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NSR database version of May 1, 2024.

Search: Author = F.Aymard

Found 5 matches.

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2016AY02      J.Phys.(London) G43, 045105 (2016)

F.Aymard, F.Gulminelli, J.Margueron

Analytical mass formula and nuclear surface properties in the ETF approximation. Part I: symmetric nuclei

doi: 10.1088/0954-3899/43/4/045105
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2016AY03      J.Phys.(London) G43, 045106 (2016)

F.Aymard, F.Gulminelli, J.Margueron

Analytical mass formula and nuclear surface properties in the ETF approximation. Part II: asymmetric nuclei

doi: 10.1088/0954-3899/43/4/045106
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2015BU14      Phys.Rev. C 92, 055804 (2015)

S.Burrello, F.Gulminelli, F.Aymard, M.Colonna, Ad.R.Raduta

Heat capacity of the neutron star inner crust within an extended nuclear statistical equilibrium model

doi: 10.1103/PhysRevC.92.055804
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2014AY04      Phys.Rev. C 89, 065807 (2014)

F.Aymard, F.Gulminelli, J.Margueron

In-medium nuclear cluster energies within the extended Thomas-Fermi approach

NUCLEAR STRUCTURE ⁴⁰Ca, ⁴⁸Cr, ⁵⁶Ni, ⁶⁸Se, ⁸⁸Ru, ^100,132,150Sn; calculated density profiles. A=20-130; calculated energy per nucleon for N=Z nuclei. Z=20, A=36-60; Z=50, A=98-170; Z=82, A=180-260; calculated difference between the energy per particle in the ETF and HF models. A=200; calculated bulk and surface energy per nucleon. A=10-250; calculated surface energy per surface nucleon as a function of nucleus mass. Simple analytical modeling of nuclear density profiles within the extended Thomas-Fermi (ETF) approximation. Hartree-Fock calculations for ground states. Comparison with experimental data.

doi: 10.1103/PhysRevC.89.065807
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2014RA05      Eur.Phys.J. A 50, 24 (2014)

Ad.R.Raduta, F.Aymard, F.Gulminelli

Clusterized nuclear matter in the (proto-)neutron star crust and the symmetry energy

doi: 10.1140/epja/i2014-14024-y
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