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NSR database version of May 8, 2024.

Search: Author = C.Gonzalez-Boquera

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2021GO18      Phys.Rev. C 103, 064314 (2021)

C.Gonzalez-Boquera, M.Centelles, X.Vinas, L.M.Robledo

Finite-size instabilities in finite-range forces

NUCLEAR STRUCTURE ²⁰⁸Pb; calculated neutron and proton density with with a harmonic oscillator (HO) basis of 12, 14, 16, 18, and 19 shells using DIM DIM* Gogny interactions. ¹⁶O, ^100,132,176Sn, ²⁰⁸Pb; calculated binding energies in Hartree-Fock from the HO-basis calculation, the coordinate-space quasilocal (QLA), and the full coordinate-space calculation (FINRES4) with D1M and D1M* Gogny interactions. ⁴⁸Ca, ¹⁵⁴Sm; calculated differences between the HFB energies as functions of number of harmonic oscillator (HO) shells and quadrupole deformation β₂. Hartree-Fock (HF) method in the quasilocal approximation to finite-range forces. Role of the slope of the symmetry energy for nuclear structure properties.

doi: 10.1103/PhysRevC.103.064314
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2019GO15      Phys.Rev. C 100, 015806 (2019)

C.Gonzalez-Boquera, M.Centelles, X.Vinas, T.R.Routray

Core-crust transition in neutron stars with finite-range interactions: The dynamical method

doi: 10.1103/PhysRevC.100.015806
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2018GO07      Phys.Lett. B 779, 195 (2018)

C.Gonzalez-Boquera, M.Centelles, X.Vinas, L.M.Robledo

New Gogny interaction suitable for astrophysical applications

NUCLEAR STRUCTURE N<180; calculated binding energy differences in even-even nuclei. Comparison with available data.

doi: 10.1016/j.physletb.2018.02.005
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2017GO18      Phys.Rev. C 96, 065806 (2017)

C.Gonzalez-Boquera, M.Centelles, X.Vinas, A.Rios

Higher-order symmetry energy and neutron star core-crust transition with Gogny forces

doi: 10.1103/PhysRevC.96.065806
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