PaperPanorama

Nuclear Theory·nucl-th

Tuesday·May 9, 2023

8 papers2 primary·6 cross-listed

  1. 01

    Predicting nuclear masses with product-unit networks

    Babette Dellen · Uwe Jaekel · Paulo S.A. Freitas · John W. Clark

    Accurate estimation of nuclear masses and their prediction beyond the experimentally explored domains of the nuclear landscape are crucial to an understanding of the fundamental origin of nuclear properties and to many applications of nuclear science, most notably in quantifying the -process of stellar nucleosynthesis. Neural networks have been applied with some success to the prediction of nuclear masses, but they are known to have shortcomings in application to extrapolation tasks. In this work, we propose and explore a novel type of neural network for mass prediction in which the usual neuron-like processing units are replaced by complex-valued product units that permit multiplicative couplings of inputs to be learned from the input data. This generalized network model is tested on both interpolation and extrapolation data sets drawn from the Atomic Mass Evaluation. Its performance is compared with that of several neural-network architectures, substantiating its suitability for nuclear mass prediction. Additionally, a prediction-uncertainty measure for such complex-valued networks is proposed that serves to identify regions of expected low prediction error.

    nucl-thcs.LGPLB(2024)·8 citations
  2. 02

    Dense Baryonic Matter Predicted in "Pseudo-Conformal Model"

    Mannque Rho🇫🇷

    The World-Class University/Hanyang Project launched in Korea in 2007 led to what's now called ``pseudo-conformal model" that addresses dense compact-star matter and is confronted in this short note with the presently available astrophysical observables, with focus on those from gravity waves. The predictions made nearly free of parameters by the model involving ``topology change" remain more or less intact ``un-torpedoed" by the data.

    nucl-thhep-phSymmetry(2023)·9 citations
  3. 03

    Strong-Field Physics in QED and QCD: From Fundamentals to Applications

    Koichi Hattori🇨🇳 · Kazunori Itakura🇯🇵 · Sho Ozaki🇯🇵

    We provide a pedagogical review article on fundamentals and applications of the quantum dynamics in strong electromagnetic fields in QED and QCD. The fundamentals include the basic picture of the Landau quantization and the resummation techniques applied to the class of higher-order diagrams that are enhanced by large magnitudes of the external fields. We then discuss observable effects of the vacuum fluctuations in the presence of the strong fields, which consist of the interdisciplinary research field of nonlinear QED. We also discuss extensions of the Heisenberg-Euler effective theory to finite temperature/density and to non-Abelian theories with some applications. Next, we proceed to the paradigm of the dimensional reduction emerging in the low-energy dynamics in the strong magnetic fields. The mechanisms of superconductivity, the magnetic catalysis of the chiral symmetry breaking, and the Kondo effect are addressed from a unified point of view in terms of the renormalization-group method. We provide an up-to-date summary of the lattice QCD simulations in magnetic fields for the chiral symmetry breaking and the related topics as of the end of 2022. Finally, we discuss novel transport phenomena induced by chiral anomaly and the axial-charge dynamics. Those discussions are supported by a number of appendices.

    hep-phastro-ph.HEcond-mat.str-elhep-lat+1PPNP(2023)·67 citations
  4. 04

    decaying to and

    Brenda B. Malabarba🇧🇷 · K. P. Khemchandani🇧🇷 · A. Martinez Torres🇧🇷

    In this work we calculate the decay widths of to and by considering as a state, with clustering as . These decay widths have been recently determined by the BESIII, BaBar and Belle collaborations with the aim of unraveling the nature of . By analyzing the data on the cross sections of the process , two solutions were found by the BESIII collaboration with the same , mass and width for . However, different values for were obtained: eV (solution I) and eV (solution II). In case of , a value of was determined by the BESIII collaboration from fits to the data on the cross section of . The Belle collaboration has also determined more recently, although the statistical significance related to the signal of in the data is low. We calculate the decay widths of to and , and compare their ratio with the one determined by using the above mentioned experimental data. Considering the theoretical and experimental uncertainties, the lower limit of our theoretical result () is close to the upper value obtained () by using the solution II of BESIII for , as well as to the upper limit found () when considering the solutions III and IV of the Belle collaboration for .

    hep-phnucl-thPRD(2023)·11 citations
  5. 05

    Relativistic Bulk Rheology: From Neutron Star Mergers to Viscous Cosmology

    Lorenzo Gavassino · Jorge Noronha

    We develop the first causal and stable theory of a bulk-viscous relativistic pseudoplastic (or dilatant) fluid. This new formalism brings to light the rheological properties of several relativistic physical systems. Neutron star collisions can behave as a relativistic pseudoplastic material with viscous properties dictated by the non-conservation of lepton currents due to weak decay. Two-temperature relativistic plasmas, such as those surrounding supermassive galactic black holes, are predominantly pseudoplastic. Our framework can also be employed to construct novel viscous models for the evolution of the Universe with pseudoplastic or dilatant features.

    gr-qcnucl-thPRD(2024)·43 citations
  6. 06

    Double DVCS as a window to the complete mapping of GPDs

    K. Deja🇵🇱 · V. Martinez-Fernandez🇵🇱 · B. Pire🇫🇷 · P. Sznajder🇵🇱 · J. Wagner🇵🇱

    Double deeply virtual Compton scattering (DDVCS) is the process where an electron scatters off a nucleon and produces a lepton pair. The main advantage of this process in contrast with deeply virtual and timelike Compton scatterings (DVCS and TCS) is the possibility of directly measuring GPDs for at leading order in (LO). We present a new calculation of the DDVCS amplitude based on spinor techniques which produce expressions for amplitudes that are perfectly suited for their implementation in numerical simulations. Elements of impact studies, including predictions for experiments at JLab12, JLab20+ and the Electron-Ion Collider (EIC), are studied by means of the PARTONS software and the EpIC Monte Carlo event generator.

    hep-phhep-exnucl-exnucl-th2 citations
  7. 07

    Threshold resummation for computing large- parton distribution through large-momentum effective theory

    Xiangdong Ji🇺🇸 · Yizhuang Liu🇵🇱 · Yushan Su🇺🇸

    Parton distribution functions (PDFs) at large are poorly constrained by high-energy experimental data, but extremely important for probing physics beyond standard model at colliders. We study the calculation of PDFs at large- through large-momentum expansion of the lattice quasi PDFs. Similar to deep-inelastic scattering, there are two distinct perturbative scales in the threshold limit where the matching coefficient can be factorized into a space-like jet function at scale and a pair of heavy-light Sudakov form factors at scale . The matching formula allows us to derive a full renormalization group resummation of large threshold logarithms, and the result is consistent with the known calculation to the next-to-next to leading order (NNLO). This paves the way for direct large- PDFs calculations in lattice QCD. As by-products, we find that the space-like jet function is related to a time-like version calculated previously through analytic continuation, and the heavy-light Sudakov form factor, calculated here to NNLO, is a universal object appearing as well in the large momentum expansion of quasi transverse-momentum-dependent PDFs and quasi wave-function amplitudes.

    hep-phhep-lathep-thnucl-thJHEP(2023)·40 citations
  8. 08

    Stability of interlinked neutron vortex and proton flux-tube arrays in a neutron star -- III. Proton feedback

    K. H. Thong · A. Melatos · L. V. Drummond

    The coupled, time-dependent Gross-Pitaevskii and Ginzburg-Landau equations are solved simultaneously in three dimensions to investigate the equilibrium state and far-from-equilibrium, spin-down dynamics of an interpenetrating neutron superfluid and proton type-II superconductor, as an idealized description of the outer core of a neutron star. The simulations generalize previous calculations without the time-dependent Ginzburg-Landau equation, where proton feedback is absent. If the angle between the rotation and magnetic axes does not equal zero, the equilibrium state consists of geometrically complicated neutron vortex and proton flux-tube tangles, as the topological defects pin to one another locally but align with different axes globally. During spin-down, new types of motion are observed. For , entire vortices pair rectilinearly with flux tubes and move together while pinned. For , vortex segments pair with segments from one or more flux tubes, and the paired segments move together while pinned. The degree to which proton feedback impedes the deceleration of the crust is evaluated as a function of and the pinning strength, . Key geometric properties of vortex-flux-tube tangles, such as filament length, mean curvature, and polarity are analysed. It is found that proton feedback smooths the deceleration of the crust, reduces the rotational glitch sizes, and stabilizes the vortex tangle dynamics. The dimensionless control parameters in the simulations are mutually ordered to match what is expected in a real neutron star, but their central values and dynamics ranges differ from reality by many orders of magnitude due to computational limitations.

    astro-ph.HEcond-mat.quant-gascond-mat.supr-connucl-thMNRAS(2023)·11 citations

Affiliations

first authorsco-authorsvia INSPIRE