PaperPanorama

Nuclear Theory·nucl-th

Wednesday·June 14, 2023

9 papers4 primary·5 cross-listed

  1. 01

    [Submitted on 11 Jun 2023]

    Additive Multi-Index Gaussian process modeling, with application to multi-physics surrogate modeling of the quark-gluon plasma

    Kevin Li · Simon Mak · J.-F Paquet · Steffen A. Bass

    The Quark-Gluon Plasma (QGP) is a unique phase of nuclear matter, theorized to have filled the Universe shortly after the Big Bang. A critical challenge in studying the QGP is that, to reconcile experimental observables with theoretical parameters, one requires many simulation runs of a complex physics model over a high-dimensional parameter space. Each run is computationally very expensive, requiring thousands of CPU hours, thus limiting physicists to only several hundred runs. Given limited training data for high-dimensional prediction, existing surrogate models often yield poor predictions with high predictive uncertainties, leading to imprecise scientific findings. To address this, we propose a new Additive Multi-Index Gaussian process (AdMIn-GP) model, which leverages a flexible additive structure on low-dimensional embeddings of the parameter space. This is guided by prior scientific knowledge that the QGP is dominated by multiple distinct physical phenomena (i.e., multiphysics), each involving a small number of latent parameters. The AdMIn-GP models for such embedded structures within a flexible Bayesian nonparametric framework, which facilitates efficient model fitting via a carefully constructed variational inference approach with inducing points. We show the effectiveness of the AdMIn-GP via a suite of numerical experiments and our QGP application, where we demonstrate considerably improved surrogate modeling performance over existing models.

    Subjects:
    Nuclear Theory (nucl-th); Machine Learning (cs.LG); High Energy Physics — Phenomenology (hep-ph); Machine Learning (stat.ML)
    arXiv:
    2306.07299 [pdf]
    1 citation
  2. 02

    [Submitted on 12 Jun 2023]

    Hydrodynamic theories for a system of weakly self-interacting classical ultra-relativistic scalar particles: microscopic derivations and attractors

    Gabriel S. Rocha🇧🇷 · Caio V. P. de Brito🇧🇷 · Gabriel S. Denicol🇧🇷

    We derive and investigate several hydrodynamic formalisms that emerge from a system of classical, ultra-relativistic scalar particles self-interacting via a quartic potential. The specific form of the total cross-section enables the analytical computation of all transport coefficients that appear in Navier-Stokes (NS), Bemfica-Disconzi-Noronha-Kovtun (BDNK), and second-order transient hydrodynamic theories. We solve all these formalisms in a Bjorken flow scenario and show that NS and BDNK theories display unphysical features when gradients become sufficiently large. This implies that these hydrodynamic approaches may not be suitable to describe the early stages of heavy ion collisions.

    Comments:
    30 pages, 8 figures
    Subjects:
    Nuclear Theory (nucl-th); High Energy Physics — Phenomenology (hep-ph); High Energy Physics — Theory (hep-th)
    arXiv:
    2306.07423 [pdf]
    PRD(2023)·28 citations
  3. 03

    [Submitted on 12 Jun 2023]

    Probing DDM and ML quantum concepts in shape phase transitions of -unstable nuclei

    S. Ait El Korchi · M. Chabab · A. El Batoul · A. Lahbas · M. Oulne

    In a recent paper (S. Ait El Korchi et al. 2020 EPL 132 52001), we explored, inside the context of Critical Point Symmetries (CPSs) X(3) and Z(4), a correlation between two exceedingly known quantum concepts, the Minimal Length (ML) and the Deformation-Dependent Mass (DDM), that are commonly applied in various areas of physics. Such a correlation has been strongly identified in transition nuclei by calculating some physical observables of that quantum system, like as energy spectra, moments of inertia and transition probabilities. In this paper we extend that study to E(5) dynamical symmetry corresponding to the shape phase transition U(5)O(6). The experimental realization of the models was found to occur in some nuclei, using the existing phenomenological potentials : Infinite Square Well, Davidson and Kratzer, whose models fits provide the best agreement. Importantly the calculations performed in this work using these potentials corroborate the fact that the revealed correlation between both quantum concepts is not destructively affected by the presence of other model parameters and hence its existence is independent of the form or type of the used potential. Undoubtedly, the present work will open the way for more investigations of this correlation in the limits of other critical points symmetries in nuclear shape phase transitions which play today a major role in nuclear structure research from theoretical as well as experimental point of view.

    Comments:
    31 pages, 3 figures, accepted in Nuclear Physics A
    Subjects:
    Nuclear Theory (nucl-th); Nuclear Experiment (nucl-ex)
    arXiv:
    2306.07439 [pdf]
    NPA(2023)·2 citations
  4. 04

    [Submitted on 13 Jun 2023]

    Born-Infeld nonlinear electromagnetism in relativistic heavy ion collisions

    Will Price🇺🇸 · Martin Formanek🇨🇿 · Johann Rafelski🇺🇸

    We study the effect of the limiting field strength of Born-Infeld electromagnetism on the dynamics of charged particle scattering. We formulate the Born-Infeld limiting field in an invariant manner, showing that it is the electric field-dominated eigenvalue `' of the field tensor which is limited rather than the individual field vectors. Heavy ion collisions in particular provide uniquely large values of the field invariants that appear in the BI action, amplifying nonlinear effects. Thus ``'' is the dominant input into the force between heavy ions that we use to compute the scattering angle as a function of impact parameter. We evaluate the BI effects, showing relevance at small impact parameters and exhibiting their dependence on the value of the limiting field strength.

    Comments:
    This article belongs to the special issue of Acta Physica Polonica A printed in honor of Professor Iwo Bialynicki-Birula on the occasion of his 90th birthday (Ed. Tomasz Sowinski, DOI:10.12693/APhysPolA.143.S0)
    Subjects:
    Nuclear Theory (nucl-th); High Energy Physics — Phenomenology (hep-ph); Quantum Physics (quant-ph)
    arXiv:
    2306.07704 [pdf]
    Acta Phys.Polon.A(2023)·3 citations
  5. 05

    [Submitted on 13 Jun 2023] (cross-list from astro-ph.HE)

    Shear and interface modes in neutron stars with pasta structures

    Hajime Sotani

    We carefully examine the shear and interface modes, which are excited due to the presence of crust elasticity, in neutron stars with pasta structures, adopting the relativistic Cowling approximation. We find that the shear modes are independent of the presence of the cylindrical-hole and spherical-hole nuclei at least up to a few kilohertz, while the interface modes strongly depend on the presence of the cylindrical-hole and spherical-hole nuclei. In addition, we find empirical relations for the interface mode frequencies multiplied by the stellar mass and for the shear mode frequencies multiplied by the stellar radius. These relations are expressed as a function of the stellar compactness almost independently of the stiffness in a higher-density region inside the neutron star, once one selects the crust equation of state. Thus, if one would simultaneously observe the shear and interface modes from a neutron star, one might extract the neutron star mass and radius with the help of the constraint on the crust stiffness obtained from terrestrial experiments.

    Comments:
    Accepted for publication in RPD
    Subjects:
    High Energy Astrophysical Phenomena (astro-ph.HE); Nuclear Theory (nucl-th)
    arXiv:
    2306.07531 [pdf]
    PRD(2023)·11 citations
  6. 06

    [Submitted on 13 Jun 2023] (cross-list from hep-th)

    Causality Criteria from Stability Analysis at Ultra-High Boost

    Shuvayu Roy🇮🇳 · Sukanya Mitra🇮🇳

    In this work, we have exclusively employed the linear stability analysis at ultra-high boost on two well-known stable-causal theories - second-order MIS and first-order BDNK, to identify the region of parameter space over which they are frame-invariantly stable and obey causal signal propagation. It has been shown that at near-luminal boost, stability criteria alone can provide the causality constraints on transport coefficients, which are identical to the asymptotic causality conditions, without actually going to the asymptotic limit of the theories. Thus, we present an alternative approach to derive the causality constraints, which is more appropriate for low-energy effective theories like relativistic hydrodynamics.

    Comments:
    8+1 pages, 2 figures, 1 supplementary material. Version accepted in Phys. Rev. D
    Subjects:
    High Energy Physics — Theory (hep-th); High Energy Physics — Phenomenology (hep-ph); Nuclear Theory (nucl-th)
    arXiv:
    2306.07564 [pdf]
    PRD(2024)·8 citations
  7. 07

    [Submitted on 13 Jun 2023] (cross-list from astro-ph.HE)

    R-process beta-decay neutrino flux from binary neutron star mergers and collapsars

    Yu An🇨🇳 · Meng-Ru Wu🇹🇼 · Gang Guo🇨🇳 · Yue-Lin Sming Tsai🇨🇳 · Shih-Jie Huang🇹🇼 · Yi-Zhong Fan🇨🇳

    This study investigates the antineutrinos production by -decay of -process nuclei in two astrophysical sites that are capable of producing gamma-ray bursts (GRBs): binary neutron star mergers (BNSMs) and collapsars, which are promising sites for heavy element nucleosynthesis. We employ a simplified method to compute the -decay energy spectrum and consider a number of different representative thermodynamic trajectories for -process simulations, each with four sets of distribution. The time evolution of the spectrum is derived for both the dynamical ejecta and the disk wind for BNSMs and collapsar outflow, based on approximated mass outflow rates. Our results show that the has an average energy of approximately 3 to 9~MeV, with a high energy tail of up to 20 MeV. The flux evolution is primarily determined by the outflow duration, and can thus remain large for ~s and ~s for BNSMs and collapsars, respectively. For a single merger or collapsar at 40~Mpc, the flux is ~cm~s, indicating a possible detection horizon up to ~Mpc for Hyper-Kamiokande. We also estimate their contributions to the diffuse background, and find that both sources should only contribute subdominantly to the diffuse background when compared to that expected from core-collapse supernovae.

    Comments:
    14 pages, 8 figures
    Subjects:
    High Energy Astrophysical Phenomena (astro-ph.HE); Nuclear Theory (nucl-th)
    arXiv:
    2306.07659 [pdf]
    PRD(2023)·8 citations
  8. 08

    [Submitted on 13 Jun 2023] (cross-list from nucl-ex)

    Rotation of pear-shaped Ru nucleus

    A. Karmakar · P. Datta · Soumik Bhattacharya · Shabir Dar · S. Bhattacharyya · G. Mukherjee · H. Pai · S. Basu · S. Nandi · S. S. Nayak · Sneha Das · R. Raut and 5 other authors

    Atomic nuclei in general can have deformed shapes and nearly all these shapes are symmetric with respect to reflection. Only a few Actinide nuclei have stable reflection asymmetric pear shapes in their ground state and exhibit characteristic rotational bands. In this article, we report on the observation of two alternate parity rotational bands in 100Ru, which are connected by seven interleaved electric dipole transitions and their rates are found to be enhanced. In addition, the moments of inertia associated with these two opposite parity rotational bands have been found to be similar. These experimental observations indicate the rotation of a stable pear-shaped 100Ru nucleus, which is the first such observation outside the Actinide mass region. This shape is built on an excited configuration and originates from the rotational alignment of the angular momenta of a pair of neutrons. This unique observation establishes an alternate mechanism by which an atomic nucleus can assume a pear shape.

    Comments:
    13 pages, 7 figures, 2 tables
    Subjects:
    Nuclear Experiment (nucl-ex); Nuclear Theory (nucl-th)
    arXiv:
    2306.07670 [pdf]
    1 citation
  9. 09

    [Submitted on 13 Jun 2023] (cross-list from hep-ph)

    Heavy quark radiation in an anisotropic hot QCD medium

    Jai Prakash🇮🇳 · Vinod Chandra🇮🇳 · Santosh K. Das🇮🇳

    The impact of momentum anisotropy on the heavy quarks (HQs) dynamics has been investigated in a hot QCD medium while considering both collisional and radiative processes within the ambit of the Fokker-Planck approach. The relative orientation of the HQs motion (momentum vector) with respect to the direction of anisotropy is responsible for the character of transport coefficients. Therefore, the drag and diffusion coefficients of the HQs are decomposed, respectively, into two and four components by considering a general tensor basis. Each component of the drag and diffusion coefficient of the HQs has been analyzed in detail. It is observed that the anisotropy has a significant impact on the transport coefficients of the HQ for both the collisional and the radiational processes. The nuclear suppression factor, , has been computed considering the anisotropic medium. It is observed that the momentum anisotropy affects the of the HQs significantly in both elastic and inelastic cases.

    Comments:
    Published in Physical Review D
    Subjects:
    High Energy Physics — Phenomenology (hep-ph); Nuclear Theory (nucl-th)
    arXiv:
    2306.07966 [pdf]
    PRD(2023)·24 citations

Affiliations

first authorsco-authorsvia INSPIRE