NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = C.Providencia Found 143 matches. Showing 1 to 100. [Next]2024PE05 Phys.Rev. C 109, 025206 (2024) R.C.Pereira, P.Costa, C.Providencia, J.Moreira New approach to the 3-momentum regularization of the in-medium one- and two-fermion line integrals with applications to cross sections in the Nambu-Jona-Lasinio model
doi: 10.1103/PhysRevC.109.025206
2022AN24 Eur.Phys.J. A 58, 254 (2022) D.Antonopoulou, E.Bozzo, C.Ishizuka, D.I.Jones, M.Oertel, C.Providencia, L.Tolos, S.Typel CompOSE: a repository for neutron star equations of state and transport properties
doi: 10.1140/epja/s10050-022-00908-2
2022CU05 Phys.Rev. C 105, 065803 (2022) T.Custodio, H.Pais, C.Providencia Heavy baryons in hot stellar matter with light nuclei and hypernuclei NUCLEAR STRUCTURE 1n, 1,2,3,4H, 3,4,6He; calculated unbound nucleon and light cluster fractions as a function of temperature, density, mass fractions of Λ, Σ, and Ξ hyperons, Δ isobars, 1n, 1,2,3H, 3,4,6He light clusters, and 3,4H, 6He hypernuclei clusters as a function of the density; deduced that heavy-baryons, hyperons and Δs favor the formation of clusters, while a larger number of clusters decreases the fraction of free nucleons, favoring processes such as direct Urca reactions. Relativistic mean-field theory (RMF) with DD2 and FSU2H models. Relevance to the production of light nuclei, hypernuclei heavy baryons such as hyperons and Δ baryons in the low-density matter of stellar environments such as supernova or binary mergers.
doi: 10.1103/PhysRevC.105.065803
2022MA50 Phys.Rev. C 106, L042801 (2022) T.Malik, B.K.Agrawal, C.Providencia Inferring the nuclear symmetry energy at suprasaturation density from neutrino cooling
doi: 10.1103/PhysRevC.106.L042801
2022MA57 Phys.Rev. C 106, 055801 (2022) K.D.Marquez, D.P.Menezes, H.Pais, C.Providencia Δ baryons in neutron stars
doi: 10.1103/PhysRevC.106.055801
2022SU24 Phys.Rev. C 106, 035805 (2022) L.Suleiman, M.Fortin, J.L.Zdunik, C.Providencia Polytropic fits of modern and unified equations of state
doi: 10.1103/PhysRevC.106.035805
2022TY01 Eur.Phys.J. A 58, 221 (2022) S.Typel, M.Oertel, T.Klahn, D.Chatterjee, V.Dexheimer, C.Ishizuka, M.Mancini, J.Novak, H.Pais, C.Providencia, Ad.R.Raduta, M.Servillat, L.Tolos, for the CompOSE Core Collaboration CompOSE reference manual
doi: 10.1140/epja/s10050-022-00847-y
2021BO13 Phys.Rev. C 103, 055804 (2021) O.Boukari, H.Pais, S.Antic, C.Providencia Critical properties of calibrated relativistic mean-field models for the transition to warm, nonhomogeneous nuclear and stellar matter
doi: 10.1103/PhysRevC.103.055804
2021CU03 Phys.Rev. C 104, 035801 (2021) T.Custodio, H.Pais, C.Providencia Light hyperclusters and hyperons in low-density hot stellar matter NUCLEAR STRUCTURE 2,3H, 3,4,6He; calculated mass fractions of light clusters and unbound protons and neutrons in equilibrium versus density for temperature T=10, 30, 50, 100 MeV, unbound nucleon and light cluster fractions with and without hyperons as function of temperature T=10-100 MeV, unbound nucleon and hyperon (Λ, Σ, Ξ) fractions, total mass fraction of the light clusters, and mass fractions of the unbound protons and neutrons, Λ, Σ and Ξ, light clusters, and light hypernuclei as a function of the density, with and without light clusters; deduced that dissolution of the less-abundant clusters occurs at larger densities due to smaller Pauli-blocking effects. Calculations based on relativistic mean-field model (RMF) with density-dependent (DD) couplings in low-density matter. Relevance to the presence of light nuclei in core-collapse supernova matter and in binary neutron star (NS) mergers.
doi: 10.1103/PhysRevC.104.035801
2021FE10 Eur.Phys.J. A 57, 263 (2021) M.Ferreira, A.Rabhi, C.Providencia Crust-core transition of a neutron star: effect of the temperature under strong magnetic fields
doi: 10.1140/epja/s10050-021-00572-y
2021PA23 Eur.Phys.J. A 57, 193 (2021) H.Pais, B.Bertolino, J.Fang, X.Wang, C.Providencia Strong magnetic fields: neutron stars with an extended inner crust
doi: 10.1140/epja/s10050-021-00506-8
2021RA08 Phys.Rev. C 103, 035811 (2021) A.Rabhi, C.Providencia, S.A.Moszkowski, J.da Providencia, H.Bohr Neutron stars within the Bogoliubov quark-meson coupling model
doi: 10.1103/PhysRevC.103.035811
2020CU05 Eur.Phys.J. A 56, 295 (2020) T.Custodio, A.Falcao, H.Pais, C.Providencia, F.Gulminelli, G.Ropke Light clusters in warm stellar matter: calibrating the cluster couplings
doi: 10.1140/epja/s10050-020-00302-w
2020MA58 Phys.Rev. C 102, 052801(R) (2020) T.Malik, B.K.Agrawal, C.Providencia, J.N.De Unveiling the correlations of tidal deformability with the nuclear symmetry energy parameters
doi: 10.1103/PhysRevC.102.052801
2020PA23 Phys.Rev.Lett. 125, 012701 (2020) H.Pais, R.Bougault, F.Gulminelli, C.Providencia, E.Bonnet, B.Borderie, A.Chbihi, J.D.Frankland, E.Galichet, D.Gruyer, M.Henri, N.Le Neindre, O.Lopez, L.Manduci, M.Parlog, G.Verde Low Density In-Medium Effects on Light Clusters from Heavy-Ion Data NUCLEAR REACTIONS 124Sn(136Xe, X), 112Sn(124Xe, X), E not given; analyzed available data; deduced chemical constants from heavy-ion collisions.
doi: 10.1103/PhysRevLett.125.012701
2019MA35 Phys.Rev. C 99, 052801 (2019) T.Malik, B.K.Agrawal, J.N.De, S.K.Samaddar, C.Providencia, C.Mondal, T.K.Jha Tides in merging neutron stars: Consistency of the GW170817 event with experimental data on finite nuclei
doi: 10.1103/PhysRevC.99.052801
2019PA29 Phys.Rev. C 99, 055806 (2019) H.Pais, F.Gulminelli, C.Providencia, G.Ropke Full distribution of clusters with universal couplings and in-medium effects NUCLEAR STRUCTURE 2,3H, 3,4He; A=4-12; calculated mass fraction of light- and exotic-clusters within nuclear matter using relativistic mean field framework. Relevance to warm nonhomogeneous matter at subsaturation densities in core-collapse supernova or neutron star mergers.
doi: 10.1103/PhysRevC.99.055806
2018AV04 Phys.Rev. C 98, 025805 (2018) S.Avancini, B.P.Bertolino, A.Rabhi, J.Fang, H.Pais, C.Providencia Stability of the neutron-proton-electron matter under strong magnetic fields: The covariant Vlasov approach
doi: 10.1103/PhysRevC.98.025805
2018MA58 Phys.Rev. C 98, 035804 (2018) T.Malik, N.Alam, M.Fortin, C.Providencia, B.K.Agrawal, T.K.Jha, B.Kumar, S.K.Patra GW170817: Constraining the nuclear matter equation of state from the neutron star tidal deformability
doi: 10.1103/PhysRevC.98.035804
2018PA17 Phys.Rev. C 97, 045805 (2018) H.Pais, F.Gulminelli, C.Providencia, G.Ropke Light clusters in warm stellar matter: Explicit mass shifts and universal cluster-meson couplings
doi: 10.1103/PhysRevC.97.045805
2017AL21 Phys.Rev. C 95, 055808 (2017) N.Alam, H.Pais, C.Providencia, B.K.Agrawal Warm unstable asymmetric nuclear matter: Critical properties and the density dependence of the symmetry energy NUCLEAR STRUCTURE 208Pb; calculated binding energy per particle, charge radii, neutron radii, and neutron skin thickness for 208Pb along with the maximum mass of a neutron star and corresponding radius using several relativistic mean-field models.
doi: 10.1103/PhysRevC.95.055808
2017AV02 Phys.Rev. C 95, 045804 (2017) S.S.Avancini, M.Ferreira, H.Pais, C.Providencia, G.Ropke Light clusters and pasta phases in warm and dense nuclear matter
doi: 10.1103/PhysRevC.95.045804
2017FA04 Phys.Rev. C 95, 045802 (2017) J.Fang, H.Pais, S.Pratapsi, S.Avancini, J.Li, C.Providencia Effect of strong magnetic fields on the crust-core transition and inner crust of neutron stars
doi: 10.1103/PhysRevC.95.045802
2017FA06 Phys.Rev. C 95, 062801 (2017) J.Fang, H.Pais, S.Pratapsi, C.Providencia Crust-core transition of a neutron star: Effects of the symmetry energy and temperature under strong magnetic fields
doi: 10.1103/PhysRevC.95.062801
2017FO12 Phys.Rev. C 95, 065803 (2017) M.Fortin, S.S.Avancini, C.Providencia, I.Vidana Hypernuclei and massive neutron stars NUCLEAR STRUCTURE 6He; calculated binding energy of double-Λ 6He hypernucleus as a calibrant using several different models, and compared to experimental data. Construction of unified hyperonic EoS for massive neutron stars with limited number of constraints set by phenomenological models.
doi: 10.1103/PhysRevC.95.065803
2017GR10 Phys.Rev. C 95, 055807 (2017) G.Grams, A.M.Santos, P.K.Panda, C.Providencia, D.P.Menezes Nuclear pasta phases within the quark-meson coupling model
doi: 10.1103/PhysRevC.95.055807
2017ME12 Phys.Rev. C 96, 045803 (2017) Hyperons in the nuclear pasta phase
doi: 10.1103/PhysRevC.96.045803
2016AL25 Phys.Rev. C 94, 052801 (2016) N.Alam, B.K.Agrawal, M.Fortin, H.Pais, C.Providencia, Ad.R.Raduta, A.Sulaksono Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation
doi: 10.1103/PhysRevC.94.052801
2016BO07 Eur.Phys.J. A 52, 58 (2016) I.Bombaci, D.Logoteta, I.Vidana, C.Providencia Quark matter nucleation in neutron stars and astrophysical implications
doi: 10.1140/epja/i2016-16058-5
2016FA14 Phys.Rev. C 94, 062801 (2016) J.Fang, H.Pais, S.Avancini, C.Providencia Larger and more heterogeneous neutron star crusts: A result of strong magnetic fields
doi: 10.1103/PhysRevC.94.062801
2016FO18 Phys.Rev. C 94, 035804 (2016) M.Fortin, C.Providencia, Ad.R.Raduta, F.Gulminelli, J.L.Zdunik, P.Haensel, M.Bejger Neutron star radii and crusts: Uncertainties and unified equations of state
doi: 10.1103/PhysRevC.94.035804
2016FU12 Eur.Phys.J. A 52, 290 (2016) U.J.Furtado, S.S.Avancini, J.R.Marinelli, W.Martarello, C.Providencia Neutrino diffusion in the pasta phase matter within the Thomas-Fermi approach
doi: 10.1140/epja/i2016-16290-y
2016OE01 Eur.Phys.J. A 52, 50 (2016) M.Oertel, F.Gulminelli, C.Providencia, A.R.Raduta Hyperons in neutron stars and supernova cores
doi: 10.1140/epja/i2016-16050-1
2016PA15 Phys.Rev. C 93, 045802 (2016) H.Pais, A.Sulaksono, B.K.Agrawal, C.Providencia Correlation of the neutron star crust-core properties with the slope of the symmetry energy and the lead skin thickness NUCLEAR STRUCTURE 48Ca, 132Sn, 208Pb; calculated total binding energies, charge and neutron radii for selected parametrizations, skin thickness for 208Pb; investigated correlations of crust-core transition density and pressure in neutron stars with the slope of the symmetry energy and neutron skin thickness using different families of mean-field parametrization in relativistic nonlinear Walecka model (NLWM). Asymmetric nuclear and stellar matter at zero temperature.
doi: 10.1103/PhysRevC.93.045802
2016PA26 Phys.Rev. C 93, 065805 (2016) H.Pais, D.P.Menezes, C.Providencia Neutron stars: From the inner crust to the core with the (extended) Nambu-Jona-Lasinio model
doi: 10.1103/PhysRevC.93.065805
2016PA30 Phys.Rev. C 94, 015808 (2016) Vlasov formalism for extended relativistic mean field models: The crust-core transition and the stellar matter equation of state
doi: 10.1103/PhysRevC.94.015808
2015ME05 Phys.Rev. C 91, 065205 (2015); Erratum Phys.Rev. C 97, 029904 (2018) D.P.Menezes, M.B.Pinto, C.Providencia Anisotropy in the equation of state of magnetized quark matter
doi: 10.1103/PhysRevC.91.065205
2015PA28 Phys.Rev. C 91, 055801 (2015) H.Pais, S.Chiacchiera, C.Providencia Light clusters, pasta phases, and phase transitions in core-collapse supernova matter
doi: 10.1103/PhysRevC.91.055801
2015RA06 Phys.Rev. C 91, 045803 (2015) A.Rabhi, M.A.Perez-Garcia, C.Providencia, I.Vidana Magnetic susceptibility and magnetization properties of asymmetric nuclear matter in a strong magnetic field
doi: 10.1103/PhysRevC.91.045803
2014CA04 Eur.Phys.J. A 50, 13 (2014) A.Carbone, A.Polls, C.Providencia, A.Rios, I.Vidana Tensor force effects and high-momentum components in the nuclear symmetry energy
doi: 10.1140/epja/i2014-14013-2
2014DU14 Phys.Rev. C 90, 055203 (2014) M.Dutra, O.Lourenco, S.S.Avancini, B.V.Carlson, A.Delfino, D.P.Menezes, C.Providencia, S.Typel, J.R.Stone Relativistic mean-field hadronic models under nuclear matter constraints
doi: 10.1103/PhysRevC.90.055203
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
2014ME06 Phys.Rev. C 89, 055207 (2014) D.P.Menezes, M.B.Pinto, L.B.Castro, P.Costa, C.Providencia Repulsive vector interaction in three-flavor magnetized quark and stellar matter
doi: 10.1103/PhysRevC.89.055207
2014PA15 Phys.Rev. C 89, 045803 (2014) P.K.Panda, D.P.Menezes, C.Providencia Effects of the symmetry energy on the kaon condensates in the quark-meson coupling model
doi: 10.1103/PhysRevC.89.045803
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
2013DE29 Phys.Rev. C 88, 035804 (2013) R.C.R.de Lima, S.S.Avancini, C.Providencia Effect of strong magnetic fields on the nuclear "pasta" phase structure
doi: 10.1103/PhysRevC.88.035804
2013LO11 Nucl.Phys. A914, 433c (2013) D.Logoteta, I.Vidana, C.Providencia Two-meson exchange hyperonic three-body forces and consequences for neutron stars
doi: 10.1016/j.nuclphysa.2013.01.022
2013LO14 Phys.Rev. C 88, 055802 (2013) D.Logoteta, C.Providencia, I.Vidana Formation of hybrid stars from metastable hadronic stars
doi: 10.1103/PhysRevC.88.055802
2013PR04 Phys.Rev. C 87, 055801 (2013) Interplay between the symmetry energy and the strangeness content of neutron stars
doi: 10.1103/PhysRevC.87.055801
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
2012FE07 Phys.Rev. C 85, 055811 (2012) Description of light clusters in relativistic nuclear models
doi: 10.1103/PhysRevC.85.055811
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
2012LO06 Phys.Rev. C 85, 055807 (2012) D.Logoteta, C.Providencia, I.Vidana, I.Bombaci Quark matter nucleation with a microscopic hadronic equation of state
doi: 10.1103/PhysRevC.85.055807
2012PA12 Phys.Rev. C 85, 055802 (2012) P.K.Panda, A.M.S.Santos, D.P.Menezes, C.Providencia Compact stars within a soft symmetry energy quark-meson-coupling model
doi: 10.1103/PhysRevC.85.055802
2011AV05 Phys.Rev. C 83, 065805 (2011) S.S.Avancini, D.P.Menezes, C.Providencia Finite temperature quark matter under strong magnetic fields
doi: 10.1103/PhysRevC.83.065805
2011CA09 Phys.Rev. C 83, 045201 (2011) R.Cavagnoli, C.Providencia, D.P.Menezes Hadron-quark phase transition in asymmetric matter with boson condensation
doi: 10.1103/PhysRevC.83.045201
2011CA28 Phys.Rev. C 84, 065810 (2011) R.Cavagnoli, D.P.Menezes, C.Providencia Neutron star properties and the symmetry energy
doi: 10.1103/PhysRevC.84.065810
2011DU13 Phys.Rev. C 83, 045810 (2011) C.Ducoin, J.Margueron, C.Providencia, I.Vidana Core-crust transition in neutron stars: Predictivity of density developments
doi: 10.1103/PhysRevC.83.045810
2011PE25 Phys.Rev. C 84, 045803 (2011) M.A.Perez-Garcia, C.Providencia, A.Rabhi Landau parameters for asymmetric nuclear matter with a strong magnetic field
doi: 10.1103/PhysRevC.84.045803
2011RA09 Phys.Rev. C 83, 055801 (2011) Quark matter under strong magnetic fields in chiral models
doi: 10.1103/PhysRevC.83.055801
2011RA28 Phys.Rev. C 84, 035803 (2011) A.Rabhi, P.K.Panda, C.Providencia Warm and dense stellar matter under strong magnetic fields
doi: 10.1103/PhysRevC.84.035803
2011VI07 Phys.Rev. C 84, 062801 (2011) I.Vidana, A.Polls, C.Providencia Nuclear symmetry energy and the role of the tensor force
doi: 10.1103/PhysRevC.84.062801
2010AV06 Phys.Rev. C 82, 025808 (2010) S.S.Avancini, C.C.Barros, D.P.Menezes, C.Providencia α particles and the "pasta" phase in nuclear matter
doi: 10.1103/PhysRevC.82.025808
2010AV08 Phys.Rev. C 82, 055807 (2010); Erratum Phys.Rev. C 85, 059904 (2012) S.S.Avancini, S.Chiacchiera, D.P.Menezes, C.Providencia Warm "pasta" phase in the Thomas-Fermi approximation
doi: 10.1103/PhysRevC.82.055807
2010LE10 Phys.Rev. C 82, 015809 (2010) C.H.Lenzi, A.S.Schneider, C.Providencia, R.M.Marinho Compact stars with a quark core within the Nambu-Jona-Lasinio (NJL) model
doi: 10.1103/PhysRevC.82.015809
2010MA09 Phys.Rev. C 81, 024307 (2010) G.F.Marranghello, C.Providencia, A.M.S.Santos Isospin constraints on the parametric coupling model for nuclear matter
doi: 10.1103/PhysRevC.81.024307
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
2010PA31 Phys.Rev. C 82, 045801 (2010) P.K.Panda, C.Providencia, D.P.Menezes Warm stellar matter within the quark-meson-coupling model
doi: 10.1103/PhysRevC.82.045801
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
2009BO26 Eur.Phys.J. A 41, 355 (2009) H.Bohr, C.Providencia, J.da Providencia Color-symmetric superconductivity in a phenomenological QCD model
doi: 10.1140/epja/i2009-10832-4
2009CH37 Nucl.Phys. A826, 178 (2009) M.Chiapparini, M.E.Bracco, A.Delfino, M.Malheiro, D.P.Menezes, C.Providencia Hadron production in non-linear relativistic mean field models
doi: 10.1016/j.nuclphysa.2009.05.002
2009ME03 Phys.Rev. C 79, 035807 (2009) D.P.Menezes, M.B.Pinto, S.S.Avancini, A.Perez Martinez, C.Providencia Quark matter under strong magnetic fields in the Nambu-Jona-Lasinio model
doi: 10.1103/PhysRevC.79.035807
2009ME19 Phys.Rev. C 80, 065805 (2009) D.P.Menezes, M.B.Pinto, S.S.Avancini, C.Providencia Quark matter under strong magnetic fields in the su(3) Nambu-Jona-Lasinio model
doi: 10.1103/PhysRevC.80.065805
2009PA27 Phys.Rev. C 80, 014905 (2009) P.K.Panda, D.P.Menezes, C.Providencia Particle production within the quark meson coupling model
doi: 10.1103/PhysRevC.80.014905
2009PA39 Phys.Rev. C 80, 045808 (2009) H.Pais, A.Santos, C.Providencia Dynamical instabilities of warm npe matter: δ meson effects
doi: 10.1103/PhysRevC.80.045808
2009RA02 Phys.Rev. C 79, 015804 (2009) A.Rabhi, C.Providencia, J.Da Providencia Spinodal instabilities and the distillation effect in nuclear matter under strong magnetic fields
doi: 10.1103/PhysRevC.79.015804
2009RA20 Phys.Rev. C 80, 025806 (2009) A.Rabhi, C.Providencia, J.Da Providencia Effect of the δ meson on the instabilities of nuclear matter under strong magnetic fields
doi: 10.1103/PhysRevC.80.025806
2009SA16 Phys.Rev. C 79, 045805 (2009) A.M.Santos, C.Providencia, P.K.Panda Low density instabilities in asymmetric nuclear matter within the quark-meson coupling (QMC) model with the δ meson
doi: 10.1103/PhysRevC.79.045805
2009VI07 Phys.Rev. C 80, 045806 (2009) I.Vidana, C.Providencia, A.Polls, A.Rios Density dependence of the nuclear symmetry energy: A microscopic perspective NUCLEAR STRUCTURE 132Sn, 208Pb; calculated neutron skin thickness, and transition densities using microscopic Brueckner-Hartree-Fock approach using the realistic AV18 potential plus a three-body force of Urbana type.
doi: 10.1103/PhysRevC.80.045806
2008AV04 Phys.Rev. C 78, 015802 (2008) S.S.Avancini, D.P.Menezes, M.D.Alloy, J.R.Marinelli, M.M.W.Moraes, C.Providencia Warm and cold pasta phase in relativistic mean field theory
doi: 10.1103/PhysRevC.78.015802
2008DU05 Phys.Rev. C 77, 035201 (2008) M.Dutra, O.Lourenco, A.Delfino, J.S.Sa Martins, C.Providencia, S.S.Avancini, D.P.Menezes Skyrme forces versus relativistic models: Reexamining instabilities
doi: 10.1103/PhysRevC.77.035201
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
2007AV03 Phys.Rev. C 75, 055805 (2007) S.S.Avancini, J.R.Marinelli, D.P.Menezes, M.M.W.Moraes, C.Providencia Density dependent hadronic models and the relation between neutron stars and neutron skin thickness
doi: 10.1103/PhysRevC.75.055805
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
2007ME17 Nucl.Phys. A790, 558c (2007) D.P.Menezes, D.B.Melrose, C.Providencia, K.Wu The QCD phase diagram and the gamma-ray bursts
doi: 10.1016/j.nuclphysa.2007.03.094
2007ME26 Phys.Rev. C 76, 064902 (2007) D.P.Menezes, C.Providencia, M.Chiapparini, M.E.Bracco, A.Delfino, M.Malheiro Constraining relativistic models through heavy ion collisions
doi: 10.1103/PhysRevC.76.064902
2007PA28 Phys.Rev. C 75, 065806 (2007) P.K.Panda, C.Providencia, J.da Providencia Tensor interaction and short range correlations in relativistic nuclear models
doi: 10.1103/PhysRevC.75.065806
2007TS03 Prog.Theor.Phys.(Kyoto) 117, 431 (2007) Y.Tsue, C.Providencia, J.da Providencia, M.Yamamura Semi-Classical Approach to the Two-Level Pairing Model - Various Aspects of Phase Change -
doi: 10.1143/PTP.117.431
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
2006ME05 Phys.Rev. C 73, 025806 (2006) D.P.Menezes, D.B.Melrose, C.Providencia, K.Wu γ-ray bursts and the QCD phase diagram
doi: 10.1103/PhysRevC.73.025806
2006PA14 Phys.Rev. C 73, 035805 (2006) P.K.Panda, J.da Providencia, C.Providencia Short range correlations in relativistic nuclear matter models
doi: 10.1103/PhysRevC.73.035805
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
2006PR07 Prog.Theor.Phys.(Kyoto) 115, 547 (2006) C.Providencia, J.da Providencia, Y.Tsue, M.Yamamura Boson Realization of the su(3)-Algebra. III - Schwinger Representation for the Elliot Model -
doi: 10.1143/PTP.115.547
2006PR08 Prog.Theor.Phys.(Kyoto) 115, 561 (2006) C.Providencia, J.da Providencia, Y.Tsue, M.Yamamura Boson Realization of the su(3)-Algebra. IV - Holstein-Primakoff Representation for the Elliot Model-
doi: 10.1143/PTP.115.561
2006PR10 Prog.Theor.Phys.(Kyoto) 115, 739 (2006) C.Providencia, J.da Providencia, Y.Tsue, M.Yamamura A New Boson Realization of the Two-Level Pairing Model in a Many-Fermion System and Its Classical Counterpart - The Role of the su(2) (x) su(1, 1)-Coherent State in the Schwinger Boson Representation for the su(2) (x) su(2)-Algebra-
doi: 10.1143/PTP.115.739
2006PR11 Prog.Theor.Phys.(Kyoto) 115, 759 (2006) C.Providencia, J.da Providencia, Y.Tsue, M.Yamamura A Note on the Two-Level Pairing Model Obeying the su(2) (x) su(2)-Algebra -Re-formation in Terms of the su(1, 1) (x) su(1, 1)-Algebra
doi: 10.1143/PTP.115.759
2006PR17 Prog.Theor.Phys.(Kyoto) 116, 87 (2006) C.Providencia, J.da Providencia, Y.Tsue, M.Yamamura The Lipkin Model in Many-Fermion System as an Example of the su(1, 1) (X) su(1, 1)-Algebraic Model
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
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