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NSR database version of April 26, 2024.

Search: Author = C.Ciampi

Found 9 matches.

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2024HU01      Phys.Rev. C 109, L011601 (2024)

S.Hudan, H.Desilets, R.Kumar, R.T.deSouza, C.Ciampi, A.Chbihi, K.W.Brown

Influence of additional neutrons on the fusion cross section beyond the N=8 shell

doi: 10.1103/PhysRevC.109.L011601
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2024RE04      J.Phys.(London) G51, 015104 (2024)

A.Rebillard-Soulie, R.Bougault, H.Pais, B.Borderie, A.Chbihi, C.Ciampi, Q.Fable, J.Frankland, E.Galichet, T.Genard, D.Gruyer, N.Le Neindre, I.Lombardo, O.Lopez, L.Manduci, M.Parlog, G.Verde

Isoscaling in dilute warm nuclear systems

NUCLEAR REACTIONS ¹²⁴Sn(¹²⁴Xe, X), ¹¹²Sn(¹³⁶Xe, X)²H/³H/³He/⁴He/⁶He, E=32 MeV/nucleon; measured reaction products; deduced expanding gas source temperature, total mass, total proton fraction and baryon density, mass fractions of detected charged particles, isoscaling ratio. The 4π multidetector INDRA.

doi: 10.1088/1361-6471/ad0edd
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2023CI03      Phys.Rev. C 108, 054611 (2023)

C.Ciampi, S.Piantelli, G.Casini, A.Ono, J.D.Frankland, L.Baldesi, S.Barlini, B.Borderie, R.Bougault, A.Camaiani, A.Chbihi, J.A.Duenas, Q.Fable, D.Fabris, C.Frosin, T.Genard, F.Gramegna, D.Gruyer, M.Henri, B.Hong, S.Kim, A.Kordyasz, T.Kozik, M.J.Kweon, N.Le Neindre, I.Lombardo, O.Lopez, T.Marchi, K.Mazurek, S.H.Nam, J.Park, M.Parlog, G.Pasquali, G.Poggi, A.Rebillard-Soulie, A.A.Stefanini, S.Upadhyaya, S.Valdre, G.Verde, E.Vient, M.Vigilante, for the INDRA-FAZIA Collaboration

Quasiprojectile breakup and isospin equilibration at Fermi energies: Potential indication of longer projectile-target contact times

doi: 10.1103/PhysRevC.108.054611
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2022CI05      Phys.Rev. C 106, 024603 (2022)

C.Ciampi, for the INDRA-FAZIA Collaboration

First results from the INDRA-FAZIA apparatus on isospin diffusion in ^{58, 64}Ni + ^{58, 64}Ni systems at Fermi energies

NUCLEAR REACTIONS ⁵⁸Ni(⁶⁴Ni, X), ⁶⁴Ni(⁵⁸Ni, X), E=32, 52 MeV/nucleon; measured reaction products; deduced charge and velocity distribution of the fragments, reduced impact parameter, neutron to proton ratio for the quasiprojectile fragments, isospin transport ratio, neutron to proton ratio of the forward emitted particles with respect to the quasiprojectile remnant. Comparison to simulations based on the antisymmetrized molecular dynamics model (AMD) coupled to GEMINI++ code as afterburner. INDRA-FAZIA multidetector array at GANIL.

doi: 10.1103/PhysRevC.106.024603
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2021CA04      Phys.Rev. C 103, 014605 (2021)

A.Camaiani, G.Casini, S.Piantelli, A.Ono, E.Bonnet, R.Alba, S.Barlini, B.Borderie, R.Bougault, C.Ciampi, A.Chbihi, M.Cicerchia, M.Cinausero, J.A.Duenas, D.Dell'Aquila, Q.Fable, D.Fabris, C.Frosin, J.D.Frankland, F.Gramegna, D.Gruyer, K.I.Hahn, M.Henri, B.Hong, S.Kim, A.Kordyasz, M.J.Kweon, H.J.Lee, J.Lemarie, N.LeNeindre, I.Lombardo, O.Lopez, T.Marchi, S.H.Nam, P.Ottanelli, M.Parlog, G.Pasquali, G.Poggi, J.Quicray, A.A.Stefanini, S.Upadhyaya, S.Valdre, E.Vient

Isospin diffusion measurement from the direct detection of a quasiprojectile remnant

NUCLEAR REACTIONS ^40,48Ca(⁴⁰Ca, X), (⁴⁸Ca, X), E=35 MeV/nucleon; measured reaction products, particle spectra, N/Z of quasiprojectiles (QP) using FAZIA multitelescope array at the Superconducting Cyclotron facility of INFN-LNS-Catania; deduced isotopic identification of QP phase space, isospin transport ratio, isospin diffusion as a function of reaction centrality, comparison between QP evaporative and break-up channel. Comparison of the measured equilibration degree with model predictions using antisymmetrized molecular dynamics (AMD) coupled with statistical decay using GEMINI++ code.

doi: 10.1103/PhysRevC.103.014605
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2021LO14      J.Phys.(London) G48, 065101 (2021)

I.Lombardo, D.Dell'Aquila, M.Cinausero, L.R.Gasques, M.Vigilante, V.A.B.Zagatto, S.Barlini, R.Bolzonella, M.Bruno, A.Buccola, A.Camaiani, S.M.Carturan, G.Casini, C.Ciampi, M.Cicerchia, M.D'Andrea, M.Degerlier, D.Fabris, C.Frosin, F.Gramegna, A.Lepine-Szily, G.Maggioni, G.Mantovani, T.Marchi, A.Ordine, P.Ottanelli, G.Pasquali, S.Piantelli, V.Rigato, M.Russo, L.Scomparin, S.Valdre, G.Verde

Study of the ³³Cl spectroscopic factors via the ³²S(³He, d)³³Cl one-proton transfer reaction

NUCLEAR REACTIONS ³²S(³He, d), E=9.68 MeV; measured reaction products; deduced deuteron spectrum, σ(θ), level energies, J, π, spectroscopic factors. Comparison with finite-range DWBA and coupled-channel calculations and available data. The OSCAR (hOdoscope of silicon for correlations and analysis of reaction) device. The CN van de Graaf accelerator of INFN-Laboratori Nazionali di Legnaro, Italy.

doi: 10.1088/1361-6471/abdee4
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2020CA24      Phys.Rev. C 102, 044607 (2020)

A.Camaiani, S.Piantelli, A.Ono, G.Casini, B.Borderie, R.Bougault, C.Ciampi, J.A.Duenas, C.Frosin, J.D.Frankland, D.Gruyer, N.LeNeindre, I.Lombardo, G.Mantovani, P.Ottanelli, M.Parlog, G.Pasquali, S.Upadhyaya, S.Valdre, G.Verde, E.Vient

Influence of fast emissions and statistical de-excitation on the isospin transport ratio

NUCLEAR REACTIONS ^48,40Ca(⁴⁸Ca, X), (⁴⁰Ca, X), E=35 MeV/nucleon; analyzed experimental data from INDRA+VAMOS campaign, and FAZIA experiment; calculated neutron-to-proton ratio of the quasiprojectile (QP) as a function of the QP excitation energy, correlations between the neutron-to-proton ratio, symmetry energy of nuclear equation of state, isospin transport ratio. Estimation of the perturbation introduced by dynamical and statistical emissions on the measurement of neutron-proton equilibration via isospin transport ratio. Antisymmetrized molecular dynamics (AMD), and statistical decay (GEMINI and HIPSE).

doi: 10.1103/PhysRevC.102.044607
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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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2019PI09      Phys.Rev. C 99, 064616 (2019)

S.Piantelli, A.Olmi, P.R.Maurenzig, A.Ono, M.Bini, G.Casini, G.Pasquali, A.Mangiarotti, G.Poggi, A.A.Stefanini, S.Barlini, A.Camaiani, C.Ciampi, C.Frosin, P.Ottanelli, S.Valdre

Comparison between calculations with the AMD code and experimental data for peripheral collisions of ⁹³Nb + ⁹³Nb, ¹¹⁶Sn at 38 Mev/nucleon

NUCLEAR REACTIONS ⁹³Nb, ¹¹⁶Sn(⁹³Nb, X), E=38 MeV/nucleon; measured reaction products in peripheral and semiperipheral collisions using the FIASCO setup at INFN-LNS; deduced diffusion and Wilczynski plots, quasiprojectile charge and particle multiplicities as functions of the centrality. Comparison with theoretical calculations using antisymmetrized molecular dynamics (AMD) model coupled with GEMINI++ and GEMINI f90 used as afterburner.

doi: 10.1103/PhysRevC.99.064616
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