NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = D.P.Menezes Found 94 matches. 2023PE14 Eur.Phys.J. A 59, 209 (2023) M.R.Pelicer, D.P.Menezes, M.Dutra, O.Lourenco Do short range correlations inhibit the appearance of the nuclear pasta?
doi: 10.1140/epja/s10050-023-01122-4
2022MA48 Phys.Rev. C 106, 035801 (2022) K.D.Marquez, M.R.Pelicer, S.Ghosh, J.Peterson, D.Chatterjee, V.Dexheimer, D.P.Menezes Exploring the effects of Δ baryons in magnetars
doi: 10.1103/PhysRevC.106.035801
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
2022PE17 Eur.Phys.J. A 58, 177 (2022) Phase transitions and latent heat in magnetized matter
doi: 10.1140/epja/s10050-022-00829-0
2021BA33 Eur.Phys.J. A 57, 229 (2021) B.C.T.Backes, K.D.Marquezb, D.P.Menezes Effects of strong magnetic fields on the hadron-quark deconfinement transition
doi: 10.1140/epja/s10050-021-00544-2
2021DE26 Eur.Phys.J. A 57, 216 (2021) V.Dexheimer, K.D.Marquez, D.P.Menezes Delta baryons in neutron-star matter under strong magnetic fields
doi: 10.1140/epja/s10050-021-00532-6
2021LO06 Nucl.Phys. A1009, 122171 (2021) Broken SU(6) symmetry and massive hybrid stars
doi: 10.1016/j.nuclphysa.2021.122171
2021PE11 Phys.Rev. C 104, L022801 (2021) M.R.Pelicer, D.P.Menezes, C.C.Barros, F.Gulminelli Fluctuations in the nuclear pasta phase
doi: 10.1103/PhysRevC.104.L022801
2020BA19 Phys.Rev. C 101, 035211 (2020) C.C.Barros, D.P.Menezes, F.Gulminelli Fluctuations in the composition of nuclear pasta in symmetric nuclear matter at finite temperature
doi: 10.1103/PhysRevC.101.035211
2020LO04 Eur.Phys.J. A 56, 32 (2020) O.Lourenco, M.Dutra, C.H.Lenzi, S.K.Biswal, M.Bhuyan, D.P.Menezes Consistent Skyrme parametrizations constrained by GW170817
doi: 10.1140/epja/s10050-020-00040-z
2020LO07 Eur.Phys.J. A 56, 122 (2020) Role of vector channel in different classes of (non) magnetized neutron stars
doi: 10.1140/epja/s10050-020-00125-9
2019LO05 Phys.Rev. C 99, 045202 (2019) O.Lourenco, M.Dutra, C.H.Lenzi, C.V.Flores, D.P.Menezes Consistent relativistic mean-field models constrained by GW170817
doi: 10.1103/PhysRevC.99.045202
2018DE19 Phys.Rev. C 97, 055205 (2018) T.de Oliveira, D.P.Menezes, Ma.B.Pinto, F.Gulminelli Role of strangeness and isospin in low density expansions of hadronic matter
doi: 10.1103/PhysRevC.97.055205
2017CA30 Eur.Phys.J. A 53, 191 (2017) P.H.G.Cardoso, T.Nunes da Silva, A.Deppman, D.P.Menezes Quark matter revisited with non-extensive MIT bag model
doi: 10.1140/epja/i2017-12388-0
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
2017LO06 Phys.Rev. C 95, 065212 (2017) O.Lourenco, M.Dutra, D.P.Menezes Critical parameters of consistent relativistic mean-field models
doi: 10.1103/PhysRevC.95.065212
2017ME12 Phys.Rev. C 96, 045803 (2017) Hyperons in the nuclear pasta phase
doi: 10.1103/PhysRevC.96.045803
2017TO01 Phys.Rev. C 95, 025201 (2017) J.R.Torres, F.Gulminelli, D.P.Menezes Examination of strangeness instabilities and effects of strange meson couplings in dense strange hadronic matter and compact stars
doi: 10.1103/PhysRevC.95.025201
2016DU05 Phys.Rev. C 93, 025806 (2016); Erratum Phys.Rev. C 94, 049901 (2016) M.Dutra, O.Lourenco, D.P.Menezes Stellar properties and nuclear matter constraints
doi: 10.1103/PhysRevC.93.025806
2016ME04 Eur.Phys.J. A 52, 17 (2016) Quark matter under strong magnetic fields
doi: 10.1140/epja/i2016-16017-2
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
2016TO03 Phys.Rev. C 93, 024306 (2016) J.R.Torres, F.Gulminelli, D.P.Menezes Liquid-gas phase transition in strange hadronic matter with relativistic models
doi: 10.1103/PhysRevC.93.024306
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
2015ME11 Eur.Phys.J. A 51, 155 (2015) D.P.Menezes, A.Deppman, E.Megias, L.B.Castro Non-extensive thermodynamics and neutron star properties
doi: 10.1140/epja/i2015-15155-3
2014CA01 Phys.Rev. C 89, 015805 (2014) R.H.Casali, L.B.Castro, D.P.Menezes Hadronic and hybrid stars subject to density-dependent magnetic fields
doi: 10.1103/PhysRevC.89.015805
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
2014LO05 Phys.Rev. C 89, 025805 (2014) Hypernuclear matter in a complete SU(3) symmetry group
doi: 10.1103/PhysRevC.89.025805
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
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
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
2011AL07 Phys.Rev. C 83, 035803 (2011) Nuclear "pasta phase" on neutrino opacities
doi: 10.1103/PhysRevC.83.035803
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
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
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
2010PA38 Eur.Phys.J. A 46, 413 (2010) The importance of the mixed phase in hybrid stars built with the Nambu-Jona-Lasinio model
doi: 10.1140/epja/i2010-11059-0
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
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
2009ME21 Eur.Phys.J. A 42, 97 (2009) D.P.Menezes, S.S.Avancini, C.Z.Vasconcellos, M.Razeira φ meson effects in the Nolen-Schiffer anomaly NUCLEAR STRUCTURE 41Ca, 41Sc; calculated binding energy, radii, surface energy, proton skin thickness. 17O, 17F, 27Al, 21Si, 39K, 39Ca, 41Ca, 41Sc, 81Zr, 81Nb; A=501; calculated mass differences between mirror nuclei pairs. Comparison of four relativistic models and data.
doi: 10.1140/epja/i2009-10848-8
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
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
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
2007AV06 Phys.Rev. C 76, 064318 (2007) S.S.Avancini, J.R.Marinelli, D.P.Menezes, M.M.W.Moraes, A.S.Schneider Reexamining the neutron skin thickness within a density dependent hadronic model NUCLEAR STRUCTURE 40,48Ca, 66Ni, 90Zr, 208Pb; calculated neutron skin thickness, binding energy, surface energy, density, electron scattering cross sections, asymmetry using Walecka Model.
doi: 10.1103/PhysRevC.76.064318
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
2006AV05 Phys.Rev. C 74, 015201 (2006) Density dependent parametrization models: Formalism and applications
doi: 10.1103/PhysRevC.74.015201
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
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
2005AV08 Braz.J.Phys. 35, 861 (2005) S.S.Avancini, F.F.de Souza Cruz, J.R.Marinelli, D.P.Menezes, M.M.Watanabe de Moraes Analytical Treatment for the Deuteron-Deuteron Interaction
doi: 10.1590/S0103-97332005000500039
2005ME18 Phys.Rev. C 72, 035802 (2005) D.P.Menezes, P.K.Panda, C.Providencia Kaon condensation in the quark-meson coupling model and compact stars
doi: 10.1103/PhysRevC.72.035802
2005PA11 Phys.Rev. C 71, 015801 (2005) P.K.Panda, D.P.Menezes, C.Providencia, J.da Providencia Aspects of short-range correlations in a relativistic model
doi: 10.1103/PhysRevC.71.015801
2005PA67 Phys.Rev. C 72, 058201 (2005) P.K.Panda, C.Providencia, D.P.Menezes Pentaquarks in the medium in the quark-meson coupling model
doi: 10.1103/PhysRevC.72.058201
2004AV01 J.Phys.(London) G30, 27 (2004) S.S.Avancini, M.E.Bracco, M.Chiapparini, D.P.Menezes On the density-dependent hadron field theory at finite temperature and its thermodynamical consistency
doi: 10.1088/0954-3899/30/2/003
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
2004ME05 Phys.Rev. C 69, 045801 (2004) Warm stellar matter with neutrino trapping
doi: 10.1103/PhysRevC.69.045801
2004ME21 Phys.Rev. C 70, 058801 (2004) δ meson effects on stellar matter
doi: 10.1103/PhysRevC.70.058801
2004PA05 Phys.Rev. C 69, 025207 (2004) P.K.Panda, D.P.Menezes, C.Providencia Hybrid stars in the quark-meson coupling model with superconducting quark matter
doi: 10.1103/PhysRevC.69.025207
2004PA18 Phys.Rev. C 69, 058801 (2004) P.K.Panda, D.P.Menezes, C.Providencia Stellar matter in the quark-meson-coupling model with neutrino trapping
doi: 10.1103/PhysRevC.69.058801
2004SA16 Phys.Rev. C 69, 045803 (2004) Dense and hot matter within the nonlinear Walecka model
doi: 10.1103/PhysRevC.69.045803
2003AV01 Phys.Rev. C 67, 024301 (2003) S.S.Avancini, M.E.Bracco, M.Chiapparini, D.P.Menezes Relativistic mean-field approximation in a density dependent parametrization model at finite temperature
doi: 10.1103/PhysRevC.67.024301
2003ME15 Phys.Rev. C 68, 035804 (2003) Warm stellar matter with deconfinement: Application to compact stars
doi: 10.1103/PhysRevC.68.035804
2003PA24 Phys.Rev. C 68, 015201 (2003) P.K.Panda, G.Krein, D.P.Menezes, C.Providencia Warm asymmetric matter in the quark-meson coupling model
doi: 10.1103/PhysRevC.68.015201
2002ES04 Phys.Rev. C65, 045803 (2002) Relativistic Equations of State in a Thomas-Fermi Approach for Neutron Stars
doi: 10.1103/PhysRevC.65.045803
2002ME15 Phys.Rev. C66, 015206 (2002) ρ-ω Mixing in the Nonlinear Walecka Model NUCLEAR STRUCTURE 41Ca, 41Sc, 67As, 67Se, 81Zr, 81Nb; calculated radii, binding energies, effect of ρ-ω mixing term. Nonlinear Walecka model.
doi: 10.1103/PhysRevC.66.015206
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
2001ME24 Phys.Rev. C64, 044306 (2001) Caloric Curve for Finite Nuclei in Relativistic Models NUCLEAR STRUCTURE 150,166Sm; calculated temperature vs excitation energy. Nonlinear Walecka model.
doi: 10.1103/PhysRevC.64.044306
2000AV03 Phys.Rev. C62, 024312 (2000) S.S.Avancini, F.F.de Souza Cruz, J.R.Marinelli, D.P.Menezes Quonic Expansion and Its Random-Phase Approximation Counterpart
doi: 10.1103/PhysRevC.62.024312
2000KR10 Nucl.Phys. A674, 125 (2000) G.Krein, D.P.Menezes, M.Nielsen, C.Providencia Droplet Formation in Cold Asymmetric Nuclear Matter in the Quark-Meson-Coupling Model
doi: 10.1016/S0375-9474(00)00085-3
2000ME23 Int.J.Mod.Phys. E9, 221 (2000) D.P.Menezes, M.B.Pinto, G.Krein Optimized Delta Expansion for Relativistic Nuclear Models: Renormalization of vacuum fluctuations
doi: 10.1016/S0218-3013(00)00013-1
1999AV06 J.Phys.(London) G25, 1829 (1999) S.S.Avancini, J.R.Marinelli, D.P.Menezes Boson Mapping for a Single j-Shell within the Quon Statistics
doi: 10.1088/0954-3899/25/9/306
1999ME10 Nucl.Phys. A650, 283 (1999) Droplet Formation in Cold Asymmetric Nuclear Matter
doi: 10.1016/S0375-9474(99)00109-8
1999ME18 Phys.Rev. C60, 024313 (1999) Nucleation Process in Asymmetric Hot Nuclear Matter
doi: 10.1103/PhysRevC.60.024313
1998AV01 Int.J.Mod.Phys. E7, 379 (1998) S.S.Avancini, J.R.Marinelli, D.P.Menezes, M.M.Watanabe de Moraes, N.Yoshinaga Exact Dyson Expansion for a Single J-Shell within the Quon Algebra
doi: 10.1142/S0218301398000178
1998KR01 Eur.Phys.J. A 1, 45 (1998) G.Krein, R.S.M.de Carvalho, D.P.Menezes, M.Nielsen, M.B.Pinto Optimized δ Expansion for Relativistic Nuclear Models
doi: 10.1007/s100500050030
1996KR04 Phys.Lett. 370B, 5 (1996) G.Krein, D.P.Menezes, M.B.Pinto Optimized δ Expansion for the Walecka Model
doi: 10.1016/0370-2693(95)01578-7
1995FA20 Int.J.Mod.Phys. E4, 547 (1995) F.W.Favero, L.O.E.Santos, D.P.Menezes The q-Deformed Moszkowski Model Revisited
doi: 10.1142/S0218301395000201
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
1992KR16 Phys.Lett. 294B, 7 (1992) G.Krein, D.P.Menezes, M.Nielsen Rho-Omega Mixing and Neutron-Proton Self-Energies in the Walecka Model NUCLEAR STRUCTURE 1n, 1H; calculated self-energy, mass difference vs fermi momentum. Walecka model.
doi: 10.1016/0370-2693(92)91630-R
1992KR21 Int.J.Mod.Phys. E1, 871 (1992) G.Krein, D.P.Menezes, M.Nielsen In-Medium Neutron-Proton Mass Difference with Nuclear Chiral Models NUCLEAR STRUCTURE 1n, 1H; calculated mass difference. Chiral models, nucleon, meson degrees of freedom.
doi: 10.1142/S0218301392000394
1992ME17 Int.J.Mod.Phys. E1, 397 (1992) D.P.Menezes, A.F.R.De Toledo Piza Comments on Photonuclear Reactions at Intermediate Energies NUCLEAR REACTIONS 16O(γ, p), E=61.9, 82 MeV; calculated σ(θ). Shell model knockout contribution, Woods-Saxon potential.
doi: 10.1142/S0218301392000217
1987DE39 Phys.Rev. C36, 2639 (1987) E.J.V.de Passos, D.P.Menezes, A.P.N.R.Galeao Isovector Excitations of N ≠ Z Nuclei NUCLEAR STRUCTURE 90Zr; calculated isovector resonances, Gamow-Teller transition strength distribution.
doi: 10.1103/PhysRevC.36.2639
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