PaperPanorama

Nuclear Theory·nucl-th

Friday·September 30, 2022

10 papers2 primary·8 cross-listed

  1. 01

    A novel Machine-Learning method for spin classification of neutron resonances

    G. P. A. Nobre · D. A. Brown · S. J. Hollick · S. Scoville · P. Rodríguez

    The performance of nuclear reactors and other nuclear systems depends on a precise understanding of the neutron interaction cross sections for materials used in these systems. These cross sections exhibit resonant structure whose shape is determined in part by the angular momentum quantum numbers of the resonances. The correct assignment of the quantum numbers of neutron resonances is, therefore, paramount. In this project, we apply machine learning to automate the quantum number assignments using only the resonances' energies and widths and not relying on detailed transmission or capture measurements. The classifier used for quantum number assignment is trained using stochastically generated resonance sequences whose distributions mimic those of real data. We explore the use of several physics-motivated features for training our classifier. These features amount to out-of-distribution tests of a given resonance's widths and resonance-pair spacings. We pay special attention to situations where either capture widths cannot be trusted for classification purposes or where there is insufficient information to classify resonances by the total spin . We demonstrate the efficacy of our classification approach using simulated and actual Cr resonance data.

    nucl-thPRC(2023)·10 citations
  2. 02

    The Nuclear Physics of Neutron Stars

    J. Piekarewicz🇺🇸

    Neutron stars -- compact objects with masses similar to that of our Sun but radii comparable to the size of a city -- contain the densest form of matter in the universe that can be probed in terrestrial laboratories as well as in earth- and space-based observatories. The historical detection of gravitational waves from a binary neutron star merger has opened the brand new era of multimessenger astronomy and has propelled neutron stars to the center of a variety of disciplines, such as astrophysics, general relativity, nuclear physics, and particle physics. The main input required to study the structure of neutron stars is the pressure support generated by its constituents against gravitational collapse. These include neutrons, protons, electrons, and perhaps even more exotic constituents. As such, nuclear physics plays a prominent role in elucidating the fascinating structure, dynamics, and composition of neutron stars.

    nucl-thastro-ph.HEnucl-ex14 citations

Affiliations

first authorsco-authorsvia INSPIRE