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NSR database version of May 24, 2024.

Search: Author = F.Gulminelli

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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
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2023MO03      Phys.Rev. C 107, 015801 (2023)

C.Mondal, F.Gulminelli

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
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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
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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
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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
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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
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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
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2021FU01      J.Phys.(London) G48, 015102 (2021)

U.J.Furtado, F.Gulminelli

Parametrization of the surface energy in the ETF approximation

doi: 10.1088/1361-6471/abb44b
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2021MA06      Phys.Rev. C 103, 015803 (2021)

S.Mallik, F.Gulminelli

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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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2019MA17      Phys.Rev. C 99, 025806 (2019)

J.Margueron, F.Gulminelli

Effect of high-order empirical parameters on the nuclear equation of state

doi: 10.1103/PhysRevC.99.025806
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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
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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
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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
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2019RA05      Nucl.Phys. A983, 252 (2019)

Ad.R.Raduta, F.Gulminelli

Nuclear Statistical Equilibrium equation of state for core collapse

doi: 10.1016/j.nuclphysa.2018.11.003
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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
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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
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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
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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
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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
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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
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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
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2018RA12      Phys.Rev. C 97, 064309 (2018)

Ad.R.Raduta, F.Gulminelli

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
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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
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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
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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
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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
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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
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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
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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
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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
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Data from this article have been entered in the XUNDL database. For more information, click here.

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
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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
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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
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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
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2015GU25      Phys.Rev. C 92, 055803 (2015)

F.Gulminelli, Ad.R.Raduta

Unified treatment of subsaturation stellar matter at zero and finite temperature

doi: 10.1103/PhysRevC.92.055803
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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2012GU03      Phys.Rev. C 85, 025803 (2012)

F.Gulminelli, Ad.R.Raduta

Ensemble inequivalence in supernova matter within a simple model

doi: 10.1103/PhysRevC.85.025803
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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
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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
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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
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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
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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
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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
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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
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2010RA21      Phys.Rev. C 82, 065801 (2010)

Ad.R.Raduta, F.Gulminelli

Statistical description of complex nuclear phases in supernovae and proto-neutron stars

doi: 10.1103/PhysRevC.82.065801
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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
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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
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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
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2009GU21      Int.J.Mod.Phys. E18, 1022 (2009)

F.Gulminelli, G.Lehaut

From fission to multifragmentation and back

doi: 10.1142/S021830130901318X
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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
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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
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2009RA19      Phys.Rev. C 80, 024606 (2009)

Ad.R.Raduta, F.Gulminelli

Thermodynamics of clusterized matter

doi: 10.1103/PhysRevC.80.024606
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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
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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
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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
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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
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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
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2007GU23      Nucl.Phys. A791, 165 (2007)


Looking for bimodal distributions in multi-fragmentation reactions

doi: 10.1016/j.nuclphysa.2007.03.178
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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
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2007RA01      Phys.Rev. C 75, 024605 (2007)

Ad.R.Raduta, F.Gulminelli

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
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2007RA07      Phys.Rev. C 75, 044605 (2007)

Ad.R.Raduta, F.Gulminelli

Isospin dependent thermodynamics of fragmentation

doi: 10.1103/PhysRevC.75.044605
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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
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2006CH49      Eur.Phys.J. A 30, 317 (2006)

P.Chomaz, F.Gulminelli

The challenges of finite-system statistical mechanics

doi: 10.1140/epja/i2006-10126-5
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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
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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
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2006GU25      Eur.Phys.J. A 30, 253 (2006)

F.Gulminelli, M.D'Agostino

Fluctuations of fragment observables

doi: 10.1140/epja/i2006-10121-x
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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
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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
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2005CH17      Nucl.Phys. A749, 3c (2005)

Ph.Chomaz, F.Gulminelli

Phase Transition in Small System

doi: 10.1016/j.nuclphysa.2004.12.003
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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
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2005GU19      Phys.Rev. C 71, 054607 (2005)

F.Gulminelli, Ph.Chomaz

Distribution of the largest fragment in the lattice gas model

doi: 10.1103/PhysRevC.71.054607
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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
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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
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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
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2004GU05      Nucl.Phys. A734, 581 (2004)

F.Gulminelli, P.Chomaz

Equilibrium under flow

doi: 10.1016/j.nuclphysa.2004.01.107
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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
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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
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2002CH64      Prog.Theor.Phys.(Kyoto), Suppl. 146, 135 (2002)

P.Chomaz, F.Gulminelli

Phase Coexistence in Finite Systems

doi: 10.1143/PTPS.146.135
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