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NSR database version of May 2, 2024.

Search: Author = F.Grill

Found 5 matches.

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2014GR14      Phys.Rev. C 90, 045803 (2014)

F.Grill, H.Pais, C.Providencia, Is.Vidana, S.S.Avancini

Equation of state and thickness of the inner crust of neutron stars

doi: 10.1103/PhysRevC.90.045803
Citations: PlumX Metrics

2014PR02      Eur.Phys.J. A 50, 44 (2014)

C.Providencia, S.S.Avancini, R.Cavagnoli, S.Chiacchiera, C.Ducoin, F.Grill, J.Margueron, D.P.Menezes, A.Rabh, I.Vidana

Imprint of the symmetry energy on the inner crust and strangeness content of neutron stars

doi: 10.1140/epja/i2014-14044-7
Citations: PlumX Metrics

2012GR10      Phys.Rev. C 85, 055808 (2012)

F.Grill, C.Providencia, S.S.Avancini

Neutron star inner crust and symmetry energy

doi: 10.1103/PhysRevC.85.055808
Citations: PlumX Metrics

2011GR19      Phys.Rev. C 84, 065801 (2011)

F.Grill, J.Margueron, N.Sandulescu

Cluster structure of the inner crust of neutron stars in the Hartree-Fock-Bogoliubov approach

NUCLEAR STRUCTURE Z=12-60, N=82-1750; calculated neutron and proton densities, pairing gaps, HF binding energies, pairing correlations in the inner crust of neutron stars. SkyrmeHartree-Fock-Bogoliubov (HFB) calculations with zero-range density-dependent pairing forces by treating nuclear clusters in the Wigner-Seitz approximation.

doi: 10.1103/PhysRevC.84.065801
Citations: PlumX Metrics

2010FO12      Phys.Rev. C 82, 065804 (2010)

M.Fortin, F.Grill, J.Margueron, D.Page, N.Sandulescu

Thermalization time and specific heat of the neutron stars crust

doi: 10.1103/PhysRevC.82.065804
Citations: PlumX Metrics