6,032 research outputs found

    Microscopic linear response calculations based on the Skyrme functional plus the pairing contribution

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    A self-consistent Quasiparticle-Random-Phase-Approximation (QRPA) model which employs the canonical Hartree-Fock-Bogoliubov (HFB) basis and an energy-density functional with a Skyrme mean field part and a density-dependent pairing, is used to study the monopole collective excitations of spherical even-even nuclei. The influence of the spurious state on the strength function of the isoscalar monopole excitations is clearly assessed. We compare the effect of different kinds of pairing forces (volume pairing, surface pairing and mixed pairing) on the monopole excitation strength function. The energy of the Isoscalar Giant Monopole Resonance (ISGMR), which is related to the nuclear incompressibility K∞K_{\infty}, is calculated for tin isotopes and the results are discussed.Comment: Accepted for publication in Phys. Rev.

    Pairing Properties of Symmetric Nuclear Matter in Relativistic Mean Field Theory

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    The properties of pairing correlations in symmetric nuclear matter are studied in the relativistic mean field (RMF) theory with the effective interaction PK1. Considering well-known problem that the pairing gap at Fermi surface calculated with RMF effective interactions are three times larger than that with Gogny force, an effective factor in the particle-particle channel is introduced. For the RMF calculation with PK1, an effective factor 0.76 give a maximum pairing gap 3.2 MeV at Fermi momentum 0.9 fm−1^{-1}, which are consistent with the result with Gogny force.Comment: 14 pages, 6 figures

    Scalar strangeness content of the nucleon and baryon sigma terms

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    The scalar strangeness content of the nucleon, characterized by the so-called strangeness-nucleon sigma term, is of fundamental importance in understanding its sea-quark flavor structure. We report a determination of the octet baryon sigma terms via the Feynman-Hellmann theorem by analyzing the latest high-statistics nf=2+1n_f=2+1 lattice QCD simulations with covariant baryon chiral perturbation theory up to next-to-next-to-next-to-leading order. In particular, we predict σπN=55(1)(4)\sigma_{\pi N}=55(1)(4) MeV and σsN=27(27)(4)\sigma_{sN}=27(27)(4) MeV, while the first error is statistical and the second systematic due to different lattice scales. The predicted σsN\sigma_{sN} is consistent with the latest LQCD results and the results based on the next-to-next-to-leading order chiral perturbation theory. Several key factors in determining the sigma terms are systematically taken into account and clarified for the first time, including the effects of lattice scale setting, systematic uncertainties originating from chiral expansion truncations, and constraint of strong-interaction isospin breaking effects.Comment: 6 pages, 2 figures; version to appear in Physical Review

    Spin-orbit and orbit-orbit strengths for radioactive neutron-rich doubly magic nucleus 132^{132}Sn in relativistic mean field theory

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    Relativistic mean field (RMF) theory is applied to investigate the properties of the radioactive neutron-rich doubly magic nucleus 132^{132}Sn and the corresponding isotopes and isotones. The two-neutron and two-proton separation energies are well reproduced by the RMF theory. In particular, the RMF results agree with the experimental single-particle spectrum in 132^{132}Sn as well as the Nilsson spin-orbit parameter CC and orbit-orbit parameter DD thus extracted, but remarkably differ from the traditional Nilsson parameters. Furthermore, the present results provide a guideline for the isospin dependence of the Nilsson parameters.Comment: 4 pages, 4 figures, Phys. Rev. C in pres

    Octet baryon masses and sigma terms in covariant baryon chiral perturbation theory

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    We report an analysis of the octet baryon masses using the covariant baryon chiral perturbation theory up to next-to-next-to-next-to-leading order with and without the virtual decuplet contributions. Particular attention is paid to the finite-volume corrections and the finite lattice spacing effects on the baryon masses. A reasonable description of all the publicly available nf=2+1n_f=2+1 lattice QCD data is achieved.Utilyzing the Feynman-Hellmann theorem, we determine the nucleon sigma terms as σπN=55(1)(4)\sigma_{\pi N}=55(1)(4) MeV and σsN=27(27)(4)\sigma_{sN}=27(27)(4) MeV.Comment: 4 pages; presented by Xiu-Lei Ren at The Seventh International Symposium on Chiral Symmetry in Hadrons and Nuclei (Chiral 2013), October 27-30, 2013, Beijing, Chin
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