NSR Query Results
Output year order : Descending NSR database version of April 25, 2024. Search: Author = F.Gulminelli Found 133 matches. Showing 1 to 100. [Next]2023DI10 Eur.Phys.J. A 59, 292 (2023) H.Dinh Thi, A.F.Fantina, F.Gulminelli Light clusters in the liquid proto-neutron star inner crust
doi: 10.1140/epja/s10050-023-01199-x
2023MO03 Phys.Rev. C 107, 015801 (2023) Nucleonic metamodeling in light of multimessenger, PREX-II, and CREX data NUCLEAR STRUCTURE 48Ca, 208Pb; calculated posterior probability distributions of binding energies, neutron skin thickness, symmetry energy parameters. Full Bayesian study for static astrophysical observables as well as ground-state finite nuclear properties. Nuclear metamodelling technique used to calculate the ground-state properties of nuclei within the extended Thomas-Fermi (ETF) method.
doi: 10.1103/PhysRevC.107.015801
2023SC06 Phys.Rev. C 107, 045806 (2023) L.Scurto, H.Pais, F.Gulminelli Strong magnetic fields and pasta phases reexamined
doi: 10.1103/PhysRevC.107.045806
2022GI08 Phys.Lett. B 833, 137309 (2022) S.Giraud, L.Canete, B.Bastin, A.Kankainen, A.F.Fantina, F.Gulminelli, P.Ascher, T.Eronen, V.Girard Alcindor, A.Jokinen, A.Khanam, I.D.Moore, D.A.Nesterenko, F.de Oliveira Santos, H.Penttila, C.Petrone, I.Pohjalainen, A.De Roubin, V.A.Rubchenya, M.Vilen, J.Aysto Mass measurements towards doubly magic 78Ni: Hydrodynamics versus nuclear mass contribution in core-collapse supernovae ATOMIC MASSES 74,75Ni, 76,76m,77,78Cu, 79,79mZn; measured cyclotron resonance frequencies using time-of-flight ion-cyclotron-resonance (TOF-ICR) technique at the ISISOL-JYFLTRAP facility of the University of Jyvaskyla; deduced mass excesses, and compared with previously available experimental values and with AME2020 evaluation. Isotopes produced in U(p, F), E=35 MeV at the Ion-Guide Isotope Separator On-Line (IGISOL) facility in Jyvaskyla, followed by mass separation of fission fragments. Z=26-39, N=44-51; systematics of experimental and theoretical values of two-neutron shell-gap energies.
doi: 10.1016/j.physletb.2022.137309
2022MA01 J.Phys.(London) G49, 015102 (2022) S.Mallik, F.GulminellI, D.Gruyer Constraining the density dependence of the symmetry energy: the isospin transport ratio revisited NUCLEAR REACTIONS 58,64Ni(58Ni, X), (64Ni, X), E=52 MeV/nucleon; analyzed available data; deduced isospin diffusion of the quasi-projectile in the framework of the Boltzmann-Uehling-Uhlenbeck transport model.
doi: 10.1088/1361-6471/ac3473
2022PF01 Phys.Rev. C 105, 035802 (2022) A.Pfaff, H.Hansen, F.Gulminelli Bayesian analysis of the properties of hybrid stars with the Nambu--Jona-Lasinio model
doi: 10.1103/PhysRevC.105.035802
2021DI08 Eur.Phys.J. A 57, 296 (2021) H.Dinh Thi, A.F.Fantina, F.Gulminelli The effect of the energy functional on the pasta-phase properties of catalysed neutron stars
doi: 10.1140/epja/s10050-021-00605-6
2021FU01 J.Phys.(London) G48, 015102 (2021) Parametrization of the surface energy in the ETF approximation
doi: 10.1088/1361-6471/abb44b
2021MA06 Phys.Rev. C 103, 015803 (2021) Statistical treatment of nuclear clusters in the continuum NUCLEAR STRUCTURE 2,3,5,7H, 4,6,8,10He; calculated densities of hydrogen and helium isotopes as a function of the global proton fraction at T=5 and 10 MeV at full thermodynamic equilibrium; proposed a protocol to consistently treat the internal nuclear degrees of freedom in the finite-temperature subsaturation equation of state needed to model different dynamical processes such as supernova collapse, proto-neutron star cooling, neutron star mergers, and heavy-ion collisions.
doi: 10.1103/PhysRevC.103.015803
2021MA76 Eur.Phys.J. A 57, 262 (2021) S.Mallik, H.Pais, F.Gulminelli Binding energy shifts from heavy-ion experiments in a nuclear statistical equilibrium model NUCLEAR REACTIONS 124Sn(124Xe, X), E=32 MeV/nucleon; analyzed available data; deduced chemical constants. Comparison with predictions of an extended nuclear statistical equilibrium model including mean-field interactions and in-medium binding energy shifts for the light clusters.
doi: 10.1140/epja/s10050-021-00573-x
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
2020AL23 Phys.Rev. C 102, 064620 (2020) N.Alam, G.Chaudhuri, F.Gulminelli Isospin properties of the pasta phase with an extended statistical model from microscopic energy functionals NUCLEAR STRUCTURE A=40-200; Z=20, 28, 50, 82; Z/N=0.6-1.25; calculated differences between theoretical and experimental energies per particle. A=6-250; calculated average Z/N and multiplicity of the clusters as a function of their size and density, with and without the Coulomb screening effect. Canonical thermodynamical model (CTM) for nuclear multifragmentation, with inputs from the relativistic mean-field energy density functionals. Relevance to cooling dynamics of proto-neutron stars.
doi: 10.1103/PhysRevC.102.064620
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
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
2020PA01 Phys.Rev. C 101, 015803 (2020) A.Pascal, S.Giraud, A.F.Fantina, F.Gulminelli, J.Novak, M.Oertel, A.R.Raduta Impact of electron capture rates for nuclei far from stability on core-collapse supernovae NUCLEAR STRUCTURE Z=10-60, N=20-114; Z=15-55, N-16-90; calculated electron-capture (EC) rates for ≈170 different nuclear species around 86Kr using self-consistent numerical simulations of core-collapse supernovae (CCSN), with hydrodynamic codes COCONUT and ACCEPT.
doi: 10.1103/PhysRevC.101.015803
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
2019BR23 J.Phys.(London) G46, 125101 (2019) M.Bruno, M.D'Agostino, M.V.Managlia, L.Morelli, G.Baiocco, F.Gulminelli, C.Frosin, S.Barlini, A.Buccola, A.Camaiani, G.Casini, M.Cicerchia, M.Cinausero, M.Degerlier, D.Fabris, F.Gramegna, G.Mantovani, T.Marchi, P.Ottanelli, G.Pasquali, S.Piantelli, S.Valdre Four α-particle decay of the excited 16O* quasi-projectile in the 16O + 12C reaction at 130 MeV RADIOACTIVITY 16O(α), (2α) [from 12C(16O, 16O'), E=130 MeV]; measured decay products, Eα, Iα; deduced resonance parameters, branching ratios of the different evaporation channels. NUCLEAR REACTIONS 12C(16O, 16O'), (16O, X), E=130 MeV; measured reaction products, Eα, Iα. 16O, 12C; deduced yields, excitation energies, resonance parameters. Comparison with theoretical calculations.
doi: 10.1088/1361-6471/ab46cd
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
2019CA33 Acta Phys.Pol. B50, 305 (2019) G.Casini, A.Camaiani, L.Morelli, S.Barlini, S.Piantelli, G.Baiocco, M.Bini, M.Bruno, A.Buccola, M.Cinausero, M.Cicerchia, M.D'Agostino, M.Degelier, D.Fabris, C.Frosin, N.Gelli, F.Gramegna, F.Gulminelli, I.Lombardo, T.Marchi, A.Olmi, P.Ottanelli, G.Pasquali, G.Pastore, G.Poggi, S.Valdre, G.Verde Precise Study of Selected Evaporation Chains in Fusion Reactions Between Light Nuclei NUCLEAR REACTIONS 13C(12C, X)25Mg;, E=95 MeV; measured reaction products; deduced branching ratio for various decay chains from excited 25Mg, particles emission order in the O+α+α+n decay chain exploiting Jacobi coordinates. Comparison with statistical model based calculations (GEMINI++ code and MonteCarlo based on Hauser-Feschbach formalism). GARFIELD and RingCounter array at LNL-Legnaro.
doi: 10.5506/aphyspolb.50.305
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
2019MA59 Phys.Rev. C 100, 024611 (2019) S.Mallik, G.Chaudhuri, F.Gulminelli Sensitivity of the evaporation residue observables to the symmetry energy NUCLEAR REACTIONS 58Ni(58Ni, X), 64Ni(64Ni, X), E=50 MeV/nucleon; calculated isotropy of momentum distribution, neutron and proton emission rates, N/Z of light particles emitted as function of time, N/Z, Zmax, Amax, Ek of the heaviest residues and unbound emitted particles; deduced that higher symmetry energy at subsaturation densities give increased size and isotopic ratio for the heaviest residue. Calculations based on Boltzmann-Uehling-Uhlenbeck transport model with Sly5 effective interaction using BUU@VECC-McGill transport code. Relevance to Indra/FAZIA collaboration in an upcoming experiment at GANIL.
doi: 10.1103/PhysRevC.100.024611
2019MO18 Phys.Rev. C 99, 054610 (2019) L.Morelli, M.Bruno, M.D'Agostino, G.Baiocco, F.Gulminelli, S.Barlini, A.Buccola, A.Camaiani, G.Casini, C.Ciampi, C.Frosin, N.Gelli, A.Olmi, P.Ottanelli, G.Pasquali, S.Piantelli, S.Valdre, M.Cicerchia, M.Cinausero, F.Gramegna, G.Mantovani, T.Marchi, M.Degerlier, D.Fabris, V.L.Kravchuk Full disassembly of excited 24Mg into six α particles NUCLEAR REACTIONS 12C(12C, 6α), E=95 MeV; measured Eα, Iα, and α-α relative energy, energy distribution of (24Mg)* distribution for original and reconstructed six-α particle events, angular distribution of α particles using the GARFIELD detector and Ring Counter annular detector for α detection at LNL-Legnaro; deduced important contributions of decay channels, sequential decay with three bodies (α, 8Be/8Be*,12C*) followed by de-excitation in α-particles. Comparison with Hauser-Feshbach predictions including known levels of light nuclei and 8Be* (3 MeV) evaporation.
doi: 10.1103/PhysRevC.99.054610
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
2019RA05 Nucl.Phys. A983, 252 (2019) Nuclear Statistical Equilibrium equation of state for core collapse
doi: 10.1016/j.nuclphysa.2018.11.003
2018CA11 Phys.Rev. C 97, 044607 (2018) A.Camaiani, G.Casini, L.Morelli, S.Barlini, S.Piantelli, G.Baiocco, M.Bini, M.Bruno, A.Buccola, M.Cinausero, M.Cicerchia, M.D'Agostino, M.Degelier, D.Fabris, C.Frosin, F.Gramegna, F.Gulminelli, G.Mantovani, T.Marchi, A.Olmi, P.Ottanelli, G.Pasquali, G.Pastore, S.Valdre, G.Verde Experimental study of precisely selected evaporation chains in the decay of excited 25Mg NUCLEAR REACTIONS 13C(12C, X)25Mg*, E=95 MeV; measured reaction products, Ep, Ip, Eα, Iα, p(θ), α(θ), charge distribution, mass and kinetic energy distributions for protons and α particles in coincidence with Z=6-10 evaporation residues (ER) using GARFIELD and RingCounter array at LNL-Legnaro for particle detection; deduced branching ratio for various decay chains from excited 25Mg, mass distribution of evaporation residues from Q-value distribution, neutron emission order in the O+α+α+n decay chain exploiting Jacobi coordinates. Comparison with statistical model simulation based on Hauser-Feshbach theory, using HFL and GEMINI++ codes, and with 12C(12C, X)24Mg*, E=95 MeV system.
doi: 10.1103/PhysRevC.97.044607
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
2018GR04 Phys.Rev. C 97, 035807 (2018) G.Grams, S.Giraud, A.F.Fantina, F.Gulminelli Distribution of nuclei in equilibrium stellar matter from the free-energy density in a Wigner-Seitz cell
doi: 10.1103/PhysRevC.97.035807
2018MA15 Phys.Rev. C 97, 024606 (2018) S.Mallik, G.Chaudhuri, F.Gulminelli Dynamical and statistical bimodality in nuclear fragmentation NUCLEAR REACTIONS Ca(Ca, X), E=40, 100 MeV/nucleon; calculated variation of average mass of largest cluster and second-largest cluster as function of time, probability distribution, scattering angle and momentum probability distribution of largest cluster, excitation and temperature probability distribution for the largest and second-largest clusters, probability distribution of normalized mass asymmetry using Boltzmann-Uehling-Uhlenbeck (BUU) transport equation coupled to the statistical canonical thermodynamical (CTM) decay model.
doi: 10.1103/PhysRevC.97.024606
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
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
2018RA12 Phys.Rev. C 97, 064309 (2018) Nuclear skin and the curvature of the symmetry energy NUCLEAR STRUCTURE Z=82, A=162-234; calculated binding energies, rms radii of neutron and charge distributions, neutron skin thickness of ground states as a function of total isospin asymmetry, EoS parameters. 208Pb; 48Ca, 48Ni; 50Ni, 50Ti; 52Ni, 52Cr; 54Ni, 54Fe; calculated correlations between neutron skin thickness in 208Pb and differences in the proton radii of mirror nuclei in A=48-54 region. 208Pb; calculated electric dipole polarizability, isovector giant dipole resonance (IVGDR) energy constant, slope of symmetry energy at saturation (Lsym). Extended Thomas-Fermi approximation (ETF) calculations with 17 different Skyrme interactions. Comparison to available experimental results.
doi: 10.1103/PhysRevC.97.064309
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
2017RA02 Phys.Rev. C 95, 025805 (2017) Ad.R.Raduta, F.Gulminelli, M.Oertel Stellar electron capture rates on neutron-rich nuclei and their impact on stellar core collapse
doi: 10.1103/PhysRevC.95.025805
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
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
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
2016MO05 J.Phys.(London) G43, 045110 (2016) L.Morelli, M.Bruno, M.D'Agostino, G.Baiocco, F.Gulminelli, U.Abbondanno, S.Barlini, M.Bini, G.Casini, M.Cinausero, M.Degerlier, D.Fabris, F.Gramegna, J.Mabiala, T.Marchi, A.Olmi, G.Pasquali, S.Piantelli, S.Valdre The 12C* Hoyle state in the inelastic 12C + 12C reaction and in 24Mg* decay NUCLEAR REACTIONS 12C(12C, X)24Mg, E=95 MeV; measured reaction products, Eα, Iα; deduced Hoyle state decay, σ(θ), σ(E), experimental energy Dalitz plots. Comparison with available data.
doi: 10.1088/0954-3899/43/4/045110
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
2016RA05 Phys.Rev. C 93, 025803 (2016) Ad.R.Raduta, F.Gulminelli, M.Oertel Modification of magicity toward the dripline and its impact on electron-capture rates for stellar core collapse NUCLEAR STRUCTURE A=17-80; calculated electron capture rates in stellar environment using extended nuclear statistical equilibrium (NSE) model, possible quenching of N=50 and N=82 shell closures on the electron-capture rates during core collapse. Z=27-68, N=28-98; calculated S(2n) using different mass models and compared with experimental data. Z=10-70, N=10-70; calculated proton and neutron numbers of A≥20 nuclei produced in core-collapsing solar systems as a function of baryonic density. Z<80, N<100; calculated nuclear abundances and compared with experimental mass measurements. Z=22, N=5-65; Z=26, N=10-80; Z=30, N=20-95; Z=36, N=20-100; Z=40, N=20-110; Z=44, N=30-120; calculated LDM-shifted binding energies as function of neutron number for isotopes strongly populated during stellar core collapse. Discussed impact of nuclear binding energies on nuclear abundances, and effect of nuclear structure far from stability on electron-capture probabilities.
doi: 10.1103/PhysRevC.93.025803
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
2015BU14 Phys.Rev. C 92, 055804 (2015) S.Burrello, F.Gulminelli, F.Aymard, M.Colonna, Ad.R.Raduta Heat capacity of the neutron star inner crust within an extended nuclear statistical equilibrium model
doi: 10.1103/PhysRevC.92.055804
2015GU25 Phys.Rev. C 92, 055803 (2015) Unified treatment of subsaturation stellar matter at zero and finite temperature
doi: 10.1103/PhysRevC.92.055803
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
2015MA65 Phys.Rev. C 92, 064605 (2015) S.Mallik, F.Gulminelli, G.Chaudhuri Finite-size effects on the phase diagram of the thermodynamical cluster model
doi: 10.1103/PhysRevC.92.064605
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
2014MO12 J.Phys.(London) G41, 075107 (2014) L.Morelli, G.Baiocco, M.D'Agostino, F.Gulminelli, M.Bruno, U.Abbondanno, S.Appannababu, S.Barlini, M.Bini, G.Casini, M.Cinausero, M.Degerlier, D.Fabris, N.Gelli, F.Gramegna, V.L.Kravchuk, T.Marchi, A.Olmi, G.Pasquali, S.Piantelli, S.Valdre, A.R.Raduta Thermal properties of light nuclei from 12C + 12C fusion-evaporation reactions NUCLEAR REACTIONS 12C(12C, X)24Mg, E=95 MeV/nucleon; measured reaction products, Ep, Ip, Eα, Iα; deduced charged-particles multiplicity distributions, σ(θ), σ(E) for isotopes, branching ratios.
doi: 10.1088/0954-3899/41/7/075107
2014MO13 J.Phys.(London) G41, 075108 (2014) L.Morelli, G.Baiocco, M.D'Agostino, F.Gulminelli, M.Bruno, U.Abbondanno, S.Appannababu, S.Barlini, M.Bini, G.Casini, M.Cinausero, M.Degerlier, D.Fabris, N.Gelli, F.Gramegna, V.L.Kravchuk, T.Marchi, A.Olmi, G.Pasquali, S.Piantelli, S.Valdre, A.R.Raduta Non-statistical decay and α-correlations in the 12C+12C fusion-evaporation reaction at 95 MeV NUCLEAR REACTIONS 12C(12C, X)24Mg, E=95 MeV/nucleon; measured reaction products, Ep, Ip, Eα, Iα, α-α-coin.; deduced α-particles multiplicity distributions, α-α-energy, σ(θ), σ(E) for isotopes, branching ratios. Comparison with Hauser-Feshbach calculations.
doi: 10.1088/0954-3899/41/7/075108
2014RA05 Eur.Phys.J. A 50, 24 (2014) Ad.R.Raduta, F.Aymard, F.Gulminelli Clusterized nuclear matter in the (proto-)neutron star crust and the symmetry energy
doi: 10.1140/epja/i2014-14024-y
2013BA17 Phys.Rev. C 87, 054614 (2013) G.Baiocco, L.Morelli, F.Gulminelli, M.D'Agostino, M.Bruno, U.Abbondanno, S.Barlini, M.Bini, S.Carboni, G.Casini, M.Cinausero, M.Degerlier, F.Gramegna, V.L.Kravchuk, T.Marchi, A.Olmi, G.Pasquali, S.Piantelli, Ad.R.Raduta α-clustering effects in dissipative 12C + 12C reactions at 95 MeV NUCLEAR REACTIONS 12C(12C, X), E=95 MeV; measured Ep, Ip, Eα, Iα, (residues)p-, (residues)α-coin, yields as function of Eα, yield of oxygen isotopes, transmission coefficients using GARFIELD and RCo systems at LNL, Legnaro facility; deduced isotopic, charge, and velocity distributions. Dissipative collision. Cluster correlations. Comparison with Hauser-Feshbach calculation.
doi: 10.1103/PhysRevC.87.054614
2013GU05 Phys.Scr. T152, 014009 (2013) Neutron-rich nuclei and the equation of state of stellar matter
doi: 10.1088/0031-8949/2013/T152/014009
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
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
2012DA01 Nucl.Phys. A875, 139 (2012) M.D'Agostino, M.Bruno, F.Gulminelli, L.Morelli, G.Baiocco, L.Bardelli, S.Barlini, F.Cannata, G.Casini, E.Geraci, F.Gramegna, V.L.Kravchuk, T.Marchi, A.Moroni, A.Ordine, Ad.R.Raduta Towards an understanding of staggering effects in dissipative binary collisions NUCLEAR REACTIONS 58,64Ni(32S, X), E-14.5 MeV/nucleon; measured reaction fragments using GARFILED detector array and ring counter; deduced yield, charge distribution, reaction mechanisms, even-odd effects, correlation functions; calculated yields using GEMINI code.
doi: 10.1016/j.nuclphysa.2011.11.011
2012GU03 Phys.Rev. C 85, 025803 (2012) Ensemble inequivalence in supernova matter within a simple model
doi: 10.1103/PhysRevC.85.025803
2012GU17 Phys.Rev. C 86, 025805 (2012) F.Gulminelli, Ad.R.Raduta, M.Oertel Phase transition toward strange matter
doi: 10.1103/PhysRevC.86.025805
2011DA11 Nucl.Phys. A861, 47 (2011) M.D'Agostino, M.Bruno, F.Gulminelli, L.Morelli, G.Baiocco, L.Bardelli, S.Barlini, F.Cannata, G.Casini, E.Geraci, F.Gramegna, V.L.Kravchuk, T.Marchi, A.Moroni, A.Ordine, Ad.R.Raduta Reaction mechanisms and staggering in S+Ni collisions NUCLEAR REACTIONS 58,64Ni(32S, X), E=463 MeV; measured Z(particle), A(particle), E(particle), I(particle, θ); deduced yields, even-odd effects, flow; calculated yields, even-odd effects, fragment relative velocity using GEMINI code with different assumptions on reaction mechanism and de-excitation chain.
doi: 10.1016/j.nuclphysa.2011.06.017
2011GU25 Phys.Rev. C 84, 065806 (2011) F.Gulminelli, T.Furuta, O.Juillet, C.Leclercq Boundary conditions for star matter and other periodic fermionic systems
doi: 10.1103/PhysRevC.84.065806
2010BO17 Nucl.Phys. A834, 535c (2010) B.Borderie, E.Bonnet, F.Gulminelli, N.Le Neindre, D.Mercier, S.Piantelli, Ad.R.Raduta, M.F.Rivet, B.Tamain, R.Bougault, A.Chbihi, R.Dayras, J.D.Frankland, E.Galichet, F.Gagnon-Moisan, D.Guinet, P.Lautesse, J.Lukasik, M.Parlog, E.Rosato, R.Roy, M.Vigilante, J.P.Wieleczko, and the INDRA and ALADIN Collaboration Multifragmentation and phase transition for hot nuclei: recent progress
doi: 10.1016/j.nuclphysa.2010.01.084
2010FU11 Phys.Rev. C 82, 034307 (2010) T.Furuta, K.H.O.Hasnaoui, F.Gulminelli, C.Leclercq, A.Ono Monopole oscillations in light nuclei with a molecular dynamics approach NUCLEAR STRUCTURE 4He, 12C, 16O, 24Mg, 40Ca; calculated ground state properties, rms radii, monopole oscillation, inverse width optimal value, peak positions of monopole oscillations, AMD density distributions, spectral function, and resonances in the framework of an antisymmetrized version of molecular dynamics as a function of the vibration amplitude (AMD and FMD) with SLy4, SIII, and Gogny effective interactions. Comparison with experimental data.
doi: 10.1103/PhysRevC.82.034307
2010HA20 Nucl.Phys. A834, 571c (2010) K.H.O.Hasnaoui, Ph.Chomaz, F.Gulminelli Fermionic Molecular Dynamics for nuclear dynamics and thermodynamics
doi: 10.1016/j.nuclphysa.2010.01.094
2010NA06 Phys.Rev. C 81, 044619 (2010) P.Napolitani, M.Colonna, F.Gulminelli, E.Galichet, S.Piantelli, G.Verde, E.Vient Probing the nuclear equation of state in heavy-ion collisions at Fermi energy in isospin-sensitive exclusive experiments NUCLEAR REACTIONS 58,68Ni(58Ni, X), E=15, 40 MeV/nucleon; 68Ni(68Ni, X), E=15, 40 MeV/nucleon; calculated isotopic composition of largest fragment, impact parameters versus transverse energy per nucleon, proton and neutron yields within the framework of the Stochastic Mean Field (SMF) model.
doi: 10.1103/PhysRevC.81.044619
2010RA21 Phys.Rev. C 82, 065801 (2010) Statistical description of complex nuclear phases in supernovae and proto-neutron stars
doi: 10.1103/PhysRevC.82.065801
2009BO19 Phys.Rev.Lett. 103, 072701 (2009) E.Bonnet, D.Mercier, B.Borderie, F.Gulminelli, M.F.Rivet, B.Tamain, R.Bougault, A.Chbihi, R.Dayras, J.D.Frankland, E.Galichet, F.Gagnon-Moisan, D.Guinet, P.Lautesse, J.Lukasik, N.Le Neindre, M.Parlog, E.Rosato, R.Roy, M.Vigilante, J.P.Wieleczko, B.Zwieglinski, for the INDRA and ALADIN Collaborations Bimodal Behavior of the Heaviest Fragment Distribution in Projectile Fragmentation NUCLEAR REACTIONS 197Au(197Au, X), E=60, 80, 100 MeV/nucleon; measured charge distribution of reaction fragments; deduced bimodality in the decay pattern. INDRA apparatus.
doi: 10.1103/PhysRevLett.103.072701
2009CH02 Nucl.Phys. A815, 89 (2009) G.Chaudhuri, S.Das Gupta, F.Gulminelli Bimodality and Coulomb effects with a canonical thermodynamic model
doi: 10.1016/j.nuclphysa.2008.11.001
2009CH61 Phys.Rev. C 80, 054606 (2009) G.Chaudhuri, F.Gulminelli, S.Das Gupta Symmetry energy from fragment observables in the canonical thermodynamic model NUCLEAR STRUCTURE 135,149Nd, 202,222Th, 165,186Re; calculated isoscaling parameters as a function of temperature, and symmetry energy of fragmenting source as a function of cluster charge using McGill canonical thermodynamic model (CTM) for heavy-ion collisions.
doi: 10.1103/PhysRevC.80.054606
2009GU21 Int.J.Mod.Phys. E18, 1022 (2009) From fission to multifragmentation and back
doi: 10.1142/S021830130901318X
2009HA38 Int.J.Mod.Phys. E18, 2061 (2009) K.H.O.Hasnaoui, Ph.Chomaz, F.Gulminelli Fermionic molecular dynamics for nuclear dynamics and thermodynamics NUCLEAR STRUCTURE 4He, 6Li, 8Be, 12C, 16O, 40Ca; calculated ground state energy, temperature as a function of the excitation energy per nucleon using Skyrme functional.
doi: 10.1142/S0218301309014299
2009LE07 Phys.Rev.Lett. 102, 142503 (2009) G.Lehaut, F.Gulminelli, O.Lopez Isoscaling as a Measure of Symmetry Energy in the Lattice Gas Model
doi: 10.1103/PhysRevLett.102.142503
2009RA19 Phys.Rev. C 80, 024606 (2009) Thermodynamics of clusterized matter
doi: 10.1103/PhysRevC.80.024606
2008BR10 Nucl.Phys. A807, 48 (2008) M.Bruno, F.Gulminelli, F.Cannata, M.D'Agostino, F.Gramegna, G.Vannini Signals of bimodality in the fragmentation of Au quasi-projectiles NUCLEAR REACTIONS Au(Au, X), E=35 MeV/nucleon; measured projectile-like fission fragments kinetic energy and charge distributions; deduced fission mechanism features.
doi: 10.1016/j.nuclphysa.2008.03.019
2007CH63 Nucl.Phys. A787, 603c (2007) P.Chomaz, C.Ducoin, F.Gulminelli, K.Hasnaoui, P.Napolitani Thermodynamics of compact-star matter within an Ising approach
doi: 10.1016/j.nuclphysa.2006.12.090
2007DU01 Nucl.Phys. A781, 407 (2007) C.Ducoin, Ph.Chomaz, F.Gulminelli Isospin fractionation: Equilibrium versus spinodal decomposition
doi: 10.1016/j.nuclphysa.2006.11.047
2007DU14 Phys.Rev. C 75, 065805 (2007) C.Ducoin, K.H.O.Hasnaoui, P.Napolitani, Ph.Chomaz, F.Gulminelli Anomalous thermodynamics and phase transitions in neutron star matter
doi: 10.1103/PhysRevC.75.065805
2007DU24 Nucl.Phys. A789, 403 (2007) C.Ducoin, Ph.Chomaz, F.Gulminelli Isospin-dependent clusterization of neutron-star matter
doi: 10.1016/j.nuclphysa.2007.03.006
2007GU23 Nucl.Phys. A791, 165 (2007) Looking for bimodal distributions in multi-fragmentation reactions
doi: 10.1016/j.nuclphysa.2007.03.178
2007LE35 Nucl.Phys. A795, 47 (2007) N.Le Neindre, E.Bonnet, J.P.Wieleczko, B.Borderie, F.Gulminelli, M.F.Rivet, R.Bougault, A.Chbihi, R.Dayras, J.D.Frankland, E.Galichet, D.Guinet, P.Lautesse, A.Le Fevre, O.Lopez, J.Lukasik, D.Mercier, J.Moisan, M.Parlog, E.Rosato, R.Roy, C.Schwarz, C.Sfienti, B.Tamain, W.Trautmann, A.Trzcinski, K.Turzo, E.Vient, M.Vigilante, B.Zwieglinski Yield scaling, size hierarchy and fluctuations of observables in fragmentation of excited heavy nuclei NUCLEAR REACTIONS Sn(Xe, X), E=32-50 MeV/nucleon; Au(Au, X), E=80 MeV/nucleon; measured fragment mass, charge and energy distributions. Fisher droplet model analysis and Zipf law applicability to cluster size discussed.
doi: 10.1016/j.nuclphysa.2007.08.011
2007RA01 Phys.Rev. C 75, 024605 (2007) Multifragmentation and the symmetry term of the nuclear equation of state NUCLEAR STRUCTURE 190,200,210Pb; calculated symmetry energy vs fragment charge from excited source.
doi: 10.1103/PhysRevC.75.024605
2007RA07 Phys.Rev. C 75, 044605 (2007) Isospin dependent thermodynamics of fragmentation
doi: 10.1103/PhysRevC.75.044605
2007ZB02 Phys.Rev. C 75, 034612 (2007) K.Zbiri, A.Le Fevre, J.Aichelin, J.Lukasik, W.Reisdorf, F.Gulminelli, U.Lynen, W.F.J.Muller, H.Orth, C.Schwarz, C.Sfienti, W.Trautmann, K.Turzo, B.Zwieglinski, U.Lynen, J.L.Charvet, A.Chbihi, R.Dayras, D.Durand, J.D.Frankland, R.Legrain, N.Le Neindre, O.Lopez, L.Nalpas, M.Parlog, E.Plagnol, M.F.Rivet, E.Rosato, E.Vient, M.Vigilante, C.Volant, J.P.Wieleczko, and the ALADIN and INDRA Collaborations Transition from participant to spectator fragmentation in Au+Au reactions between 60A and 150A NUCLEAR REACTIONS 197Au(197Au, X), E=60-150 MeV/nucleon; analyzed fragment yields, multiplicity, transverse energy, charge, and mass distributions; deduced reaction mechanism features. Quantum molecular dynamics approach.
doi: 10.1103/PhysRevC.75.034612
2006CH49 Eur.Phys.J. A 30, 317 (2006) The challenges of finite-system statistical mechanics
doi: 10.1140/epja/i2006-10126-5
2006DU10 Nucl.Phys. A771, 68 (2006) C.Ducoin, Ph.Chomaz, F.Gulminelli Role of isospin in the nuclear liquid-gas phase transition
doi: 10.1016/j.nuclphysa.2006.03.005
2006GU24 Eur.Phys.J. A 30, 1 (2006) F.Gulminelli, W.Trautmann, S.J.Yennello, Ph.Chomaz Challenges in nuclear dynamics and thermodynamics
doi: 10.1140/epja/i2006-10128-3
2006GU25 Eur.Phys.J. A 30, 253 (2006) Fluctuations of fragment observables
doi: 10.1140/epja/i2006-10121-x
2006PI11 Nucl.Phys. A779, 267 (2006) M.Pichon, B.Tamain, R.Bougault, F.Gulminelli, O.Lopez, E.Bonnet, B.Borderie, A.Chbihi, R.Dayras, J.D.Frankland, E.Galichet, D.Guinet, P.Lautesse, N.Le Neindre, M.Parlog, M.F.Rivet, R.Roy, E.Rosato, E.Vient, M.Vigilante, C.Volant, J.P.Wieleczko, B.Zwieglinski, and the INDRA and ALADIN Collaborations Bimodality: A possible experimental signature of the liquid-gas phase transition of nuclear matter NUCLEAR REACTIONS Sn(Xe, X), Au(Au, X), E=60-100 MeV/nucleon; measured fragments charge distributions, quasi-projectile and quasi-target contributions, transverse energy, correlations; deduced bimodal behavior, possible phase transition features.
doi: 10.1016/j.nuclphysa.2006.08.008
2006TS05 Eur.Phys.J. A 30, 129 (2006); Erratum Eur.Phys.J. A 32, 243 (2007) M.B.Tsang, R.Bougault, R.Charity, D.Durand, W.A.Friedman, F.Gulminelli, A.Le Fevre, Al.H.Raduta, Ad.R.Raduta, S.Souza, W.Trautmann, R.Wada Comparisons of statistical multifragmentation and evaporation models for heavy-ion collisions
doi: 10.1140/epja/i2006-10111-0
2005CH17 Nucl.Phys. A749, 3c (2005) Phase Transition in Small System
doi: 10.1016/j.nuclphysa.2004.12.003
2005DA10 Nucl.Phys. A749, 55c (2005) M.D'Agostino, M.Bruno, F.Gulminelli, F.Cannata, Ph.Chomaz, G.Casini, E.Geraci, F.Gramegna, A.Moroni, G.Vannini Nuclear liquid-gas phase transition: experimental signals NUCLEAR REACTIONS C, Cu, Au(197Au, X), E=25, 35 MeV/nucleon; analyzed fragments yields, charge distributions; 58Ni(32S, X), E=15.5 MeV/nucleon; analyzed charged fragment correlation functions; deduced liquid-gas phase transition features.
doi: 10.1016/j.nuclphysa.2004.12.008
2005GU19 Phys.Rev. C 71, 054607 (2005) Distribution of the largest fragment in the lattice gas model
doi: 10.1103/PhysRevC.71.054607
2005GU39 Phys.Rev. C 72, 064618 (2005) F.Gulminelli, Ph.Chomaz, M.D'Agostino Tracking energy fluctuations from fragment partitions in the lattice gas model
doi: 10.1103/PhysRevC.72.064618
2004CH13 Phys.Rev. C 69, 034610 (2004) A.Chernomoretz, F.Gulminelli, M.J.Ison, C.O.Dorso Enhancement of kinetic energy fluctuations due to expansion
doi: 10.1103/PhysRevC.69.034610
2004DA12 Nucl.Phys. A734, 512 (2004) M.D'Agostino, M.Bruno, F.Gulminelli, R.Bougault, F.Cannata, Ph.Chomaz, F.Gramegna, N.Le Neindre, A.Moroni, G.Vannini Experimental Signals of Phase Transition NUCLEAR REACTIONS C, Cu, Au(197Au, X), E=25, 35 MeV/nucleon; analyzed fragments angular and charge distributions, related data; deduced thermodynamic features.
doi: 10.1016/j.nuclphysa.2004.01.094
2004GU05 Nucl.Phys. A734, 581 (2004) Equilibrium under flow
doi: 10.1016/j.nuclphysa.2004.01.107
2004GU20 Ann.Phys.(Paris) 29, 1 (2004) Phase coexistence in nuclei
2003DA20 Nucl.Phys. A724, 455 (2003) M.D'Agostino, M.Bruno, F.Gulminelli, R.Bougault, F.Cannata, Ph.Chomaz, F.Gramegna, I.Iori, N.Le Neindre, G.V.Margagliotti, A.Moroni, G.Vannini, J.P.Wieleczko Critical-like behaviours in central and peripheral collisions: a comparative analysis NUCLEAR REACTIONS C, Cu(197Au, X), E=25 MeV/nucleon; Cu, Au(197Au, X), E=35 MeV/nucleon; analyzed fragment charge distributions, correlations; deduced parameters, phase transition features.
doi: 10.1016/S0375-9474(03)01541-0
2003GU21 Phys.Rev.Lett. 91, 202701 (2003) F.Gulminelli, Ph.Chomaz, Al.H.Raduta, Ad.R.Raduta Influence of the Coulomb Interaction on the Liquid-Gas Phase Transition and Nuclear Multifragmentation
doi: 10.1103/PhysRevLett.91.202701
2002CH64 Prog.Theor.Phys.(Kyoto), Suppl. 146, 135 (2002) Phase Coexistence in Finite Systems
doi: 10.1143/PTPS.146.135
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