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
  8. 08

    The Electron-Ion Collider -- A U.S. facility for the European community to explore the mysteries of the building blocks of matter

    Marco Radici🇮🇹 · Silvia Dalla Torre🇮🇹 · Daria Sokhan🇫🇷

    This document is submitted as input to the NuPECC Long Range Plan 2024 by three European members of the EIC Users Group Steering Committee (Vice Chair, one at-large member, and the EU Representative). We submit the document on behalf of the international EIC Users Group (EICUG) community, but we specifically represent 335 European members of the EICUG (25%) based in 80 institutions (30% of the total) located in Armenia, Czech Republic, Finland, France, Germany, Hungary, Ireland, Israel, Italy, Netherlands, Norway, Poland, Slovenia, Spain, Sweden, Switzerland, Ukraine, and the United Kingdom. This European involvement is an important driver of the EIC, but can also be beneficial for a number of related ongoing and planned nuclear physics experiments in Europe. In this document, the shared interest regarding scientific questions and detector R&D between the EIC and European nuclear physics communities is outlined. The aim is to highlight how these synergies offer ample opportunities to foster progress at the forefront of nuclear physics.

    hep-phhep-exnucl-exnucl-th1 citation
  9. 09

    Isoscaling in central Sn+Sn collisions at 270 MeV/u

    J.W. Lee (1)🇰🇷 · M.B. Tsang (2 and 3)🇺🇸 · C.Y. Tsang (2 and 3)🇺🇸 · R. Wang (2)🇺🇸 · J. Barney (2 and 3)🇺🇸 · J. Estee (2 and 3)🇺🇸 · T. Isobe (4)🇯🇵 · M. Kaneko (4 and 5)🇯🇵 · M. Kurata-Nishimura (4)🇯🇵 · W.G. Lynch (2 and 3)🇺🇸 · T. Murakami (e6 and 4 and 5)🇯🇵 · A. Ono (6)🇯🇵 and 52 other authors

    Experimental information on fragment emissions is important in understanding the dynamics of nuclear collisions and in the development of transport model simulating heavy-ion collisions. The composition of complex fragments emitted in the heavy-ion collisions can be explained by statistical models, which assume that thermal equilibrium is achieved at collision energies below 100 MeV/u. Our new experimental data together with theoretical analyses for light particles from Sn+Sn collisions at 270 MeV/u, suggest that the hypothesis of thermal equilibrium breaks down for particles emitted with high transfer momentum. To inspect the system's properties in such limit, the scaling features of the yield ratios of particles from two systems, a neutron-rich system of and a nearly symmetric system of , are examined in the framework of the statistical multifragmentation model and the antisymmetrized molecular dynamics model. The isoscaling from low energy particles agree with both models. However the observed breakdown of isoscaling for particles with high transverse momentum cannot be explained by the antisymmetrized molecular dynamics model.

    nucl-exnucl-thEPJA(2022)·15 citations
  10. 10

    State-Specific Configuration Interaction for Excited States

    Fábris Kossoski · Pierre-François Loos

    We introduce and benchmark a systematically improvable route for excited-state calculations, state-specific configuration interaction (CI), \alert{which is a particular realization of multiconfigurational self-consistent field and multireference configuration interaction.} Starting with a reference built from optimized configuration state functions, separate CI calculations are performed for each targeted state (hence state-specific orbitals and determinants). Accounting for single and double excitations produces the CISD model, which can be improved with second-order Epstein-Nesbet perturbation theory (CISD+EN2) or a posteriori Davidson corrections (CISD+Q). These models were gauged against a vast and diverse set of 294 reference excitation energies. We have found that CI is significantly more accurate than standard ground-state-based CI, whereas close performances were found between CISD and EOM-CC2, and between CISD+EN2 and EOM-CCSD. For larger systems, CISD+Q delivers more accurate results than EOM-CC2 and EOM-CCSD. The CI route can handle challenging multireference problems, singly- and doubly-excited states, from closed- and open-shell species, with overall comparable accuracy, and thus represents a promising alternative to more established methodologies. In its current form, however, it is only reliable for relatively low-lying excited states.

    physics.chem-phcond-mat.mtrl-scicond-mat.str-elnucl-thJ.Chem.Theor.Comput.(2023)·7 citations
  11. 11

    Space-time variation of the s and c quark masses

    V.V. Flambaum🇦🇺 · P. Munro-Laylim🇦🇺

    Space-time variation of fundamental physical constants in expanding Universe is predicted by a number of popular models. The masses of second generation quarks are larger than first generation quark masses by several orders of magnitude, therefore space-time variation in quark masses may significantly vary between each generation. We evaluate limits on variation in the s and c quark masses from Big Bang nucleosynthesis, Oklo natural nuclear reactor, Yb+, Cs and Rb clock data. The construction of 229Th nuclear clock is expected to enhance these limits by several orders of magnitude. Furthermore, constraints are obtained on an oscillating scalar or pseudoscalar cold dark matter field, as interactions of the field with quarks produce variations in quark masses.

    hep-phastro-ph.COnucl-thphysics.atom-phPRD(2023)·6 citations
  12. 12

    Proton structure functions at NLO in the dipole picture with massive quarks

    Henri Hänninen🇫🇮 · Heikki Mäntysaari🇫🇮 · Risto Paatelainen🇫🇮 · Jani Penttala🇫🇮

    We predict heavy quark production cross sections in Deep Inelastic Scattering at high energy by applying the Color Glass Condensate effective theory. We demonstrate that when the calculation is performed consistently at next-to-leading order accuracy with massive quarks it becomes possible, for the first time in the dipole picture with perturbatively calculated center-of-mass energy evolution, to simultaneously describe both light and heavy quark production data at small . We furthermore show how the heavy quark cross section data provides additional strong constraints on the extracted non-perturbative initial condition for the small- evolution equations.

    hep-phnucl-thPRL(2023)·41 citations
  13. 13

    A coupled-channel system with anomalous thresholds and unitarity

    Csaba L. Korpa🇭🇺 · Matthias F.M. Lutz🇩🇪 · Xiao-Yu Guo🇨🇳 · Yonggoo Heo🇩🇪

    We consider the isospin one-half example system, with coupled channels in the partial wave, chosen such that various phenomena that come with the opening of an anomalous threshold can be illustrated in a step-wise procedure by a suitable variation of up, down and strange quark masses. We use a set of LEC in the chiral Lagrangian that were adjusted to a large set of Lattice QCD results. The six phase shifts and inelasticity parameters are presented for various choices of the pion mass. For a pion mass of 150 MeV there are no anomalous thresholds encountered. The small change from 150 MeV to 145 MeV pion mass causes a dramatic impact of the anomalous threshold on the phase shifts.

    hep-phhep-latnucl-thPRD(2023)·10 citations
  14. 14

    Counting States: A Combinatorial Analysis of SQM Fragmentation

    A. Bernardo · L. Paulucci · L. M. de Sá · J. E. Horvath

    The Strange Quark matter (SQM) hypothesis states that at extreme pressure and density conditions a new ground state of matter would arise, in which half of the \textit{down} quarks become strange quarks. If true, it would mean that at least the core of neutron stars is made of SQM. In this hypothesis, SQM would be released in the inter-stellar medium when two of these objects merge. It is estimated that of SQM would be released this way. This matter will undergo a sequence of processes that should result in a fraction of the released SQM becoming heavy nuclei through \textit{r-process}. In this work we are interested in characterizing the fragmentation of SQM, with the novelty of keeping track of the \textit{quark configuration} of the fragmented matter. This is accomplished by developing a methodology to estimate the energy of each fragment as the sum of its \textit{constituent quarks}, the Coulomb interaction among the quarks and fragments' momenta. The determination of the fragmentation output is crucial to fully characterize the subsequent nucleosynthesis.

    astro-ph.HEnucl-thAstron.Nachr.(2023)·0 citations

Affiliations

first authorsco-authorsvia INSPIRE