May 25 – 28, 2026
Il Fuligno (Firenze, Italy)
Europe/Rome timezone

Contribution List

39 out of 39 displayed
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  1. Giovanni Passaleva (Istituto Nazionale di Fisica Nucleare)
    5/25/26, 9:30 AM
  2. Sara Pirrone (Istituto Nazionale di Fisica Nucleare)
    5/25/26, 9:45 AM
  3. Emanuele Vincenzo Pagano (Istituto Nazionale di Fisica Nucleare)
    5/25/26, 10:00 AM

    Recent highlights from CHIMERA

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  4. Sandro Barlini (Istituto Nazionale di Fisica Nucleare)
    5/25/26, 10:45 AM

    Recent highlights from INDRA-FAZIA

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  5. Jerzy Lukasik (IFJ PAN, Kraków, Poland)
    5/25/26, 11:55 AM

    The only way to study the properties of asymmetric nuclear matter at high densities in the laboratory conditions is to investigate the relativistic heavy ion collisions. A complementary source of information are the astrophysical observations and gravitational waves. The degree of compression and pressures achieved during the heavy ion collision depend on the susceptibility of the nuclear...

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  6. Emanuele Vincenzo Pagano (Istituto Nazionale di Fisica Nucleare), Cristina Zagami (Istituto Nazionale di Fisica Nucleare)
    5/25/26, 12:40 PM

    The CHIFAR experiment at the INFN-LNS coupled the 4$\pi$ CHIMERA multi-detector with 10 telescopes of the FARCOS (Femtoscope Array for COrrelations and Spectroscopy) correlator. FARCOS is a triple-stage telescope consisting of two DSSSDs (Double Sided Silicon Strip Detectors, 300 and 1500 $\mu$m thick) and 4 CsI(Tl) scintillators (6 cm thick), featuring high energy and angular resolution....

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  7. Fabio Risitano (Istituto Nazionale di Fisica Nucleare)
    5/25/26, 1:05 PM

    The study of the density dependence of the equation of state (EOS) of nuclear matter at supra-saturation densities is a major topic of modern nuclear physics, with important implications in many fields. These span from astrophysics, such as the behavior of neutron stars and core collapse supernovae, to heavy ion collision (HIC) phenomena. Symmetry energy can be investigated not only by means...

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  8. Mariangela Bondi (Istituto Nazionale di Fisica Nucleare)
    5/25/26, 2:45 PM

    Streaming readout (SRO) data acquisition is emerging as a key paradigm for high-luminosity nuclear and particle physics experiments, enabling triggerless operation through continuous, time-stamped data streams processed in software. By organizing detector hits into time slices and performing real-time reconstruction and selection using global detector information, SRO enables efficient data...

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  9. Chiara Guazzoni (Politecnico di Milano, DEIB & Istituto Nazionale di Fisica Nucleare, Sezione di Milano)
    5/25/26, 3:30 PM

    Microstrip detectors are essential, high-resolution position-sensitive sensors used in nuclear physics for tracking, vertex reconstruction, and beam monitoring. In addition to those detectors pad arrays are used when moderate position resolution is required combined with unambiguity in particle detection, for example in beam monitoring. Different ancillary detectors are based on microstrips...

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  10. Nunzia Simona Martorana (Istituto Nazionale di Fisica Nucleare)
    5/25/26, 3:55 PM

    N.S. Martorana$^{1}$, G. Cardella$^{1}$, E. De Filippo$^{1}$, E. Geraci$^{1,2,3}$, C. Guazzoni$^{4}$, P. Russotto$^{5}$, L. Acosta$^{6}$, A. Barbon$^{1,2}$, A. Castoldi$^{4}$, G. Colucci$^{7}$, G. D’Agata$^{1,2}$, B. Gnoffo$^{1,2}$, J. F. González Linares$^{6}$, T. Kurtukian-Nieto$^{6}$, F. La Via$^{8}$, C. Maiolino$^{5}$, E.V. Pagano$^{5}$, S. Pirrone$^{1}$, G. Politi$^{1,2}$, M Pozzi$^{4}$,...

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  11. Emanuele Vincenzo Pagano (Istituto Nazionale di Fisica Nucleare)
    5/25/26, 4:45 PM
  12. Enrico De Filippo (Istituto Nazionale di Fisica Nucleare)
    5/25/26, 5:00 PM
  13. Rémi Bougault (LPC/ENSI Caen)
    5/25/26, 5:30 PM
  14. Alessia Francesca Di Pietro (Istituto Nazionale di Fisica Nucleare)
    5/26/26, 9:30 AM

    The region of the nuclear chart corresponding to light radioactive nuclei has, over the years, yielded many surprising results, among others the discovery of the halo structure in neutron and proton dripline nuclei. This region of the nuclear chart is also rich of many other phenomena like the appearance of molecular-like structures where -particle-clusters are bound together by the exchange...

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  15. Martina Figuera (Università degli Studi di Catania)
    5/26/26, 10:15 AM

    M. Figueraᵃ, A. Di Pietroᵇ, N. Szegediᵇ, D. Torresiᵇ, P. Figueraᵇ, A. Shotterᶜ, R. J. de Boerᵈ, S.Cherubiniᵇᵃ, M. La Cognataᵇ, L. Guardoᵇ, M. Gulinoᵇᵉ, L. Lamiaᵇᵃ, A. Olivaᵇ, G. Pizzoneᵇᵃ, G.Rapisardaᵇᵃ, R. Spartaᵇᵉ, M. L. Sergiᵇᵃ, A. Tuminoᵇᵉ, T. Davinsonᶜ, N. Duyᶠ, J. P. Fernández Garcíaᵍ,S. Heinitzʰ, S. Hayakawaᶦ, E. A. Maugeriʰ, M. Milinʲ, A. Nurmukhanbetovaᵇᵉ, H. Shimizuᶦ, D.Schumannʰ, N....

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  16. Rosaria Cavallaro (Dipartimento di Fisica e Astronomia "E. Majorana", Università degli Studi di Catania & INFN-Sezione di Catania)
    5/26/26, 10:40 AM

    R. Cavallaro$^{*1,2}$, G. Cardella$^2$, N. S. Martorana$^2$, A. Castoldi$^3$, E. De Filippo$^2$, E. Gambera$^{1,2}$, E. Geraci$^{1,2,4}$, B. Gnoffo$^{1,2}$, C. Guazzoni$^3$, C. Maiolino$^5$, E. V. Pagano$^5$, S. Pirrone$^2$, G. Politi$^{1,2}$, F. Risitano$^{2,4,6}$, F. Rizzo$^{1,4,5}$, P. Russotto$^5$, M. Trimarchi$^{2,6}$, C. Zagami$^{4,5}$

    *1. Dipartimento di Fisica e Astronomia “E....

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  17. Ilham Dekhissi (LPC Caen)
    5/26/26, 11:05 AM

    The second $0_{2}^+$ state of $^{12}$C at an excitation energy of 7.654 MeV, known as the Hoyle state [1], is crucial to understanding how $^{12}$C is formed in stellar nucleosynthesis. Despite recent studies, there is no consensus on the properties of the Hoyle state, with different theoretical models predicting a range of radii values and spatial arrangements [2-3].

    Experimentally, only a...

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  18. Louis Heitz (CEA)
    5/26/26, 12:00 PM

    Clustering in finite nuclei is best understood not as an isolated peculiarity of a few light systems, but as a structural and dynamical regime whose signatures run from spectroscopy to decay. In this talk, I will discuss how cluster correlations emerge, evolve, and eventually disappear as nuclei are driven across density- and temperature-controlled regimes, including dilution-induced quantum...

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  19. Rodrigue Didier-Pichat (IJCLab)
    5/26/26, 12:45 PM

    It has been shown for several years that cluster states in nuclei could be understood through universal microscopic approaches [1, 2]. Furthermore, starting from a nuclear matter model including clusters, and with a finite nucleus-matter correspondence, it is possible to predict and observe alpha clusters at the surface of Tin isotopes[3]. Here, we present a unified theoretical framework for...

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  20. Carmelo Piazza (Istituto Nazionale di Fisica Nucleare), Carmelo Piazza (INFN - LNS & UniCT)
    5/26/26, 1:10 PM

    The formation of nuclear clusters, emerging as many-body correlations at sub-saturation densities, constitutes an essential feature for the construction of a reliable Equation of State (EOS). Phenomenological models based on energy density functionals (EDFs) offer a convenient approach to account for these bound states by introducing clusters as additional degrees of freedom (DOF)[1].
    In this...

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  21. Sylvie Hudan (Indiana University)
    5/26/26, 2:30 PM

    The effect of $N/Z$ has been probed through different processes such as reactions around the Fermi energy where nuclear dynamics is prominent. Alternatively, the fusion of two nuclei is a process where both the initial structure of the two nuclei and the collision dynamics can play an important role. Light nuclei in particular provide a rich testing ground for the interplay of nuclear...

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  22. Paolo Napolitani (IPN)
    5/26/26, 3:15 PM

    Taking as a reference the system $^{40,48}$Ca$+^{40,48}$Ca at 35 $A$MeV, recently measured at Ganil with the VAMOS-INDRA setup [1], we build a microscopic simulation of neutron and proton currents characterising nuclear systems at Fermi energies.
    In particular, we focus on the combination of collective and dissipative processes occurring at midrapidity, related to drifts and fluctuations, and...

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  23. Dan Cozma (IFIN-HH), Dan Cozma (IFIN-HH)
    5/26/26, 4:10 PM
  24. Arnaud Le Fèvre (GSI Helmholtzzentrum Darmstadt)
    5/26/26, 4:40 PM
  25. Paolo Russotto (Istituto Nazionale di Fisica Nucleare)
    5/26/26, 5:10 PM
  26. Jose Luis Rodriguez Sanchez (University of Coruña)
    5/27/26, 9:30 AM

    The SOFIA/R3B experimental setup at the GSI/FAIR facility (Darmstadt, Germany) is designed to exploit relativistic heavy-ion beams produced at the Fragment Separator (FRS), and in the future at the Super-FRS. These spectrometers deliver intense beams of exotic heavy nuclei, which are used as projectiles in inverse kinematics for fission studies performed with the SOFIA/R3B setup. Building on...

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  27. Lucia Baldesi (Istituto Nazionale di Fisica Nucleare)
    5/27/26, 10:15 AM

    We present a study of the reaction dynamics of semiperipheral 58Ni+58Ni collisions at 32, 52, and 74 MeV/nucelon through the reconstruction of primary sources and the study of their evolution with centrality and beam energy. The analysis exploits the capabilities of the INDRA–FAZIA apparatus, which combines large angular coverage with excellent isotopic resolution.
    After efficiency...

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  28. Silvia Piantelli (Istituto Nazionale di Fisica Nucleare)
    5/27/26, 10:40 AM

    Experimental data for the systems $^{16}$S+$^{40,48}$Ca at 17.7AMeV, collected with GARFIELD+RCO setup, have been investigated. In particular, the decay of hot sources formed both in highly dissipative binary collisions and in fusion reactions is considered, with a focus on the break up channel, where the light partner of the fission can also be reconstructed via particle correlations. The...

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  29. Dr Eulalia Gambera, Eulalia Gambera (Istituto Nazionale di Fisica Nucleare), Eulalia Gambera (student at Department of Physics and Astronomy " E. Majorana", University of Catania)
    5/27/26, 11:35 AM

    In March 2025, at the GSI laboratory in Germany, the ASY-EOS II experiment was conducted. The reaction ^{197}Au+^{197}Au was studied at beam energies of 280, 400, 600, and 1000 AMeV. The experiment was designed to investigate high-density nuclear matter and to provide a new and robust constraint on the symmetry energy term of the nuclear equation of state (EoS).
    Understanding the behavior of...

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  30. Seon Ho Nam (Korea University)
    5/27/26, 12:00 PM

    The nuclear symmetry energy and its density dependence, particularly above saturation density, remain among the most significant uncertainties in the nuclear equation of state (EoS). These properties play a crucial role in both intermediate-energy heavy-ion collisions and the structure of neutron star matter. Experimental information at supra-saturation densities, however, is still limited,...

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  31. Arnaud Le Fèvre (GSI Helmholtzzentrum Darmstadt)
    5/27/26, 12:25 PM

    A new method, based on comparing isotopic yield ratios measured at forward and sideward polar angles and on cross-bombarding heavy nuclei with different neutron-to-proton ratios, is used to quantify the stopping power of nuclear matter in heavy-ion collisions. For central collisions of isotopically separated 124,129Xe+112,124Sn at 100 MeV/nucleon bombarding energy, measured with the 4π...

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  32. Rémi Bougault (LPC/ENSI Caen)
    5/27/26, 12:50 PM

    Heavy ion collisions provide a unique laboratory for studying nuclear matter under extreme conditions. The mid-rapidity region, characterized by particles emitted perpendicular to the beam axis, shows experimentally a neutron enrichment. The isospin transport processes and the density-dependent behaviour of the symmetry energy affect the transport of nucleons to this region of interaction...

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  33. Bao-An Li (East Texas A&M University)
    5/28/26, 9:30 AM

    The trace anomaly of dense matter, $\Delta \equiv 1/3 - P/\varepsilon$, defined in terms of the ratio of pressure $P$ to energy density $\varepsilon$, quantifies deviations from conformal symmetry and plays a central role in both the hydrodynamic response and gravitational equilibrium. While $\Delta(\varepsilon)$ has recently been inferred from neutron star observations, we report the first...

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  34. Daniele Poidomani (CEA)
    5/28/26, 10:15 AM

    Neutrino physics is essential for understanding a wide range of astrophysical phenomena. In particular, neutrinos play a fundamental role throughout the entire collapse of a massive star—from the supernova explosion and the early evolution of compact stellar remnants to neutron star cooling and neutron star mergers.

    To calculate the opacity of nuclear matter to neutrinos, we employ the...

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  35. Silvia Piantelli (Istituto Nazionale di Fisica Nucleare)
    5/28/26, 10:40 AM

    A Bayesian analysis aimed at tuning two parameters of the AMD model related to the dynamical cluster formation and the in-medium nucleon-nucleon cross section was performed. The adopted technique required to produce a huge number of time-consuming simulations varying the relevant model parameters. A very preliminary attempt at making the parameter grid more rarefied in order to reduce the...

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  36. Brunilde Gnoffo
    5/28/26, 11:30 AM

    The NarCoS (Neutron Array for Correlation Studies) detector array has been developed for the simultaneous detection of neutrons and charged particles, in particular in heavy-ion collisions involving neutron-rich nuclei. Such measurements are essential for investigating reaction mechanisms and for nuclear spectroscopy studies in which neutron emission plays a central role.
    NarCoS is a compact,...

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  37. Dr Anna Togni for the ASFIN and GAMMA collaborations (Istituto Nazionale di Fisica Nucleare)
    5/28/26, 11:55 AM

    The facility EXOTIC at the Laboratori Nazionali di Legnaro (LNL, Italy) has been in operation for about 20 years for the production of light weakly-bound Radioactive Ion Beams (RIBs), employing two-body inverse kinematics reactions on a cryogenic gas target (e.g. [1,2] and references therein). The installation of the gamma-ray tracking spectrometer AGATA at LNL provided the unique opportunity...

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  38. Andrzej Kordyasz (Heavy Ion Laboratory - University of Warsaw)
    5/28/26, 12:20 PM

    Thin 20 µm n-type silicon was obtained using of selective dissolution n$^+$ - n structures. Obtained thin epitaxial silicon wafers were cut by laser into 21.3 mm X 21.3 mm squares. The thin silicon squares were collimated by 20 mm X 20 mm Al foil windows followed B$^+$ implantation with dose $5\cdot 10^{14}$ ions/cm$^2$ and energy about 50 keV. After that Al contacts were evaporated on both...

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  39. Alex Rebillard-Soulié (LPC CAEN)
    5/28/26, 12:45 PM

    For decades, physicists have relied on stopping power and range table to study ion-matter interactions. While advanced simulation tools such as SRIM and Geant4 provide detailed modeling of microscopic processes, their compexity often limits accessibility for non-expert users. In this work, we present an application designed to simulate one-dimensional ion propagation through material layers,...

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