NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = J.Margueron Found 89 matches. 2023CA05 Phys.Rev. C 107, 035805 (2023) B.V.Carlson, M.Dutra, O.Lourenco, J.Margueron Low-energy nuclear physics and global neutron star properties NUCLEAR STRUCTURE 16O, 34Si, 40,48,52,54Ca, 48,56,78Ni, 90Zr, 100,132Sn, 208Pb; calculated binding energies, charge radii, isoscalar giant monopole resonance (ISGMR) centroid energy; deduced symmetry energy parameters, neutron star properties (mass, radius). Calculation testing 415 relativistic mean field and nonrelativistic Skyrme-type interactions.
doi: 10.1103/PhysRevC.107.035805
2023CH43 Eur.Phys.J. A 59, 177 (2023) M.Chamseddine, J.Margueron, G.Chanfray, H.Hansen, R.Somasundaram Relativistic Hartree-Fock chiral Lagrangians with confinement, nucleon finite size and short-range effects
doi: 10.1140/epja/s10050-023-01089-2
2023CH53 Eur.Phys.J. A 59, 264 (2023) G.Chanfray, H.Hansen, J.Margueron Constraints on the in-medium nuclear interaction from chiral symmetry and lattice-QCD
doi: 10.1140/epja/s10050-023-01179-1
2023GU18 Phys.Rev. C 108, 035810 (2023) H.Guven, J.Margueron, K.Bozkurt, E.Khan Characteristics of compact stars determined by gravitational waves, radio-astronomy, x-ray emission, and nuclear physics
doi: 10.1103/PhysRevC.108.035810
2023LI09 Phys.Rev. C 107, 015804 (2023) Z.Lin, A.W.Steiner, J.Margueron Uncertainty quantification for neutrino opacities in core-collapse supernovae and neutron star mergers
doi: 10.1103/PhysRevC.107.015804
2023SO04 Phys.Rev. C 107, 025801 (2023) R.Somasundaram, I.Tews, J.Margueron Investigating signatures of phase transitions in neutron-star cores
doi: 10.1103/PhysRevC.107.025801
2023SO08 Phys.Rev. C 107, L052801 (2023) R.Somasundaram, I.Tews, J.Margueron Perturbative QCD and the neutron star equation of state
doi: 10.1103/PhysRevC.107.L052801
2023YE07 Phys.Rev. C 108, 044312 (2023) J.Ye, J.Margueron, N.Li, W.Z.Jiang Zero-sound modes for the nuclear equation of state at supra-normal densities
doi: 10.1103/PhysRevC.108.044312
2022GR02 Phys.Rev. C 105, 035806 (2022) G.Grams, R.Somasundaram, J.Margueron, S.Reddy Properties of the neutron star crust: Quantifying and correlating uncertainties with improved nuclear physics
doi: 10.1103/PhysRevC.105.035806
2022GR03 Eur.Phys.J. A 58, 56 (2022) G.Grams, J.Margueron, R.Somasundaram, S.Reddy Confronting a set of Skyrme and χEFTpredictions for the crust of neutron stars
doi: 10.1140/epja/s10050-022-00706-w
2022GR10 Phys.Rev. C 106, 044305 (2022) G.Grams, R.Somasundaram, J.Margueron, E.Khan Nuclear incompressibility and speed of sound in uniform matter and finite nuclei NUCLEAR STRUCTURE 98,99,100,101,102,103,104,105,106,107,108,109,110,111,112,113,114,115,116,117,118,119,120,121,122,123,124,125,126,127,128,129,130,131,132,133,134,135,136,137,138,139,140,141,142,143,144,145,146,147,148,149,150,151,152,153,154,155,156,157,158,159,160,161,162Sn, 174,175,176,177,178,179,180,181,182,183,184,185,186,187,188,189,190,191,192,193,194,195,196,197,198,199,200,201,202,203,204,205,206,207,208,209,210,211,212,213,214,215,216,217,218,219,220,221,222,223,224,225,226,227,228,229,230,231,232,233,234,235,236,237,238,239,240,241,242,243,244,245,246,247,248,249,250,251,252,253,254,255,256,257,258,259,260Pb, 90,92,94Zr; calculated surface tension, incompressibility, contributions from the surface and Coulomb terms to the incompressibility, speed of sound in finite nuclei matter. 100,106,114,120Sn, 180,200,208Pb; binding energies, isoscalar giant monopole resonance energy (ISGMR). Compressible liquid-drop model extended with a density-dependent surface term. Bayesian approach coupled to a Markov-Chain Monte Carlo exploration of the parameter space to confront the model predictions. Comparison to experimental results, EDF calculations and AME2020 data.
doi: 10.1103/PhysRevC.106.044305
2022SO05 Europhys.Lett. 138, 14002 (2022) Impact of massive neutron star radii on the nature of phase transitions in dense matter
doi: 10.1209/0295-5075/ac63de
2022SO06 Eur.Phys.J. A 58, 84 (2022) R.Somasundaram, J.Margueron, G.Chanfray, H.Hansen Comparison of different relativistic models applied to dense nuclear matter
doi: 10.1140/epja/s10050-022-00733-7
2021GR10 Few-Body Systems 62, 116 (2021) G.Grams, J.Margueron, R.Somasundaram, S.Reddy Properties of Neutron Star Crust with Improved Nuclear Physics: Impact of Chiral EFT Interactions and Experimental Nuclear Masses
doi: 10.1007/s00601-021-01697-y
2021GU29 Phys.Rev. C 104, 064306 (2021) H.Guven, K.Bozkurt, E.Khan, J.Margueron Ground state properties of charmed hypernuclei within a mean field approach NUCLEAR STRUCTURE 5Li, 17F, 41S, 57Cu, 133Sb, 209Bi; calculated binding energy per baryon for hypernuclei with respect to one of the nucleus without the charmed baryon, and separation energies of Λc hyperons, Fermi energies of neutrons and protons for hypernuclei, contributions of the kinetic energies, interaction and the Coulomb potentials on the Λc separation energies, Λc density distributions, Λc (Λ) single particle energy spectra. Hartree-Fock approach by using three different force sets (NSC89, NSC97a, NSC97f) derived from microscopic Brueckner-Hartree-Fock calculations of hypernuclei. Comparison with available experimental data.
doi: 10.1103/PhysRevC.104.064306
2021MA75 Phys.Rev. C 104, 055803 (2021) J.Margueron, H.Hansen, P.Proust, G.Chanfray Quarkyonic stars with isospin-flavor asymmetry
doi: 10.1103/PhysRevC.104.055803
2021SO13 Phys.Rev. C 103, 045803 (2021) R.Somasundaram, C.Drischler, I.Tews, J.Margueron Constraints on the nuclear symmetry energy from asymmetric-matter calculations with chiral NN and 3N interactions
doi: 10.1103/PhysRevC.103.045803
2020CH29 Phys.Rev. C 102, 024331 (2020) Contribution of the ρ meson and quark substructure to the nuclear spin-orbit potential
doi: 10.1103/PhysRevC.102.024331
2020GU14 Phys.Rev. C 102, 015805 (2020) H.Guven, K.Bozkurt, E.Khan, J.Margueron Multimessenger and multiphysics Bayesian inference for the GW170817 binary neutron star merger
doi: 10.1103/PhysRevC.102.015805
2019CA23 Phys.Rev. C 100, 055803 (2019) T.Carreau, F.Gulminelli, J.Margueron General predictions for the neutron star crustal moment of inertia
doi: 10.1103/PhysRevC.100.055803
2019CA26 Eur.Phys.J. A 55, 188 (2019) T.Carreau, F.Gulminelli, J.Margueron Bayesian analysis of the crust-core transition with a compressible liquid-drop model
doi: 10.1140/epja/i2019-12884-1
2019LI01 Phys.Lett. B 788, 192 (2019) J.J.Li, W.H.Long, J.Margueron, N.Van Giai 48Si: An atypical nucleus? NUCLEAR STRUCTURE 48Si; calculated energy levels, J, π, pairing gap, the onset of doubly magicity using the relativistic Hartree-Fock Lagrangian PKA1.
doi: 10.1016/j.physletb.2018.11.034
2019MA17 Phys.Rev. C 99, 025806 (2019) Effect of high-order empirical parameters on the nuclear equation of state
doi: 10.1103/PhysRevC.99.025806
2019TE02 Eur.Phys.J. A 55, 97 (2019) Confronting gravitational-wave observations with modern nuclear physics constraints
doi: 10.1140/epja/i2019-12774-6
2018GU07 Phys.Rev. C 98, 014318 (2018) H.Guven, K.Bozkurt, E.Khan, J.Margueron ΛΛ pairing in multistrange hypernuclei NUCLEAR STRUCTURE 60Ca, 172Sn, 278Pb; calculated Λ single particle spectra with 20 Λ added in 40Ca, 40 Λ added in 132Sn and 70 Λ added in 208Pb. 40Ca, 132Sn, 208Pb; calculated proton, neutron, and Λ Fermi energies as function of strangeness number, ΛΛ pairing, binding energies, density profiles, and Λ pairing densities. 44,48Ca, 244Pb; calculated single particle spectra with four Λ added in 40Ca, eight Λ added in 40Ca, and 36 Λ added in 208Pb; deduced effect of Λ pairing on the ground state properties of hypernuclei. Hartree-Fock-Bogoliubov (HBF) calculations with SLy5 Skyrme functional for the nucleon-nucleon (NN) channel, and Brueckner-Hartree-Fock calculations with the DF-NSC89, DF-NSC97a and DF-NSC97f functionals for the nucleon-hyperon (NΛ) channel.
doi: 10.1103/PhysRevC.98.014318
2018MA16 Phys.Rev. C 97, 025805 (2018) J.Margueron, R.H.Casali, F.Gulminelli Equation of state for dense nucleonic matter from metamodeling. I. Foundational aspects
doi: 10.1103/PhysRevC.97.025805
2018MA17 Phys.Rev. C 97, 025806 (2018) J.Margueron, R.H.Casali, F.Gulminelli Equation of state for dense nucleonic matter from metamodeling. II. Predictions for neutron star properties
doi: 10.1103/PhysRevC.97.025806
2018RO06 Phys.Rev. C 97, 045804 (2018) A.Roggero, J.Margueron, L.F.Roberts, S.Reddy Nuclear pasta in hot dense matter and its implications for neutrino scattering
doi: 10.1103/PhysRevC.97.045804
2018TE05 Phys.Rev. C 98, 045804 (2018) Critical examination of constraints on the equation of state of dense matter obtained from GW170817
doi: 10.1103/PhysRevC.98.045804
2017BE16 Phys.Rev. C 96, 024304 (2017) M.Belabbas, J.J.Li, J.Margueron Finite-temperature pairing re-entrance in the drip-line nucleus 48Ni NUCLEAR STRUCTURE 48Ni; calculated temperature-averaged proton pairing gap versus temperature based on SLY4-5 and SIII Skyrme interactions, proton pairing gap as function of the temperature based on FT-RHFB PKA1 and PKO3 effective Lagrangians, temperature evolution of proton quasiparticle energies corresponding to states around the Fermi energy. Finite-temperature Hartree-Fock-Bogoliubov (FT-HFB) and relativistic Hartree-Fock-Bogoliubov (FT-RHFB) theories.
doi: 10.1103/PhysRevC.96.024304
2017CH54 Phys.Rev. C 96, 065805 (2017) D.Chatterjee, F.Gulminelli, Ad.R.Raduta, J.Margueron Constraints on the nuclear equation of state from nuclear masses and radii in a Thomas-Fermi meta-modeling approach NUCLEAR STRUCTURE A=20-100; calculated difference between theoretical and experimental energy per particle of symmetric nuclei. Z=20, 28, 50, 82; calculated difference between theoretical and experimental energy per particle vs asymmetry, rms charge radii and neutron skins vs (N-Z)/A; developed a meta-modeling analysis of the correlations of empirical parameters among themselves and with nuclear observables such as masses, radii, and neutron skins using extended Thomas-Fermi approximation.
doi: 10.1103/PhysRevC.96.065805
2017MA73 Phys.Rev. C 96, 054317 (2017) J.Margueron, E.Khan, F.Gulminelli Density Functional approach for multistrange hypernuclei: Competition between Λ and Ξ0, - hyperons NUCLEAR STRUCTURE 6He; calculated parameters and resulting bond energy for double-Λ 6He hypernucleus. 40Ca, 56Ni, 132Sn, 208Pb; calculated binding energies for multi-strange hypernuclei as a function of strangeness number. 12Be, 15C; calculated Ξ- removal energies of 12Be in ground state, and of 15C in its ground and first excited states. 40Ca, 132Sn, 240Pb; calculated Chemical potential for double hypernuclei. Z=10-120, A=20-380; calculated parameter Sinst as defined in the text using different density functionals. Competition between Λ and Ξ hyperons. Nonrelativistic density functional approach, partially constrained by ab initio calculations and experimental data, using DF-NSC89, DF-NSC97a, and DF-NSC97f density functionals.
doi: 10.1103/PhysRevC.96.054317
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
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
2016LI02 Phys.Lett. B 753, 97 (2016) J.J.Li, J.Margueron, W.H.Long, N.Van Giai Magicity of neutron-rich nuclei within relativistic self-consistent approaches NUCLEAR STRUCTURE 24O, 48Si, 52,54Ca; calculated single particle energies, spin orbital splittings; deduce magicity. Relativistic Hartree-Fock-Bogoliubov theory.
doi: 10.1016/j.physletb.2015.12.004
2016NA24 Eur.Phys.J. A 52, 185 (2016) H.Nakada, K.Sugiura, T.Inakura, J.Margueron Can realistic interaction be useful for nuclear mean-field approaches? NUCLEAR STRUCTURE 40,48,52,80Ca; calculated energy difference between p1s1/2 and sp0d3/2 states. Ca, Sn, Pb; calculated isotope shifts. M3Y-type semi-realistic interaction within mean-field approach. Compared with available data.
doi: 10.1140/epja/i2016-16185-y
2016TA05 Phys.Rev. C 93, 035806 (2016) N.H.Tan, D.T.Loan, D.T.Khoa, J.Margueron Mean-field study of hot β-stable protoneutron star matter: Impact of the symmetry energy and nucleon effective mass
doi: 10.1103/PhysRevC.93.035806
2015KH07 Phys.Rev. C 92, 044313 (2015) E.Khan, J.Margueron, F.Gulminelli, Ad.R.Raduta Microscopic evaluation of the hypernuclear chart with Λ hyperons NUCLEAR STRUCTURE 5,6He, 38Si, 144Ce, 210,216,228,248,278Pb; calculated density profiles of hypernuclei. Z≤120; calculated binding energies and the Λ-hypernuclear chart of even-even hypernuclei for Λ=2, 8, 20, 40, 70. 62,68Ni, 110Zr, 144Ce, 278Pb; calculated binding energies of hypernucleons with Λ=2, 6 for Ni, Λ=20 for Zr, Λ=40 for Ce and Λ=70 for Pb. Density-functional approach with microscopic Bruckner-Hartree-Fock calculations and the ΛΛ term treated in a phenomenological way. First microscopic evaluation of the Λ-hypernuclear landscape. Predicted a large number of bound even-even Λ-hypernuclei.
doi: 10.1103/PhysRevC.92.044313
2015LI25 Phys.Rev. C 92, 014302 (2015) J.J.Li, J.Margueron, W.H.Long, N.Van Giai Pairing phase transition: A finite-temperature relativistic Hartree-Fock-Bogoliubov study NUCLEAR STRUCTURE 124Sn; calculated neutron pairing gaps, density, binding energy, compression modulus, symmetry energy, and nonrelativistic effective masses, critical temperature and the occupation number of continuum states, contributions of the continuum states to the pairing and neutron numbers. Z=20-50, N=50; Z=32-76, N=82; Z=52-98, N=126; Z=28, N=22-68; Z=50, N=46-126; Z=82, N=96-184; calculated and compared critical temperatures in FT-RHFB with PKA1, PKO1, DD-ME2 and the Gogny pairing interaction D1S. 68Ni, 174Sn; calculated neutron pairing gaps as a function of temperature using FT-RHFB with Gogny D1S and DDCI pairing forces, and FT-RHF-BCS with DDCI pairing force. 120,160Sn; calculated entropy and specific heat as a function of temperature using FT-RH(F)B and FTRH(F) theories and several different interactions. Self-consistent finite-temperature RHFB (FT-RHFB) theory in a Dirac Woods-Saxon (DWS) basis with a large number of Lagrangians.
doi: 10.1103/PhysRevC.92.014302
2015SE04 Phys.Rev. C 91, 034322 (2015) A.P.Severyukhin, J.Margueron, I.N.Borzov, N.Van Giai Sensitivity of β-decay rates to the radial dependence of the nucleon effective mass NUCLEAR STRUCTURE 208Pb; calculated proton and neutron effective masses as function of radial distance, surface-peaked effective mass (SPEM) effects on giant quadrupole resonance strength (GQR), Gamow-Teller resonance (GTR), and B(E2) for first 2+ state. Skyrme energy density functional (EDFs) with several parameterizations. Comparison with experimental data for B(E2). RADIOACTIVITY 78Ni, 132Sn(β-), 100Sn(β+); calculated energy differences between the dominant single-particle states in 100Sn and 132Sn, surface-peaked effective mass (SPEM) effects on T1/2 and Gamow-Teller strength, Skyrme energy density functional (EDFs) with several parameterizations. Comparison with experimental data for decay rates.
doi: 10.1103/PhysRevC.91.034322
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
2014MA11 Eur.Phys.J. A 50, 18 (2014) J.Margueron, E.Khan, G.Colo, K.Hagino, H.Sagawa Effect of pairing on the symmetry energy and the incompressibility NUCLEAR STRUCTURE 120Sn; calculated mass excess, pairing correlations, incompressibility, symmetry energy using HFB modeling with different pairing interactions.
doi: 10.1140/epja/i2014-14018-9
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
2014WE02 Phys.Rev. C 89, 044311 (2014) P.Wen, L.-G.Cao, J.Margueron, H.Sagawa Spin-isospin response in finite nuclei from an extended Skyrme interaction NUCLEAR STRUCTURE 48Ca, 90Zr, 208Pb; calculated centroid energies of low and high energy peaks of Gamow-Teller (GT) response functions, RPA response function and energies of GT and magnetic dipole excitations with and without spin-density dependent terms. Fully self-consistent Hartree-Fock (HF) plus random phase approximation (RPA) with Skyrme interaction with spin and spin-isospin densities. Comparison with experimental data.
doi: 10.1103/PhysRevC.89.044311
2013GU18 Phys.Rev. C 87, 055809 (2013) F.Gulminelli, Ad.R.Raduta, M.Oertel, J.Margueron Strangeness-driven phase transition in (proto-)neutron star matter
doi: 10.1103/PhysRevC.87.055809
2013KH14 Phys.Rev. C 88, 034319 (2013) Determination of the density dependence of the nuclear incompressibility NUCLEAR STRUCTURE 120Sn, 208Pb; calculated equation of state (EoS) incompressibility K(ρ), centroids of the isoscalar giant monopole resonances (GMR) as functions of K(ρ), and density-dependent incompressibility Mc around the crossing density using various relativistic and nonrelativistic density functionals, and local density approximation (LDA).
doi: 10.1103/PhysRevC.88.034319
2013NA17 Phys.Rev. C 87, 067305 (2013) H.Nakada, K.Sugiura, J.Margueron Tensor-force effects on single-particle levels and proton bubble structure around the Z or N=20 magic number NUCLEAR STRUCTURE 34Si, 36S, 46Ar, 48Ca; calculated proton density distributions. Z=20, N=20-28, 40, 50; calculated single particle energy differences between 1s1/2 and 0d3/2 proton orbitals, tensor force effects. 34Si; possible proton bubble structure. Hartree-Fock (HF) and Hartree-Fock-Bogolyubov (HFB) calculations using semirealistic NN interactions including a realistic tensor force.
doi: 10.1103/PhysRevC.87.067305
2013PA25 Phys.Rev. C 88, 034314 (2013) A.Pastore, J.Margueron, P.Schuck, X.Vinas Pairing in exotic neutron-rich nuclei near the drip line and in the crust of neutron stars NUCLEAR STRUCTURE Z=20, A=36-120; Z=28, A=52-128; Z=40, A=80-240; Z=42, A=82-162; Z=50, A=100-250; Z=82, A=178-342; 66,68,70Ca; 122,124,126,128,130,166,250,500Zr; calculated pairing energies, neutron pairing gaps, single-particle energies and other properties for neutron drip line nuclei immersed in low-density gas of neutrons in outer crust of neutron stars. Skyrme energy density functional theory with density-dependent contact interaction, and Gogny finite range pairing functionals interactions. Hartree-Fock-Bogoliubov and BCS approaches compared. Strong impact of resonances in the continuum on pairing properties of drip line nuclei.
doi: 10.1103/PhysRevC.88.034314
2013PA31 Phys.Rev. C 88, 045805 (2013) P.Papakonstantinou, J.Margueron, F.Gulminelli, Ad.R.Raduta Densities and energies of nuclei in dilute matter at zero temperature NUCLEAR STRUCTURE Z=20, N=15-3000; Z=28, N=40-3000; Z=40, N=40-4000; Z=50, N=40-4000; Z=82, N=80-4000; calculated ground-state density profiles, energies of medium-mass and heavy clusters in a dilute nucleon gas such as in stellar matter in the cores of supernovae and in the crust of neutron stars.
doi: 10.1103/PhysRevC.88.045805
2012KH08 Phys.Rev.Lett. 109, 092501 (2012) Constraining the Nuclear Equation of State at Subsaturation Densities NUCLEAR STRUCTURE 208Pb; calculated matter density, energy per unit of volume at the crossing density. Comparison with available data.
doi: 10.1103/PhysRevLett.109.092501
2012MA43 Prog.Theor.Phys.(Kyoto), Suppl. 196, 172 (2012) J.Margueron, M.Grasso, S.Goriely, G.Colo, H.Sagawa Extended Skyrme Interaction in the Spin Channel NUCLEAR STRUCTURE 41,42,49,50Ca; calculated total energy, mean field, spin-orbit, Coulomb and kinetic contributions to the total energy. Skyrme interactions.
doi: 10.1143/PTPS.196.172
2012MA58 Phys.Rev. C 86, 065801 (2012) Suppression, persistence, and reentrance of superfluidity near and beyond the neutron drip NUCLEAR STRUCTURE N=20-300, Z=28, 36, 38, 40, 42, 44, 50, 52; calculated neutron pairing gaps versus neutron density for neutron drip-line nuclei. 160,176,180,200Sn; calculated temperature-averaged neutron pairing gap versus temperature. Superfluid reentrant effect. Role of continuum coupling in suppression, persistence, and reentrance of pairing. HFB approach, Wigner-Seitz cells modeling.
doi: 10.1103/PhysRevC.86.065801
2012YA12 Phys.Rev. C 86, 034333 (2012) M.Yamagami, J.Margueron, H.Sagawa, K.Hagino Isoscalar and isovector density dependence of the pairing functional determined from global fitting NUCLEAR STRUCTURE N>8, Z>8; calculated pair-density functional (pair-DF) with isoscalar and isovector density dependences using experimental neutron and proton pairing gaps for even-even nuclides of N, Z>8.
doi: 10.1103/PhysRevC.86.034333
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
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. SkyrmeHartree-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
2011LO16 Phys.Rev. C 83, 065809 (2011) D.T.Loan, N.H.Tan, Dao T.Khoa, J.Margueron Equation of state of neutron star matter, and the nuclear symmetry energy
doi: 10.1103/PhysRevC.83.065809
2011PL01 Phys.Rev. C 83, 034613 (2011) E.Pllumbi, M.Grasso, D.Beaumel, E.Khan, J.Margueron, J.van de Wiele Probing the pairing interaction through two-neutron transfer reactions NUCLEAR REACTIONS 124,136Sn(p, t), E=15-35 MeV; analyzed differential σ, σ(θ), form factors, σ(g.s.)/σ(excited 0+) using one-step distorted-wave Born approximation (DWBA) with HFB+QRPA for transition densities and form factors.
doi: 10.1103/PhysRevC.83.034613
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
2010GR05 Phys.Rev. C 82, 014315 (2010) P.Grygorov, E.N.E.van Dalen, H.Muther, J.Margueron Separable form of a low-momentum realistic NN interaction
doi: 10.1103/PhysRevC.82.014315
2010KH03 Phys.Rev. C 82, 024322 (2010) E.Khan, J.Margueron, G.Colo, K.Hagino, H.Sagawa Effect of pairing correlations on incompressibility and symmetry energy in nuclear matter and finite nuclei NUCLEAR STRUCTURE 114,120Sn, 208Pb; calculated effects of pairing correlations on incompressibility and symmetry energy using a microscopic constrained-HFB approach with several pairing functionals. Evaluated pairing effect on the centroid energies of the isoscalar giant monopole resonances (GMR) in Pb and Sn isotopes.
doi: 10.1103/PhysRevC.82.024322
2009CH03 Phys.Rev. C 79, 012801 (2009) Neutron specific heat in the crust of neutron stars from the nuclear band theory NUCLEAR STRUCTURE Z=40, N=160, 210, 280; calculated neutron-specific heat using band theory of solids with Skyrme nucleon-nucleon interaction.
doi: 10.1103/PhysRevC.79.012801
2009GR16 Int.J.Mod.Phys. E18, 2009 (2009) M.Grasso, E.Khan, J.Margueron, N.Van Giai, L.Gaudefroy, T.Niksic, D.Vretenar, J.Piekarewicz, O.Sorlin Bubbles in exotic nuclei NUCLEAR STRUCTURE 46,68Ar; calculated proton densities with SkI5, SLy4 interactions in the HF approach.
doi: 10.1142/S0218301309014184
2009KH08 Phys.Rev. C 80, 044328 (2009) Constraining the nuclear pairing gap with pairing vibrations NUCLEAR STRUCTURE 124,136Sn; analyzed neutron quasiparticle states, response functions and neutron transition densities using Hartree-Fock-Bogoliubov (HFB) model and quasiparticle random-phase approximation (QRPA).
doi: 10.1103/PhysRevC.80.044328
2009MA66 Int.J.Mod.Phys. E18, 2098 (2009) Extended Skyrme interaction for spin channels
doi: 10.1142/S0218301309014366
2009SA47 Int.J.Mod.Phys. E18, 2035 (2009) H.Sagawa, J.Margueron, K.Hagino Pairing correlations in unstable nuclei and BCS-BED crossover
doi: 10.1142/S021830130901424X
2008DU11 Nucl.Phys. A809, 30 (2008) C.Ducoin, J.Margueron, Ph.Chomaz Cluster formation in asymmetric nuclear matter: Semi-classical and quantal approaches
doi: 10.1016/j.nuclphysa.2008.05.015
2008GR13 Nucl.Phys. A807, 1 (2008) M.Grasso, E.Khan, J.Margueron, N.Van Giai Low-energy excitations in nuclear systems: From exotic nuclei to the crust of neutron stars NUCLEAR STRUCTURE Z=40, 50; calculated neutron densities, quadrupole strength distributions using QRPA in relation to neutron stars.
doi: 10.1016/j.nuclphysa.2008.04.003
2008KH01 Nucl.Phys. A800, 37 (2008) E.Khan, M.Grasso, J.Margueron, N.Van Giai Detecting bubbles in exotic nuclei NUCLEAR STRUCTURE 46Ar; calculated proton density, monopole, dipole and quadrupole strength functions using Hartree-Fock approach.
doi: 10.1016/j.nuclphysa.2007.11.012
2008MA17 Phys.Rev. C 77, 054309 (2008) J.Margueron, H.Sagawa, K.Hagino Effective pairing interactions with isospin density dependence NUCLEAR STRUCTURE 36,37,38,39,40,41,42,43,44,45,46,47,48,49,50,51,52,53,54,55,56,57,58,59,60,61,62Ca, 52,53,54,55,56,57,58,59,60,61,62,63,64,65,66,67,68,69,70,71,72,73,74,75,76,77,78,79,80,81,82,83,84,85,86,87,88,89,90Ni, 100,101,102,103,104,105,106,107,108,109,110,111,112,113,114,115,116,117,118,119,120,121,122,123,124,125,126,127,128,129,130,131,132,133,134,135,136,137,138,139,140,141,142,143,144,145,146,147,148,149,150,151,152,153,154,155,156,157,158,159,160,161,162,163,164,165,166,167,168,169,170Sn, 182,183,184,185,186,187,188,189,190,191,192,193,194,195,196,197,198,199,200,201,202,203,204,205,206,207,208,209,210,211,212,213,214,215,216,217,218,219,220,221,222,223,224,225,226,227,228,229,230,231,232,233,234,235,236,237,238,239,240,241,242,243,244,245,246,247,248,249,250,251,252,253,254,255,256,257,258,259,260,261,262,263,264,265,266,267Pb; calculated odd-even mass staggering, binding energies, two-neutron separation energies, pairing gaps. Comparison with experimental data. 110,150Sn; calculated particle densities, neutron Fermi momentum. Hartree-Fock-Bogoliubov model.
doi: 10.1103/PhysRevC.77.054309
2008MA20 Phys.Rev. C 77, 064306 (2008) J.Margueron, J.Navarro, Nguyen Van Giai, P.Schuck Continued fraction approximation for the nuclear matter response function
doi: 10.1103/PhysRevC.77.064306
2007CH44 Phys.Rev. C 75, 055806 (2007) N.Chamel, S.Naimi, E.Khan, J.Margueron Validity of the Wigner-Seitz approximation in neutron star crust
doi: 10.1103/PhysRevC.75.055806
2007GR21 Phys.Rev. C 76, 044319 (2007) M.Grasso, Z.Y.Ma, E.Khan, J.Margueron, N.Van Giai Evolution of the proton sd states in neutron-rich Ca isotopes NUCLEAR STRUCTURE 48,52,70,78Ca; calculated excitation energies. Skyrme-Hartree-Fock equations used.
doi: 10.1103/PhysRevC.76.044319
2007MA68 Phys.Rev. C 76, 034309 (2007) J.Margueron, E.van Dalen, C.Fuchs Low densities in asymmetric nuclear matter
doi: 10.1103/PhysRevC.76.034309
2007MA84 Phys.Rev. C 76, 064316 (2007) J.Margueron, H.Sagawa, K.Hagino BCS-BEC crossover of neutron pairs in symmetric and asymmetric nuclear matter
doi: 10.1103/PhysRevC.76.064316
2007MO21 Phys.Rev. C 75, 065807 (2007) C.Monrozeau, J.Margueron, N.Sandulescu Nuclear superfluidity and cooling time of neutron star crusts
doi: 10.1103/PhysRevC.75.065807
2006BA67 Eur.Phys.J. A 30, 141 (2006) Instabilities in nuclear matter and finite nuclei
doi: 10.1140/epja/i2006-10112-y
2006MA42 Phys.Rev. C 74, 015805 (2006) J.Margueron, N.Van Giai, J.Navarro Effects of spin-orbit interaction on nuclear response and neutrino mean free path
doi: 10.1103/PhysRevC.74.015805
2005BO17 Ann.Phys.(New York) 318, 245 (2005) P.Bozek, J.Margueron, H.Muther Dynamical response functions in correlated fermionic systems
doi: 10.1016/j.aop.2005.01.001
2005MA08 Phys.Rev. C 71, 024318 (2005) Supersymmetry transformation for excitation processes
doi: 10.1103/PhysRevC.71.024318
2005MA74 Phys.Rev. C 72, 034311 (2005) J.Margueron, N.Van Giai, J.Navarro Nuclear response functions in homogeneous matter with finite range effective interactions
doi: 10.1103/PhysRevC.72.034311
2004MA73 Phys.Rev. C 70, 028801 (2004) J.Margueron, J.Navarro, P.Blottiau Nuclear liquid-gas phase transition and supernovae evolution
doi: 10.1103/PhysRevC.70.028801
2003CH74 Nucl.Phys. A722, 315c (2003) Chemical and mechanical spinodals a unique liquid-gas instability
doi: 10.1016/S0375-9474(03)01383-6
2003MA15 Phys.Rev. C 67, 041602 (2003) A unique spinodal region in asymmetric nuclear matter
doi: 10.1103/PhysRevC.67.041602
2003MA20 Nucl.Phys. A720, 337 (2003); Erratum Nucl.Phys. A741, 381 (2004) J.Margueron, A.Bonaccorso, D.M.Brink A non-perturbative approach to halo breakup NUCLEAR REACTIONS 208Pb(11Be, n10Be), E=72 MeV/nucleon; 208Pb(19C, n18C), E=67 MeV/nucleon; calculated neutron spectra relative to core fragment. 197Au(11Be, n10Be), E=41 MeV/nucleon; calculated neutron σ(θ). Coulomb and nuclear contributions, high-order effects discussed. Comparison with data.
doi: 10.1016/S0375-9474(03)01092-3
2003MA49 Nucl.Phys. A719, 169c (2003) J.Margueron, J.Navarro, N.Van Giai Neutrino mean free path and in-medium nuclear interaction
doi: 10.1016/S0375-9474(03)00987-4
2003MA76 Phys.Rev. C 68, 055806 (2003) J.Margueron, I.Vidana, I.Bombaci Microscopic calculation of the neutrino mean free path inside hot neutron matter
doi: 10.1103/PhysRevC.68.055806
2002FA02 Nucl.Phys. A700, 70 (2002) M.Fallot, J.A.Scarpaci, D.Lacroix, Ph.Chomaz, J.Margueron Coulomb versus Nuclear Break-Up of 11Be Halo Nucleus in a Nonperturbative Framework NUCLEAR REACTIONS 9Be, 48Ti, 197Au(11Be, n10Be), E=41 MeV/nucleon; calculated σ(θ), σ, Coulomb and nuclear contributions, neutron-core relative energy. 11Be deduced halo features. Time-dependent quantum calculation, comparison with data.
doi: 10.1016/S0375-9474(01)01303-3
2002MA26 Nucl.Phys. A703, 105 (2002) J.Margueron, A.Bonaccorso, D.M.Brink Coulomb-Nuclear Coupling and Interference Effects in the Breakup of Halo Nuclei NUCLEAR REACTIONS 9Be, 48Ti, 197Au(11Be, n10Be), E=30, 41, 120 MeV/nucleon; 208Pb(11Be, n10Be), E=72 MeV/nucleon; calculated neutron spectra, σ(E, θ), integrated breakup σ; deduced role of Coulomb-nuclear coupling and interference effects.
doi: 10.1016/S0375-9474(01)01336-7
2002MA49 Phys.Rev. C66, 014303 (2002) J.Margueron, J.Navarro, V.G.Nguyen Instabilities of Infinite Matter with Effective Skyrme-Type Interactions
doi: 10.1103/PhysRevC.66.014303
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