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arxiv: 1502.01248 · v1 · pith:Y6GR5U4Xnew · submitted 2015-02-04 · ⚛️ nucl-th · astro-ph.SR

Comparative study of three-nucleon force models in nuclear matter

classification ⚛️ nucl-th astro-ph.SR
keywords matterforcemodelsnuclearthree-nucleonenergyreproducesymmetric
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We calculate the energy per particle of symmetric nuclear matter and pure neutron matter using the microscopic many-body Brueckner-Hartree-Fock (BHF) approach and employing the Argonne V18 (AV18) nucleon-nucleon (NN) potential supplemented with two different three-nucleon force models recently constructed to reproduce the binding energy of $^3$H, $^3$He and $^4$He nuclei as well as the neutron-deuteron doublet scattering length. We find that none of these new three-nucleon force models is able to reproduce simultaneously the empirical saturation point of symmetric nuclear matter and the properties of three- and four-nucleon systems.

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