2017
DOI: 10.1016/j.physletb.2016.12.013
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Constraining nucleon high momentum in nuclei

Abstract: Recent studies at Jefferson Lab show that there are a certain proportion of nucleons in nuclei have momenta greater than the so-called nuclear Fermi momentum $p_{F}$. Based on the transport model of nucleus-nucleus collisions at intermediate energies, nucleon high momentum caused by the neutron-proton short-range correlations in nuclei is constrained by comparing with $\pi$ and photon experimental data and considering some uncertainties. The high momentum cutoff value $p_{max}$ $\leq$ 2$p_{F}$ is obtained.Comm… Show more

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Cited by 30 publications
(32 citation statements)
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“…The neutron and proton density distributions in nucleus are given by the Skyrme-Hartree-Fock with Skyrme M * force parameters [37]. In initialization of colliding nuclei, the proton and neutron momentum distributions with high-momentum tails are employed [35,36,[38][39][40]. The isospin-and momentum-dependent single nucleon mean-field potential reads…”
Section: Model and Methodsmentioning
confidence: 99%
“…The neutron and proton density distributions in nucleus are given by the Skyrme-Hartree-Fock with Skyrme M * force parameters [37]. In initialization of colliding nuclei, the proton and neutron momentum distributions with high-momentum tails are employed [35,36,[38][39][40]. The isospin-and momentum-dependent single nucleon mean-field potential reads…”
Section: Model and Methodsmentioning
confidence: 99%
“…In the used IBUU model, nucleon spatial distribution in initial colliding nuclei is given by [11,23]…”
Section: The Initialization Of Nucleon Momentum and The Transportmentioning
confidence: 99%
“…[26,27]. For example, properties of the short-range tensor force and ramifications of the HMT on the Equation of State (EOS) of neutron-rich matter [28][29][30][31][32], especially the density dependence of nuclear symmetry energy E sym (ρ) are still poorly known. The E sym (ρ) encodes information about the isospin dependence of nuclear EOS, it is measured in the so-called parabolic approximation of the EOS by the change in single nucleonic energy when all protons are replaced by neutrons [33].…”
Section: Introductionmentioning
confidence: 99%