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Recent Progress in Quantum Hadrodynamics

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arxiv nucl-th/9701058 v1 pith:6OIE5LYI submitted 1997-01-28 nucl-th hep-ph

classification nucl-thhep-ph
keywords nuclearrelativisticeffectivehadrodynamicsmattermodelsnucleiquantum
verification ladder T0 review T1 audit T2 compute T3 formal
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Quantum hadrodynamics (QHD) is a framework for describing the nuclear many-body problem as a relativistic system of baryons and mesons. Motivation is given for the utility of such an approach and for the importance of basing it on a local, Lorentz-invariant lagrangian density. Calculations of nuclear matter and finite nuclei in both renormalizable and nonrenormalizable, effective QHD models are discussed. Connections are made between the effective and renormalizable models, as well as between relativistic mean-field theory and more sophisticated treatments. Recent work in QHD involving nuclear structure, electroweak interactions in nuclei, relativistic transport theory, nuclear matter under extreme conditions, and the evaluation of loop diagrams is reviewed.

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Cited by 6 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Explicitly on-shell currents in relativistic mean field models

    nucl-th 2026-07 conditional novelty 7.0 of 10

    The 'off-shell ambiguity' in relativistic mean-field one-body currents is spurious when currents are defined via free-nucleon operators; the correct mapping (Eq. 26) is parametrization-independent and requires time-li...

  2. Self-gravitating quantum stars with a globally relevant Bohm potential

    hep-th 2026-05 conditional novelty 6.0 of 10

    The equilibrium radius of self-gravitating dark fermion stars is determined by the fermion mass once the total mass is given, with the Bohm potential supplying outward pressure for heavier species and inward tension f...

  3. Casimir effect for a massive scalar field confined between parallel plates with a spatially varying effective mass

    hep-th 2026-07 reject novelty 5.0 of 10

    A claimed exact Casimir energy for a scalar field with a quadratic position-dependent mass is derived, but the conversion from continuum to discrete transverse modes uses an unproven Landau-style measure.

  4. Speed and accuracy for long signals: Frequency-domain effective-one-body waveforms for compact binary coalescences

    gr-qc 2026-06 unverdicted novelty 5.0 of 10

    Hybrid SPA-plus-FFT frequency-domain version of SEOBNRv5THM for quasi-circular spin-aligned BNS systems matches time-domain baseline accuracy while cutting computational cost for long signals.

  5. Compact star and compact star matter properties from a baryonic extended linear sigma model with explicit chiral symmetry breaking

    nucl-th 2025-12 reject novelty 5.0 of 10

    Tuning the πN sigma term to about -600 MeV (or incompressibility to ~500 MeV) lets one RMF model match neutron-star observations, but the tuning is fitting, not prediction.

  6. Nuclear matter properties and neutron star structures from an extended linear sigma model

    nucl-th 2026-03 unverdicted novelty 4.0 of 10

    An extended linear sigma model with delta meson and negative sigma_piN produces a symmetry-energy plateau and stiffer EOS that satisfies neutron-star and nuclear constraints.

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