NSR Query Results
Output year order : Descending NSR database version of May 3, 2024. Search: Author = L.Brito Found 20 matches. 2014CA18 Nucl.Data Sheets 118, 276 (2014) B.V.Carlson, L.Brito, D.F.Mega, R.Capote, M.Herman, M.E.Rego Exclusive Multiple Emission Cross Sections in the Hybrid Monte Carlo Pre-equilibrium Model and in EMPIRE-3.1 NUCLEAR REACTIONS 59Co(p, 2n), (p, 3n), E=50, 100, 200 MeV; calculated exclusive neutron σ(En) using hybrid Monte Carlo simulation model; discussed implementation to EMPIRE-3.1.
doi: 10.1016/j.nds.2014.04.057
2012AV03 Phys.Rev. C 85, 035806 (2012) S.S.Avancini, C.C.Barros, L.Brito, S.Chiacchiera, D.P.Menezes, C.Providencia Light clusters in nuclear matter and the "pasta" phase
doi: 10.1103/PhysRevC.85.035806
2010PA24 Phys.Rev. C 82, 025801 (2010) H.Pais, A.Santos, L.Brito, C.Providencia Dynamical properties of nuclear and stellar matter and the symmetry energy
doi: 10.1103/PhysRevC.82.025801
2009AV02 Phys.Rev. C 79, 035804 (2009) S.S.Avancini, L.Brito, J.R.Marinelli, D.P.Menezes, M.M.W.de Moraes, C.Providencia, A.M.Santos Nuclear "pasta" phase within density dependent hadronic models
doi: 10.1103/PhysRevC.79.035804
2008DU19 Phys.Rev. C 78, 055801 (2008) C.Ducoin, C.Providencia, A.M.Santos, L.Brito, Ph.Chomaz Cluster formation in compact stars: Relativistic versus Skyrme nuclear models
doi: 10.1103/PhysRevC.78.055801
2008SA15 Phys.Rev. C 77, 045805 (2008) A.M.Santos, L.Brito, C.Providencia Dynamical instabilities in density-dependent hadronic relativistic models
doi: 10.1103/PhysRevC.77.045805
2007BR28 Phys.Rev. C 76, 044316 (2007) L.Brito, Ph.Chomaz, D.P.Menezes, C.Providencia Low-density expansion and isospin dependence of nuclear energy functional: Comparison between relativistic and Skyrme models
doi: 10.1103/PhysRevC.76.044316
2006AV07 Phys.Rev. C 74, 024317 (2006) S.S.Avancini, L.Brito, Ph.Chomaz, D.P.Menezes, C.Providencia Spinodal instabilities and the distillation effect in relativistic hadronic models
doi: 10.1103/PhysRevC.74.024317
2006BR23 Phys.Rev. C 74, 045801 (2006) L.Brito, C.Providencia, A.M.Santos, S.S.Avancini, D.P.Menezes, Ph.Chomaz Unstable modes in relativistic neutron-electron-proton (npe) matter at finite temperature
doi: 10.1103/PhysRevC.74.045801
2006PR04 Phys.Rev. C 73, 025805 (2006) C.Providencia, L.Brito, S.S.Avancini, D.P.Menezes, Ph.Chomaz Low-density instabilities in relativistic asymmetric matter of compact stars
doi: 10.1103/PhysRevC.73.025805
2006PR21 Phys.Rev. C 74, 045802 (2006) C.Providencia, L.Brito, A.M.S.Santos, D.P.Menezes, S.S.Avancini Coupling of nuclear and electron modes in relativistic stellar matter
doi: 10.1103/PhysRevC.74.045802
2005AV05 Phys.Rev. C 71, 044323 (2005) S.S.Avancini, L.Brito, D.P.Menezes, C.Providencia Collective modes in relativistic asymmetric nuclear matter
doi: 10.1103/PhysRevC.71.044323
2005AV07 Braz.J.Phys. 35, 832 (2005) S.S.Avancini, D.P.Menezes, L.Brito, C.Providencia Asymmetric Nuclear Matter and its Instabilities
doi: 10.1590/S0103-97332005000500031
2004AV04 Phys.Rev. C 70, 015203 (2004) S.S.Avancini, L.Brito, D.P.Menezes, C.Providencia Instabilities in asymmetric nuclear matter
doi: 10.1103/PhysRevC.70.015203
2002PR07 Nucl.Phys. A703, 188 (2002) C.Providencia, D.P.Menezes, L.Brito Relativistic Thomas-Fermi Description of Sm Isotopes at Finite Temperature NUCLEAR STRUCTURE 150,166Sm; calculated proton density, neutron skin thickness, radii, and binding energy vs temperature. Nuclear Walecka model, Thomas-Fermi approximation.
doi: 10.1016/S0375-9474(01)01334-3
1996DA32 Phys.Rev. C54, 2525 (1996) C.da Providencia, L.Brito, J.da Providencia, M.Nielsen, X.Vinas Relativistic Thomas-Fermi Description of Collective Modes in Droplets of Nuclear Matter
doi: 10.1103/PhysRevC.54.2525
1994PR07 J.Phys.(London) G20, 1209 (1994); Erratum J.Phys.(London) G21, 591 (1995) C.Providencia, L.Brito, J.da Providencia, D.Bonatsos, D.P.Menezes The q-Deformed Moszkowski Model: High-spin states
doi: 10.1088/0954-3899/20/8/011
1986BR24 Phys.Lett. 177B, 251 (1986) Surface Tension and Nuclear Low-Lying Vibrations in a Fluid-Dynamical Approach NUCLEAR STRUCTURE 208Pb; calculated levels, multipole excitation EWSR. Nuclear fluid dynamical model.
doi: 10.1016/0370-2693(86)90747-1
1985BR24 Phys.Rev. C32, 2049 (1985) Variational Formulation of Nuclear Fluid Dynamics NUCLEAR STRUCTURE 208Pb; calculated giant multipoles excitation, EWSR. Fluid dynamical model, variational formulation.
doi: 10.1103/PhysRevC.32.2049
1984BR18 Phys.Lett. 143B, 36 (1984) Interaction between First Sound and Zero Sound Degrees of Freedom NUCLEAR STRUCTURE 208Pb; calculated levels, giant multipole resonances. Fluid dynamical model.
doi: 10.1016/0370-2693(84)90799-8
Back to query form Note: The following list of authors and aliases matches the search parameter L.Brito: , L.P.BRITO |