23–26 nov. 2021
GANIL, Caen
Fuseau horaire Europe/Paris

Session

Isospin Effects and EoS in nuclear reactions

3
24 nov. 2021, 10:00
Maison d'hôtes (GANIL, Caen)

Maison d'hôtes

GANIL, Caen

Bd Henri Becquerel, 14000 Caen

Description

Isospin Effects and EoS in nuclear reactions

Documents de présentation

Aucun document.

  1. Dr CAMAIANI, Alberto (IKS - KU Leuven, Belgium)
    24/11/2021 10:00
    Understanding isospin transport ratio: influence of fast emissions and statistical de-excitation
    Regular talk (YP)

    Isospin transport ratio is a powerful method to estimate the neutron-proton (n-p) equilibration in heavy-ion collisions, and extensively used to obtain information on the asy-stiffness of the nuclear Equation of State. In fact such a ratio is expected to bypass any perturbations introducing a linear
    transformation of the chosen observable. In particular, it is supposed to overcome...

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  2. Dr GNOFFO, Brunilde (Univ. Catania and INFN Sez. Catania, Italy)
    24/11/2021 10:25
    Isospin influence on the thermal characteristics in the reactions 78,86Kr+ 40,48Ca at 10 AMeV
    Regular talk (YP)

    B. Gnoffo1,2, S. Pirrone2, G. Politi1,2, L. Acosta2,3, G. Cardella2, E. De Filippo2, E. Geraci1,2, L. Lo Monaco1, C. Maiolino4, N.S. Martorana1,4, A. Pagano2, E.V. Pagano4, M. Papa2, F. Risitano2,5, F. Rizzo1,4, P. Russotto4 and M. Trimarchi2,5

    1) Dipartimento di Fisica e Astronomia E. Majorana, Università di Catania, Italy
    2) INFN-Sezione di Catania, Italy
    3) Instituto de Fisica,...

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  3. Dr FABLE, Quentin (L2it, CNRS/IN2P3, France)
    24/11/2021 11:30
    Experimental study of the symmetry energy from 40,48 Ca+ 40,48 Ca reactions at 35 AMeV
    Regular talk (YP)

    We investigated the possibility to probe the symmetry energy term of the nuclear equation of state with isoscaling observables from 40,48 Ca+ 40,48 Ca reactions at 35 AMeV . Data were obtained using the unique coupling of the VAMOS high acceptance spectrometer and the 4π INDRA detector. This required a precise study of the trajectory reconstruction in the spectrometer focal plane along with...

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  4. M. QUICRAY, Joël (LPC Caen, France)
    24/11/2021 11:55
    Probing nuclear isospin equilibration : the INDRA-FAZIA experiment in GANIL
    Regular talk (YP)

    J. Quicray
    On behalf of the INDRA and FAZIA collaborations

    Normandie Univ, ENSICAEN, UNICAEN, CNRS/IN2P3, LPC Caen, 14000 Caen, France

    The study of fragmentation reactions produced in heavy-ion collisions has permitted major advances in the understanding of the dynamics and thermodynamics of nuclear matter [1, 2] and is still one of the most promising tools to constrain its equation of...

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  5. M. LEE, Jung Woo (Korea University, South Korea)
    24/11/2021 12:20
    Isoscaling effect with $Z$=1 and 2 particles in Sn+Sn at 270 AMeV
    Regular talk (YP)

    Isoscaling effect with $Z$=1 and 2 particles in Sn+Sn at 270 AMeV

    J. W. Lee for S$\pi$RIT collaboration
    Korea University, Seoul, Korea

    The mechanism of the fragmentation in heavy ion collision is studied with particle yields of light nuclei. In the thermal equilibrium view, the primary fragment yield can be predicted using the partition function of each fragment. However, the fragments...

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  6. Dr LI, Bao An (Texas A&M Commerce, USA)
    24/11/2021 14:15
    Theoretical aspects: Isospin effects and EOS in nuclear reactions
    Regular talk (remote)

    The isospin dependence of in-medium nuclear effective interactions is a fundamental issue in nuclear physics and has broad ramifications in astrophysics. Its uncertainties, especially the difference of neutron-proton interactions in the isosinglet and isotriplet channels, affect significantly the density and momentum dependence of the isovector single-nucleon potential and nucleon-nucleon...

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  7. Dr RUSSOTTO, Paolo (INFN-LNS Catania, Italy)
    24/11/2021 15:00
    Status of data analysis and preliminary results of the CHIFAR experiment
    Regular talk (remote)

    The CHIFAR experiment [1] was carried out at LNS in November 2019. Reactions between beams of 124Sn,124Xe and 112Sn, accelerated at 20 AMeV by the CS, and targets of 64Ni, 64Zn and 58Ni were studied by using the CHIMERA multi-detector [2] coupled to 10 telescopes of the FARCOS array [3]. The ten FARCOS telescopes, grouped in 5 couples, were arranged in a ring-like configuration covering about...

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  8. Dr LYNCH, William (NSCL/FRIB Dept. of Physics and Astronomy Michigan State Univ., USA)
    24/11/2021 15:25
    Constraints on the symmetry energy supra-saturation density from Pion Spectral Ratios
    Regular talk (remote)

    Pion spectral ratios and double ratios are measured for neutron rich 132Sn+124Sn and neutron deficient 108Sn+112Sn collisions. Both pi-/Pi+ single spectral ratios for the two systems and double ratios obtained by combining both systems can be described by a dcQMD calculations. These comparisons provide a correlated constraint on L and on the neutron-proton effect mass difference. This...

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