PaperPanorama

Nuclear Theory·nucl-th

Tuesday·October 8, 2024

12 papers5 primary·7 cross-listed

  1. 01

    Kubo formula for spin hydrodynamics: spin chemical potential as leading order in gradient expansion

    Sourav Dey🇮🇳 · Arpan Das🇮🇳

    We present a first-order dissipative spin hydrodynamic framework, where the spin chemical potential is treated as the leading term in the hydrodynamic gradient expansion, i.e., . We argue that for the consistency of the theoretical framework, the energy-momentum tensor needs to be symmetric at least up to order . We consider the phenomenological form of the spin tensor, where it is anti-symmetric in the last two indices only. A comprehensive analysis of spin hydrodynamics is conducted using both macroscopic entropy current analysis and microscopic Kubo formalism, establishing consistency between the two approaches. A key finding is the entropy production resulting from spin-orbit coupling, which alters the traditional equivalence between the Landau and Eckart fluid frames. Additionally, we identify cross-diffusion effects, where vector dissipative currents are influenced by gradients of both spin chemical potential and chemical potential corresponding to the conserved charge through off-diagonal transport coefficients. Two distinct methods for decomposing the spin tensor are proposed, and their equivalence is demonstrated through Kubo relations.

    nucl-thhep-phhep-thPRD(2025)·21 citations
  2. 02

    Peak of sound velocity, scale symmetry, and nuclear force in baryonic matter

    Lu-Qi Zhang🇨🇳 · Yao Ma🇨🇳 · Yong-Liang Ma🇨🇳

    The sound velocity in homogeneous matter has fundamental significance as it relates to the stiffness of the equation of state of compact star matter. In this work, we investigate the density evolution of the sound velocity in homogeneous {neutron matter at zero temperature} by using an effective field theory implemented with a conformal compensator -- the nonlinear realization of scale symmetry -- regarded as the source of the lightest scalar meson. We find that the peak of sound velocity emerges naturally in the intermediate density region, , without resorting to any transitions from hadron to exotic configurations or introducing new degrees of freedom. This phenomenon is not found in the Walecka-type models where the sigma meson is included in the linear-type approach, therefore it is an intrinsic character of the dilaton compensator approach through the matching of the QCD trace anomaly; a mechanism has not been found before, and it connects to the character of the lightest scalar meson. In addition, these observations shed light on how the hidden scale symmetry manifests in the nuclear medium from the unitarity limit in dilute matter to the dilaton limit in compact star matter.

    nucl-thPRC(2025)·11 citations
  3. 03

    Phase Diagrams of Relativistic Selfinteracting Boson System

    V. Gnatovskyy🇺🇦 · D. Anchishkin🇺🇦 · D. Zhuravel🇺🇦 · V. Karpenko🇺🇦

    Within the Canonical Ensemble, we investigate a system of interacting relativistic bosons at finite temperatures and finite isospin densities in a mean-field approach. The mean field contains both attractive and repulsive terms. Temperature and isospin-density dependencies of thermodynamic quantities were obtained. It is shown that in the case of attraction between particles in a bosonic system, a liquid-gas phase transition develops against the background of the Bose-Einstein condensate. The corresponding phase diagrams are given. We explain the reasons why the presence of a Bose condensate significantly increases the critical temperature of the liquid-gas phase transition compared to that obtained for the same system within the framework of the Boltzmann statistics. Our results may have implications for the interpretation of experimental data, in particular, how sensitive the critical point of the mixed phase is to the presence of the Bose-Einstein condensate.

    nucl-thhep-phquant-phUkr.J.Phys.(2024)·1 citation
  4. 04

    Probing for an IR-fixed Point in QCD by Superallowed Gamow-Teller Transitions in Doubly Magic Nuclei

    Mannque Rho🇫🇷 · Long-Qi Shao🇨🇳

    This brief note is to point out that the recent measurements at GSI and RIKEN of the superallowed Gamow-Teller transition in the doubly magic closed-shell nucleus Sn could give an indication for a possibly important {\it fundamental} quenching, thus-far unrecognized, of , unambiguously distinct from nuclear correlation effects in the framework of nuclear effective field theory. The result, either confirmed or ruled out both experimentally and theory, can have strong impacts on nuclear physics vis-à-vis with nuclear effective field theory as well as on particle physics relevant for going beyond the Standard Model.

    nucl-thhep-ph2 citations
  5. 05

    How the HESS J1731-347 event could be explained using condensation

    M. Veselsky🇨🇿 · P.S. Koliogiannis🇭🇷 · V. Petousis🇨🇿 · J. Leja🇸🇰 · Ch.C. Moustakidis🇬🇷

    The recent observation of a compact star with a mass of and a radius of km, located within the supernova remnant HESS J1731-347, has substantially reinforced the evidence for the presence of exotic matter in neutron stars core. This finding has markedly enhanced our comprehension of the equation of state for dense nuclear matter. In the present work, we investigate the possible existence of a kaon condensation in hadronic neutron stars by employing and comparing two theoretical frameworks: the Relativistic Mean Field model with first order kaon condensate and the Momentum-Dependent Interaction model complemented by chiral effective theory. To the best of our knowledge, this represents a first alternative attempt aimed to explain the bulk properties of the specific object with the inclusion of a kaon condensation in dense nuclear matter. The application of two different models enriches the research, providing insights from the aspect of different theoretical frameworks that accurately predict the existence of HESS J1731-347. In both cases significant insights are extracted for the parameter space of models, emphasizing to those concerning the nucleon-kaon potential, the threshold density for the appearance of a kaon condensation, as well as the parameter which is related to the strangeness content of the proton. Concluding, the present research indicates that a more systematic investigation of similar objects could offer valuable constraints on the properties of dense nuclear matter.

    nucl-thastro-ph.HEPLB(2025)·14 citations

Affiliations

first authorsco-authorsvia INSPIRE