Isospin-Asymmetric Cold Nuclear Matter in the Relativistic Mean-Field Theory with a Scalar-Isovector Interaction Channel

The properties of isospin-asymmetric cold nuclear matter are studied in terms of the relativistic mean-field theory in which, besides the fields of σ, ω, and ρ mesons, and the isovector, Lorentz-scalar field of the δ-meson is also taken into account. The properties of purely nucleonic np matter are...

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Veröffentlicht in:Astrophysics 2024-08, Vol.67 (2), p.215-230
Hauptverfasser: Alaverdyan, G. B., Alaverdyan, A. G.
Format: Artikel
Sprache:eng
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Zusammenfassung:The properties of isospin-asymmetric cold nuclear matter are studied in terms of the relativistic mean-field theory in which, besides the fields of σ, ω, and ρ mesons, and the isovector, Lorentz-scalar field of the δ-meson is also taken into account. The properties of purely nucleonic np matter are studied as a function of the baryon density n B and the asymmetry parameter α, as well as the properties of electrically neutral β-equilibrium npe μ matter as a function of the baryon density n B . For different values of n B and a, such characteristics of np matter as the energy per baryon, the specific energy owing to isospin asymmetry, the effective proton and neutron masses, and the specific binding energy, are determined. It is shown that the energy owing to the asymmetry for a fixed value of α is a monotonically increasing function of the baryon density n B . For npe m matter, the effective proton and neutron masses M p e f f , M n e f f , the specific binding energy E bind , the symmetry energy E sym , the quantitative fraction of protons Y p = n p / n B are studied, as well as the average meson fields σ ~ , ω ~ , δ ~ , and ρ ~ as functions of the baryon density n B .
ISSN:0571-7256
1573-8191
DOI:10.1007/s10511-024-09829-y