinating window into the physics of atomic nuclei. While fission may be more naturally known in the context of its technological applications, it also plays a crucial role in the synthesis of heavy elements in astrophysical environments. In both cases, simulations are needed for the many systems or energies inaccessible to experiments in the laboratory. In this context, the level of accuracy and precision required poses formidable challenges to nuclear theory. Overall, the goal of this article is to provide a comprehensive overview of the theoretical methods employed in the description of nuclear fission.},
doi = {10.1016/j.ppnp.2022.103963},
journal = {Progress in Particle and Nuclear Physics},
number = ,
volume = 125,
place = {United States},
year = {Tue Apr 26 00:00:00 EDT 2022},
month = {Tue Apr 26 00:00:00 EDT 2022}
}

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