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NSR database version of April 26, 2024.

Search: Author = M.Grasso

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2022BU10      Eur.Phys.J. A 58, 22 (2022)

S.Burrello, M.Grasso

Finite-temperature infinite matter with effective-field-theory-inspired energy-density functionals

doi: 10.1140/epja/s10050-022-00665-2
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2022GA04      Phys.Rev. C 105, 014321 (2022)

D.Gambacurta, M.Grasso

Quenching of Gamow-Teller strengths and two-particle-two-hole configurations

NUCLEAR STRUCTURE 48Ca, 90Zr, 132Sn, 14C, 22O; calculated Gamow-Teller strengths GT- for 48Ca and 90Zr, GT- SSRPA and RPA discrete spectra for 90Zr and 132Sn, cumulative sums for GT- strengths for 14C and 22O using charge-exchange subtracted second random-phase approximation (SSRPA), based on Skyrme functional SGII for Gamow-Teller resonances in closed-shell and closed-subshell nuclei, with the inclusion of two-particle-two-hole configurations. Comparison with ab initio coupled-cluster predictions, and with experimental data.

doi: 10.1103/PhysRevC.105.014321
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2022YA17      Phys.Rev. C 106, L011305 (2022)

C.J.Yang, W.G.Jiang, S.Burrello, M.Grasso

Calculations for nuclear matter and finite nuclei within and beyond energy-density-functional theories through interactions guided by effective field theory

NUCLEAR STRUCTURE 4He, 16O, 40Ca, 56Ni, 100Sn; calculated ground-state energies as function of angular frequency using t0-t3 model and full SLy5 and SkP energy density functionals, and up to next-to-leading order (NLO), equation of state (EoS) by constructing an effective interaction under energy-density-functional (EDF) theories. Comparison with experimental values.

doi: 10.1103/PhysRevC.106.L011305
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2021BU07      Phys.Rev. C 103, 064317 (2021)

S.Burrello, J.Bonnard, M.Grasso

Application of an ab-initio-inspired energy density functional to nuclei: Impact of the effective mass and the slope of the symmetry energy on bulk and surface properties

NUCLEAR STRUCTURE 12,14,16,18,20,22,24O, 34,36,38,40,42,44,46,48,50,52,54,56,58,60,62Ca, 78,80,82,84,86,88,90,92,94,96,98,100,102,104,106,108,110,112,114,116,118,120,122,124Zr, 100,102,104,106,108,110,112,114,116,118,120,122,124,126,128,130,132,134,136,138,140,142,144,146,148,150,152,154,156,158,160,162,164,166,168,170,172,174,176,178Sn, 178,180,182,184,186,188,190,192,194,196,198,200,202,204,206,208,210,212,214,216,218,220,222,224,226,228,230,232,234,236,238,240,242,244,246,248,250,252,254,256,258,260,262,264,266Pb; calculated S(2n) for O, Ca, Zr and Sn isotopic chains, binding energies for Ca and Zr chains, difference between neutron and proton radii for O, Ca, Zr and Pb chains, charge radii and neutron skins for 16O, 40,48Ca, 90Zr, 132Sn, 208Pb, neutron and proton density profiles for 122Zr and 266Pb, single-proton energies for 208Pb for the last occupied proton. Mean-field Hartree-Fock calculations with Yang-Grasso-Lacroix-Orsay (YGLO) density functionals. Comparison with experimental data extracted from databases at NNDC-BNL. Discussed effective masses and the slope of the symmetry energy.

doi: 10.1103/PhysRevC.103.064317
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2020BO09      Phys.Rev. C 101, 064319 (2020)

J.Bonnard, M.Grasso, D.Lacroix

Lee-Yang-inspired energy-density functional including contributions from p-wave scattering

doi: 10.1103/PhysRevC.101.064319
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2020GA33      Phys.Rev.Lett. 125, 212501 (2020)

D.Gambacurta, M.Grasso, J.Engel

Gamow-Teller Strength in 48Ca and 78Ni with the Charge-Exchange Subtracted Second Random-Phase Approximation

NUCLEAR STRUCTURE 48Ca, 78Ni; analyzed available data; calculated Gamow-Teller strength distributions using a fully self-consistent subtracted second random-phase approximation for charge-exchange processes with Skyrme energy-density functionals.

doi: 10.1103/PhysRevLett.125.212501
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2020GR07      Phys.Rev. C 101, 064314 (2020)

M.Grasso, D.Gambacurta

Beyond-mean-field effects on the symmetry energy and its slope from the low-lying dipole response of 68Ni

NUCLEAR STRUCTURE 68Ni; calculated low-energy B(E1) distributions, neutron and proton transition densities, isoscalar and isovector E1 transition densities, percentage of the EWSR, mean-field EOSs of pure neutron matter, neutron skin thickness, electric dipole polarizability, using the beyond-mean-field (BMF) subtracted second random-phase approximation (SSRPA) model based on Skyrme interaction. Comparison with experimental data. Qualitative estimate of beyond-mean-field effects on symmetry energy of infinite matter and its slope.

doi: 10.1103/PhysRevC.101.064314
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2019GA22      Phys.Rev. C 100, 014317 (2019)

D.Gambacurta, M.Grasso, O.Sorlin

Soft breathing modes in neutron-rich nuclei with the subtracted second random-phase approximation

NUCLEAR STRUCTURE 34Si, 36S, 40,48,60Ca, 68Ni; calculated isoscalar monopole excitations, strength distribution, neutron and proton transition densities, contributions from one-particle one-hole and two-particle two-hole configurations energy weighted sum rules (EWSR) using beyond mean-filed subtracted second random-phase approximation (SSRPA) based on Skyrme interaction SGII.

doi: 10.1103/PhysRevC.100.014317
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2018BO18      Phys.Rev. C 98, 034319 (2018), Erratum Phys. Rev. C 103, 039901 (2021)

J.Bonnard, M.Grasso, D.Lacroix

Energy-density functionals inspired by effective-field theories: Applications to neutron drops

NUCLEAR STRUCTURE N=2-50; calculated energies of neutron drops, internal energies of neutron drops, maximal density at the Thomas-Fermi approximation, density profiles, Hartree-Fock potentials, mean pairing gaps of neutron drops, and effective mass of neutron drops using YGLO, KIDS, and ELYO energy density functionals. Comparison with other energy density functional model predictions and ab initio results.

doi: 10.1103/PhysRevC.98.034319
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2018GA02      Phys.Lett. B 777, 163 (2018)

D.Gambacurta, M.Grasso, O.Vasseur

Electric dipole strength and dipole polarizability in 48Ca within a fully self-consistent second random-phase approximation

NUCLEAR STRUCTURE 48Ca; calculated B(E1), electric dipole polarizability using Skyrme SSRPA model in a fully self-consistent scheme.

doi: 10.1016/j.physletb.2017.12.026
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2018GR11      Phys.Rev. C 98, 051303 (2018)

M.Grasso, D.Gambacurta, O.Vasseur

Beyond-mean-field effective masses in the nuclear Fermi liquid from axial breathing modes

NUCLEAR STRUCTURE 48Ca, 90Zr, 120Sn; calculated isoscalar giant quadrupole resonances (GQR), theoretical uncertainty in the mean-field effective mass from various Skyrme parametrizations, beyond-mean-field (BMF) effective masses, random-phase approximation (RPA) and subtracted second RPA (SSRPA) diagonal matrix elements for the first three single-particle configurations using SSRPA model.

doi: 10.1103/PhysRevC.98.051303
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2018VA17      Phys.Rev. C 98, 044313 (2018)

O.Vasseur, D.Gambacurta, M.Grasso

Systematic study of giant quadrupole resonances with the subtracted second random-phase approximation: Beyond-mean-field centroids and fragmentation

NUCLEAR STRUCTURE 30,34Si, 36S, 40,48Ca, 56Ni, 90Zr, 114,116,120,132Sn, 208Pb; calculated centroids and widths of isoscalar giant quadrupole resonances (GQR) using the subtracted second random-phase-approximation (SSRPA) model in the framework of the energy-density-functional theory. Comparison with RPA calculations and experimental values.

doi: 10.1103/PhysRevC.98.044313
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2017GR08      Phys.Rev. C 95, 054327 (2017)

M.Grasso, D.Lacroix, C.J.Yang

Lee-Yang-inspired functional with a density-dependent neutron-neutron scattering length

doi: 10.1103/PhysRevC.95.054327
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2017LA07      Phys.Rev. C 95, 054306 (2017)

D.Lacroix, A.Boulet, M.Grasso, C.-J.Yang

From bare interactions, low-energy constants, and unitary gas to nuclear density functionals without free parameters: Application to neutron matter

doi: 10.1103/PhysRevC.95.054306
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2017YA15      Phys.Rev. C 95, 054325 (2017)

C.J.Yang, M.Grasso, K.Moghrabi, U.van Kolck

Renormalizability of the nuclear many-body problem with the Skyrme interaction beyond mean field

doi: 10.1103/PhysRevC.95.054325
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2017YA21      Phys.Rev. C 96, 034318 (2017)

C.-J.Yang, M.Grasso, D.Lacroix

Toward a systematic strategy for defining power counting in the construction of the energy density functional

doi: 10.1103/PhysRevC.96.034318
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2016AN12      Eur.Phys.J. A 52, 183 (2016)

M.Anguiano, A.M.Lallena, G.Co, V.De Donno, M.Grasso, R.N.Bernard

Gogny interactions with tensor terms

NUCLEAR STRUCTURE 12C, 16O, 40Ca, 48Ca, 208Pb; calculated first 0- using DRPA with D1S, D1ST, D1M, D1MT interactions. 48,52Ca; calculated B(M1) strength energy distribution, energy gaps between neutron 1f7/2 and 2p3/2 states. 34Si, 36S, 40Ca; calculated energy differences between neutron 2p1/2 and 2p3/2 states. 134Te, 136Xe, 138Ba, 140Ce, 142Nd, 144Sm, 146Gd, 148Dy, 150Er, 152Yb; calculated proton sp state energy 2d5/2 and 1g7/2. DRPA (Discrete set of sp wavefunction RPA) with D1S, D1ST, D1M, D1MT, D1MT2a, D1MT2c interactions. Calculations compared with data.

NUCLEAR REACTIONS 48Ca, 90Zr, 208Pb(p, n), E not given; calculated energy distributions of GT strengths. DRPA (Discrete set of sp wavefunction RPA) with D1MT, D1MT2a, D1MT2c forces. Calculations compared to data.

doi: 10.1140/epja/i2016-16183-1
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2016GA04      Phys.Rev. C 93, 024309 (2016)

D.Gambacurta, F.Catara, M.Grasso, M.Sambataro, M.V.Andres, E.G.Lanza

Nuclear excitations as coupled one and two random-phase-approximation modes

NUCLEAR STRUCTURE 16O; calculated low-lying levels and giant resonances (dipole, quadrupole and octupole), J, π, monopole (E0), dipole (E1), isoscalar quadrupole (E2), and isoscalar octupole (E3) response functions. Double random-phase approximation (DRPA) method to include two -particle two-hole (2p-2h) configurations and by coupling them with the 1p-1h ones and among themselves. Comparison with experimental values.

doi: 10.1103/PhysRevC.93.024309
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2016GA28      Eur.Phys.J. A 52, 198 (2016)

D.Gambacurta, M.Grasso

Second RPA calculations with the Skyrme and Gogny interactions

NUCLEAR STRUCTURE 16O; calculated giant resonance strength distributions using RPA, Skyrme-SRPA, Gogny-SRPA (SRPA = Skyrme RPA).

doi: 10.1140/epja/i2016-16198-6
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2016GR16      Phys.Scr. 91, 063005 (2016)

M.Grasso, D.Lacroix, U.van Kolck

From effective field theories to effective density functionals in and beyond the mean field

doi: 10.1088/0031-8949/91/6/063005
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2016YA11      Phys.Rev. C 94, 031301 (2016)

C.J.Yang, M.Grasso, D.Lacroix

From dilute matter to the equilibrium point in the energy-density-functional theory

NUCLEAR STRUCTURE 68Ni, 120Sn, 208Pb; calculated symmetry energy as a function of its slope and density using two parametrizations; proposed new energy-density functional. Comparison with experimental electric dipole polarizability.

doi: 10.1103/PhysRevC.94.031301
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2016YA12      Phys.Rev. C 94, 034311 (2016)

C.J.Yang, M.Grasso, X.Roca-Maza, G.Colo, K.Moghrabi

Second-order equation of state with the Skyrme interaction: Cutoff and dimensional regularization with the inclusion of rearrangement terms

doi: 10.1103/PhysRevC.94.034311
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2015GA28      Phys.Rev. C 92, 034303 (2015)

D.Gambacurta, M.Grasso, J.Engel

Subtraction method in the second random-phase approximation: First applications with a Skyrme energy functional

NUCLEAR STRUCTURE 16O; calculated energies, isoscalar monopole B(E0) and quadrupole B(E2) response for 10-30 MeV excitation, ratios of moments, EWSR, effects of two particle-two hole configurations (2p2h) on the excitation spectra of medium-mass and heavy nuclei. Subtraction procedure in the second random-phase-approximation (SRPA) with Skyrme energy density-functional theory. Comparison with experimental data.

doi: 10.1103/PhysRevC.92.034303
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2015GR15      Phys.Rev. C 92, 054316 (2015)

M.Grasso, M.Anguiano

Neutron 2p and 1f spin-orbit splittings in 40Ca, 36S and 34Si N = 20 isotones: Tensor-induced and pure spin-orbit effects

NUCLEAR STRUCTURE 34Si, 36S, 40Ca; calculated energies of 2p3/2, 2p1/2 and 1f5/2 neutron states relative to the energy of 1f7/2 neutron state, neutron 2p and 1f spin-orbit splittings using mean-field approaches based on Skyrme and Gogny forces and three types of interactions.

doi: 10.1103/PhysRevC.92.054316
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2014CO20      Phys.Scr. 89, 054006 (2014)

G.Colo, P.F.Bortignon, M.Brenna, X.Roca-Maza, E.Vigezzi, K.Moghrabi, M.Grasso, K.Mizuyama

Progress in nuclear structure beyond the mean-field approximation

NUCLEAR STRUCTURE 39,41Ca; calculated level density, spectroscopic factor, strength functions using nuclear density functional theory with particle-vibration coupling and other extensions. Compared with available data.

doi: 10.1088/0031-8949/89/5/054006
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2014GR02      Phys.Rev. C 89, 034316 (2014)

M.Grasso

Magicity of the 58Ca and 54Ca isotopes and tensor contribution within a mean-field approach

NUCLEAR STRUCTURE 40,48,52,54Ca, 54,56Ti, 56,58Cr, 58,60Fe; calculated neutron and proton single-particle energies, neutron gaps, S(2n). 52, 54Ca; investigated magicity of 52Ca and 54Ca. Mean-field approach with Skyrme interaction and Hartree-Fock calculations. Comparison with experimental data.

doi: 10.1103/PhysRevC.89.034316
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2013GR07      Phys.Rev. C 87, 064308 (2013)

M.Grasso

Two-neutron transfer probabilities and spatial-localization effects at the drip line

NUCLEAR STRUCTURE 74,76,78,80,82Cr; calculated two-nucleon transfer probabilities. HFB calculations with the Skyrme parameterization SkM* in the mean-field approach, and generating neutron pairing interactions for stable open-shell A=40-48 Ca isotopes. Persistence or suppression of pairing at drip lines.

doi: 10.1103/PhysRevC.87.064308
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2013GR16      Phys.Rev. C 88, 054328 (2013)

M.Grasso, M.Anguiano

Tensor parameters in Skyrme and Gogny effective interactions: Trends from a ground-state-focused study

NUCLEAR STRUCTURE 40,48Ca, 56Ni; calculated neutron f spin-orbit splittings and tensor parameters. 16O, 40,48Ca, 56Ni, 90Zr, 132Sn; calculated binding energies. Skyrme and Gogny effective interactions including a tensor force. Comparison with experimental data.

doi: 10.1103/PhysRevC.88.054328
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2012AN14      Phys.Rev. C 86, 054302 (2012)

M.Anguiano, M.Grasso, G.Co, V.De Donno, A.M.Lallena

Tensor and tensor-isospin terms in the effective Gogny interaction

NUCLEAR STRUCTURE 16,22O, 40,48Ca, 132,140Sn; calculated neutron energy gap, single particle energies using effective Gogny interaction in mean-field calculations with the inclusion of tensor-isospin terms.

doi: 10.1103/PhysRevC.86.054302
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2012CO04      Phys.Rev. C 85, 024322 (2012)

G.Co, V.De Donno, P.Finelli, M.Grasso, M.Anguiano, A.M.Lallena, C.Giusti, A.Meucci, F.D.Pacati

Mean-field calculations of the ground states of exotic nuclei

NUCLEAR STRUCTURE 16,22,24,28O, 40,48,52,60Ca, 48,56,68,78Ni, 100,114,116,132Sn; calculated binding energies, single particle energies, rms charge radii, neutron skin thickness. Mean-field approach, nonrelativistic Hartree-Fock, relativistic Hartree calculations. Comparison with experimental data.

NUCLEAR REACTIONS 40,48,52,60Ca(e, e'p), (e, e), E=483.2 MeV; calculated reduced cross sections, elastic scattering cross sections, neutron, proton and matter distributions, Mean-field approach, nonrelativistic Hartree-Fock, relativistic Hartree calculations. Comparison with experimental data.

doi: 10.1103/PhysRevC.85.024322
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2012GA31      Phys.Rev. C 86, 021304 (2012)

D.Gambacurta, M.Grasso, V.De Donno, G.Co, F.Catara

Second random-phase approximation with the Gogny force: First applications

NUCLEAR STRUCTURE 16O; calculated isoscalar monopole discrete strength distribution B(E0), isoscalar monopole response, proton and neutron transition densities. Random-phase approximation (RPA), second RPA (SRPA) with finite-range Gogny interaction. Discussed effects of particle-hole couplings in Gogny-SRPA calculations.

doi: 10.1103/PhysRevC.86.021304
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2012GR07      Phys.Rev. C 85, 034317 (2012)

M.Grasso, D.Lacroix, A.Vitturi

Pair-transfer probability in open- and closed-shell Sn isotopes

NUCLEAR STRUCTURE 100,102,104,106,108,110,112,114,116,118,120,122,124,126,128,130,132,134,136,138,140,142,144Sn; calculated two nucleon transfer (removal or addition) strength from ground-state to ground-state, neutron Fermi energy, entropy, pairing gap for mixed pairing case and pure surface case. Canonical basis formulation, and Hartree-Fock-Bogoliubov (HFB) theory. Discussed role of particle number restoration.

doi: 10.1103/PhysRevC.85.034317
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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
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2012MO12      Phys.Rev. C 85, 044323 (2012); Erratum Phys.Rev. C 94, 069901 (2016)

K.Moghrabi, M.Grasso, X.Roca-Maza, G.Colo

Second-order equation of state with the full Skyrme interaction: Toward new effective interactions for beyond-mean-field models

doi: 10.1103/PhysRevC.85.044323
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2012MO27      Phys.Rev. C 86, 044319 (2012)

K.Moghrabi, M.Grasso

Dimensional regularization applied to nuclear matter with a zero-range interaction

doi: 10.1103/PhysRevC.86.044319
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2011GA02      J.Phys.(London) G38, 035103 (2011)

D.Gambacurta, M.Grasso, F.Catara

Residual interaction in second random-phase approximation with density-dependent forces: rearrangement terms

doi: 10.1088/0954-3899/38/3/035103
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2011GA39      Phys.Rev. C 84, 034301 (2011)

D.Gambacurta, M.Grasso, F.Catara

Low-lying dipole response in the stable 40, 48Ca nuclei with the second random-phase approximation

NUCLEAR STRUCTURE 40,48Ca; calculated isoscalar and isovector B(E1) strength distributions in 5-10 MeV excitation region, EWSR, neutron and proton transition densities. Random-phase approximation (RPA) and second random-phase approximation (SRPA) with Skyrme interaction SGII with inclusion of 2p2h configurations. Pygmy resonances. Comparison with experimental data.

doi: 10.1103/PhysRevC.84.034301
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2011PE26      Phys.Rev. C 84, 045806 (2011)

D.Pena Arteaga, M.Grasso, E.Khan, P.Ring

Nuclear structure in strong magnetic fields: Nuclei in the crust of a magnetar

NUCLEAR STRUCTURE 16O, 56Fe; calculated evolution of single-particle level energies, binding energy per article, radius, and β deformation as a function of magnetic field strengths. Z=22-30, N=22-36; calculated minimum magnetic field for which the first level crossing at the Fermi energy occurs. Influence of strong magnetic fields on nuclear structure using a fully self-consistent covariant density functional.

doi: 10.1103/PhysRevC.84.045806
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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
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2010GA07      Phys.Rev. C 81, 054312 (2010)

D.Gambacurta, M.Grasso, F.Catara

Collective nuclear excitations with Skyrme-second random-phase approximation

NUCLEAR STRUCTURE 16O; calculated isoscalar and isovector strength distributions for monopole 0+, dipole 1- and quadrupole 2+ states, B(E0), B(E1), B(E2), transition densities using second random phase approximation using second random-phase approximation (SRPA) calculations with a Skyrme force. Comparison between RPA and SRPA calculations.

doi: 10.1103/PhysRevC.81.054312
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2010MO12      Phys.Rev. C 81, 064327 (2010)

M.Moreno Torres, M.Grasso, H.Liang, V.De Donno, M.Anguiano, N.Van Giai

Tensor effects in shell evolution at Z, N=8, 20, and 28 using nonrelativistic and relativistic mean-field theory

NUCLEAR STRUCTURE 14C, 16,22O, 40,48,52,54Ca, 34,42Si, 36,44S, 56,60,66,68,78Ni; analyzed effects of the tensor force on the neutron and proton gaps. Hartree-Fock calculations with Skyrme and Gogny interactions. Non-relativistic and relativistic mean-field approaches. Comparison with experimental data.

doi: 10.1103/PhysRevC.81.064327
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2010MO28      Phys.Rev.Lett. 105, 262501 (2010)

K.Moghrabi, M.Grasso, G.Colo, N.Van Giai

Beyond Mean-Field Theories with Zero-Range Effective Interactions: A Way to Handle the Ultraviolet Divergence

doi: 10.1103/PhysRevLett.105.262501
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2009GA22      Phys.Rev. C 80, 014303 (2009)

D.Gambacurta, F.Catara, M.Grasso

Self-consistent extension of random-phase approximation enlarged beyond particle-hole configurations

doi: 10.1103/PhysRevC.80.014303
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2009GR04      Phys.Rev. C 79, 034318 (2009)

M.Grasso, L.Gaudefroy, E.Khan, T.Niksic, J.Piekarewicz, O.Sorlin, N.Van Giai, D.Vretenar

Nuclear "bubble" structure in 34Si

NUCLEAR STRUCTURE 22,24O, 34,36Si; calculated neutron densities, charge densities, binding energies, charge radii, neutron skin thickness. Shell model, non-relativistic mean-field approach and relativistic mean-field approach calculations.

doi: 10.1103/PhysRevC.79.034318
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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
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2009KH08      Phys.Rev. C 80, 044328 (2009)

E.Khan, M.Grasso, J.Margueron

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
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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
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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
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2007GR20      Nucl.Phys. A788, 337c (2007)

M.Grasso, S.Yoshida, N.Sandulescu, N.Van Giai

Giant halo and anti-halo in the non-relativistic mean field approach

NUCLEAR STRUCTURE Zr; calculated radii, two-neutron separation energies, halo features. Non-relativistic mean field approach.

doi: 10.1016/j.nuclphysa.2007.01.063
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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
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2006BE04      Phys.Rev.Lett. 96, 012501 (2006)

E.Becheva, Y.Blumenfeld, E.Khan, D.Beaumel, J.M.Daugas, F.Delaunay, Ch.-E.Demonchy, A.Drouart, M.Fallot, A.Gillibert, L.Giot, M.Grasso, N.Keeley, K.W.Kemper, D.T.Khoa, V.Lapoux, V.Lima, A.Musumarra, L.Nalpas, E.C.Pollacco, O.Roig, P.Roussel-Chomaz, J.E.Sauvestre, J.A.Scarpaci, F.Skaza, H.S.Than

N = 14 Shell Closure in 22O Viewed through a Neutron Sensitive Probe

NUCLEAR REACTIONS 1H(22O, 22O), (22O, 22O'), E=46.6 MeV/nucleon; measured particle spectra, σ(E, θ). 22O level deduced deformation parameter, shell closure features. MUST detector array.

doi: 10.1103/PhysRevLett.96.012501
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetF0738. Data from this article have been entered in the XUNDL database. For more information, click here.


2006GA09      Phys.Rev. C 73, 024319 (2006)

D.Gambacurta, M.Grasso, F.Catara, M.Sambataro

Extension of the second random-phase approximation

doi: 10.1103/PhysRevC.73.024319
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2006GR27      Phys.Rev.C 74, 064317 (2006)

M.Grasso, S.Yoshida, N.Sandulescu, N.Van Giai

Giant neutron halos in the non-relativistic mean field approach

NUCLEAR STRUCTURE 56,58,60,62,64,66,68,70,72Ca, 116,118,120,122,124,126,128,130,132,134,136,138,140Zr; calculated radii, two-neutron separation energies, halo features. Non-relativistic mean field approach.

doi: 10.1103/PhysRevC.74.064317
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2004KH02      Phys.Rev. C 69, 014314 (2004)

E.Khan, N.Sandulescu, N.Van Giai, M.Grasso

Two-neutron transfer in nuclei close to the drip line

NUCLEAR REACTIONS 22O(t, p), E=15 MeV/nucleon; calculated form factors, σ(E, θ). Continuum quasiparticle RPA.

NUCLEAR STRUCTURE 18,20,22O; calculated single-particle energies, response functions for two-neutron transfer. Continuum quasiparticle RPA.

doi: 10.1103/PhysRevC.69.014314
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2004KH03      Nucl.Phys. A731, 311 (2004)

E.Khan, N.Van Giai, M.Grasso

Collective Motions in Hot Exotic Nuclei: the Finite Temperature Continuum-QRPA

NUCLEAR STRUCTURE 22O, 120,136Sn; calculated dipole and quadrupole response functions. Finite temperature continuum-quasiparticle RPA.

doi: 10.1016/j.nuclphysa.2003.11.042
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2004KH06      Phys.Rev. C 69, 044605 (2004)

D.T.Khoa, H.S.Than, T.H.Nam, M.Grasso, N.Van Giai

Microscopic calculation of the interaction cross section for stable and unstable nuclei based on the nonrelativistic nucleon-nucleon t matrix

NUCLEAR REACTIONS 12C(α, X), (6He, X), (8He, X), (6Li, X), (7Li, X), (8Li, X), (9Li, X), (11Li, X), (12C, X), (13C, X), (14C, X), (15C, X), (16C, X), (17C, X), (18C, X), (19C, X), (20C, X), (16O, X), (17O, X), (18O, X), (19O, X), (20O, X), (21O, X), (22O, X), (23O, X), (24O, X), E ≈ 740-1050 MeV/nucleon; calculated reaction and interaction σ. DWIA, microscopic complex optical potential, folding model.

doi: 10.1103/PhysRevC.69.044605
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2003KH10      Nucl.Phys. A722, 92c (2003)

D.T.Khoa, H.S.Than, M.Grasso

Microscopic study of interaction cross sections measured at relativistic energies for stable and unstable nuclei

NUCLEAR REACTIONS 12C(α, X), (6He, X), (8He, X), (6Li, X), (7Li, X), (8Li, X), (9Li, X), (11Li, X), (12C, X), (14C, X), (16C, X), (18C, X), (19C, X), (20C, X), (16O, X), (18O, X), (20O, X), (22O, X), (24O, X), E ≈ 790-1050 MeV/nucleon; calculated reaction, interaction σ. Parameter-free folding approach, comparisons with data.

doi: 10.1016/S0375-9474(03)01342-3
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2002GR14      Phys.Lett. 535B, 103 (2002)

M.Grasso, N.Van Giai, N.Sandulescu

Continuum HFB Calculations with Finite Range Pairing Interactions

NUCLEAR STRUCTURE 18C; calculated total energy, pairing interaction features. Hartree-Fock-Bogoliubov approach, Skyrme and Gogny forces.

doi: 10.1016/S0370-2693(02)01719-7
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2002GR30      Phys.Rev. C 66, 064303 (2002)

M.Grasso, F.Catara, M.Sambataro

Boson-mapping-based extension of the random-phase approximation in a three-level Lipkin model

doi: 10.1103/PhysRevC.66.064303
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2002GR35      Prog.Theor.Phys.(Kyoto), Suppl. 146, 619 (2002)

M.Grasso, E.Khan, N.Van Giai, N.Sandulescu

Pairing Correlations in Nuclei Close to the Drip Line

NUCLEAR STRUCTURE 74,76,78,80,82,84,86,88Ni; calculated pairing correlation energies. 24O calculated quadrupole strength distribution.

doi: 10.1143/PTPS.146.619
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2002KH10      Phys.Rev. C66, 024309 (2002)

E.Khan, N.Sandulescu, M.Grasso, N.V.Giai

Continuum quasiparticle random phase approximation and the time-dependent Hartree-Fock-Bogoliubov approach

NUCLEAR STRUCTURE 18,20,22,24O; calculated neutron pairing gaps, transitions B(E2), quadrupole strength functions. Continuum quasiparticle RPA, linear response method.

doi: 10.1103/PhysRevC.66.024309
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2001GR03      Phys.Rev. C63, 014317 (2001)

M.Grasso, F.Catara

Extension of Random-Phase Approximation Preserving Energy Weighted Sum Rules: An application to a 3-level Lipkin model

doi: 10.1103/PhysRevC.63.014317
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2001GR32      Phys.Rev. C64, 064321 (2001)

M.Grasso, N.Sandulescu, V.G.Nguyen, R.J.Liotta

Pairing and Continuum Effects in Nuclei Close to the Drip Line

NUCLEAR STRUCTURE 84Ni; calculated single-particle energies, widths, neutron pairing densities. 74,76,78,80,82,84,86,88Ni; calculated pairing correlation energies, two-neutron separation energies, neutron radii. Hartree-Fock-Bogoliubov calculations, different boundary conditions compared.

doi: 10.1103/PhysRevC.64.064321
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