PaperPanorama

Nuclear Theory·nucl-th

Tuesday·November 8, 2022

14 papers7 primary·7 cross-listed

  1. 01

    Optimization of generator coordinate method with machine-learning techniques for nuclear spectra and neutrinoless double-beta decay: ridge regression for nuclei with axial deformation

    X. Zhang🇨🇳 · W. Lin🇨🇳 · J. M. Yao🇨🇳 · C. F. Jiao🇨🇳 · A. M. Romero🇺🇸 · T. R. Rodríguez🇪🇸 · H. Hergert🇺🇸

    The generator coordinate method (GCM) is an important tool of choice for modeling large-amplitude collective motion in atomic nuclei. The computational complexity of the GCM increases rapidly with the number of collective coordinates. It imposes a strong restriction on the applicability of the method. In this work, we propose a subspace-reduction algorithm that employs optimal statistical ML models as surrogates for exact quantum-number projection calculations for norm and Hamiltonian kernels. The model space of the original GCM is reduced to a subspace relevant for nuclear low energy spectra and the NME of ground state to ground state decay based on the orthogonality condition (OC) and the energy-transition-orthogonality procedure (ENTROP), respectively. For simplicity, the polynomial ridge regression (RR) algorithm is used to learn the norm and Hamiltonian kernels of axially deformed configurations. The efficiency and accuracy of this algorithm are illustrated for 76Ge and 76Se by comparing results obtained using the optimal RR models to direct GCM calculations. The low-lying energy spectra of Ge and Se, as well as the -decay NME between their ground states, are computed. The results show that the performance of the GCM+OC/ENTROP+RR is more robust than that of the GCM+RR alone, and the former can reproduce the results of the original GCM calculation accurately with a significantly reduced computational cost.

    nucl-thnucl-exPRC(2023)·11 citations
  2. 02

    Boost invariant spin hydrodynamics within the first order in derivative expansion

    Rajesh Biswas🇮🇳 · Asaad Daher🇵🇱 · Arpan Das🇵🇱 · Wojciech Florkowski🇵🇱 · Radoslaw Ryblewski🇵🇱

    Boost-invariant equations of spin hydrodynamics confined to the first-order terms in gradients are numerically solved. The spin equation of state, relating the spin density tensor to the spin chemical potential, is consistently included in the first order. Depending on its form and the structure of the spin transport coefficients, we find solutions which are both stable and unstable within the considered evolution times of 10 fm/c. These findings are complementary to the recent identification of stable and unstable modes for perturbed uniform spin systems described by similar hydrodynamic frameworks.

    nucl-thhep-phPRD(2023)·27 citations
  3. 03

    Comparative analysis of formalisms and performances of three different beyond mean-field approaches

    František Knapp · Panagiota Papakonstantinou · Petr Veselý · Giovanni De Gregorio · Jakub Herko · Nicola Lo Iudice

    We investigate the differences and analogies between the equation of motion phonon method (EMPM) and second Tamm-Dancoff and random-phase approximations (STDA and SRPA) paying special attention to the problem of spurious center-of-mass (c.m.) admixtures. In order to compare them on an equal footing, we perform self-consistent calculations of the multipole strength distributions in selected doubly magic nuclei within a space including up to two-particle-two-hole (2p-2h) basis states using the UCOM two-body intrinsic Hamiltonian and we explore the tools each approach supplies for removing the spurious c.m. admixtures. We find that the EMPM and STDA yield exactly the same results when the same intrinsic Hamiltonian is used and the coupling of the Hartree-Fock state with the 2p-2h space is neglected, but, unlike STDA and SRPA, the EMPM offers the possibility to completely remove c.m. admixtures.

    nucl-thPRC(2023)·14 citations
  4. 04

    Neutron density fluctuation and neutron-proton correlation from AMPT model

    Zuman Zhang🇨🇳 · Ning Yu🇨🇳 · Hongge Xu🇨🇳

    Using the multiphase transport (AMPT) model, we study the relative neutron density fluctuation and neutron-proton correlation in matter produced by Au+Au collisions at 7.7-200 GeV. The rapidity, centrality, and energy dependence of these two observations are also discussed. The light nuclei yield ratio of proton, deuteron, and triton calculated directly from the relative neutron density fluctuation and neutron-proton correlation, decreases with rapidity coverage and increases with collision centrality. Our study also found that the ratio does not exhibit any non-monotonic behavior in collision energy dependence. Since there is no first-order phase transition or critical physics in the AMPT model, our work provides a reference for extracting the relative neutron density fluctuation from light nuclei production in experiments.

    nucl-thEPJA(2022)·5 citations
  5. 05

    Progress on Brussels-Skyrme atomic mass models on a grid: stiff neutron matter equation of state

    Guilherme Grams · Wouter Ryssens · Guillaume Scamps · Stephane Goriely · Nicolas Chamel

    We report here the current developments on the Brussels-Skyrme-on-a-Grid (BSkG) atomic mass models. In comparison with our previous models, BSkG3 improves the infinite nuclear matter (INM) properties which opens its applications to neutron stars. The results presented here show that BSkG3 preserve the excellent agreement with experimental nuclear masses and radii, together with fission barriers of actinides obtained by BSkG1 and BSkG2, while the nuclear matter properties are considerably improved.

    nucl-thJ.Phys.Conf.Ser.(2023)·0 citations
  6. 06

    The mass of odd-odd nuclei in microscopic mass models

    W. Ryssens🇧🇪 · G. Scamps🇺🇸 · G. Grams🇧🇪 · I. Kullmann🇧🇪 · M. Bender🇫🇷 · S. Goriely🇧🇪

    Accurate estimates of the binding energy of nuclei far from stability that cannot be produced in the laboratory are crucial to our understanding of nuclear processes in astrophysical scenarios. Models based on energy density functionals have shown that they are capable of reproducing all known masses with root-mean-square error better than 800 keV, while retaining a firm microscopic foundation. However, it was recently pointed out in [M. Hukkanen et al., arXiv:2210.10674] that the recent BSkG1 model fails to account for a contribution to the binding energy that is specific to odd-odd nuclei, and which can be studied by using appropriate mass difference formulas. We analyse here the (lacking) performance of three recent microscopic mass models with respect to such formulas and examine possibilities to remedy this deficiency in the future.

    nucl-thJ.Phys.Conf.Ser.(2023)·4 citations
  7. 07

    Two-neutrino decay of Xe to the first excited state in Ba

    Lotta Jokiniemi🇨🇦 · Beatriz Romeo🇪🇸 · Catharina Brase🇩🇪 · Jenni Kotila🇫🇮 · Pablo Soriano🇪🇸 · Achim Schwenk🇩🇪 · Javier Menéndez🇪🇸

    We calculate the nuclear matrix element for the two-neutrino decay of Xe into the first excited state of Ba. We use different many-body methods: the quasiparticle random-phase approximation (QRPA) framework, the nuclear shell model, the interacting boson model (IBM-2), and an effective field theory (EFT) for and decays. While the QRPA suggests a decay rate at the edge of current experimental limits, the shell model points to a half-life about two orders of magnitude longer. The predictions of the IBM-2 and the EFT lie in between, and the latter provides systematic uncertainties at leading order. An analysis of the running sum of the nuclear matrix element indicates that subtle cancellations between the contributions of intermediate states can explain the different theoretical predictions. For the EFT, we also present results for two-neutrino decays to the first excited state in other nuclei.

    nucl-thhep-exhep-phnucl-exPLB(2023)·15 citations

Affiliations

first authorsco-authorsvia INSPIRE