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Anton Repko (Institute of Physics SAS, Bratislava, Slovakia)30/09/2026, 09:00Invited lecture
The routine calculations of atomic nuclei within Energy-Density Functionals (EDF), such as Skyrme or Gogny, usually don't count with electrons, which however tend to be bound to the experimentally measured nuclei. Besides total electron binding energy, which is indeed subtracted in the modern fits of EDF parametrizations, we should also scrutinize the fact that the inner electron orbitals...
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Barbara Sulignano (cea saclay)30/09/2026, 09:30Invited lecture
Multinucleon transfer (MNT) reactions between very heavy nuclei provide a promising pathway to access neutron-rich heavy nuclei that are difficult, or impossible, to produce through conventional fusion-evaporation reactions. In particular, collisions involving actinide nuclei may offer new opportunities to explore the region towards the heaviest elements and to investigate the interplay...
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Kohta Nakajima (Kindai Universtiy)30/09/2026, 10:00Seminar
Introduction
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The synthesis of neutron-rich heavy nuclei is essential for exploring study of islands of stability and understanding the astrophysical r-process. However, conventional fusion reactions have significant limitations in producing neutron-rich nuclei in the heavy and superheavy mass regions. In recent years, multinucleon transfer (MNT) reactions have therefore attracted considerable... -
Jun Su (Sun Yat-sen University)30/09/2026, 10:50Invited lecture
Intermediate-energy heavy-ion reactions provide essential tools for studying nuclear sizes, fragmentation mechanisms, single-particle strength, and isospin dynamics in stable and exotic nuclei. Traditionally, many inclusive reaction cross sections have been interpreted as rather direct probes of nuclear structure, such as proton radii from charge-changing cross sections, spectroscopic strength...
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Michal Ciemala (IFJ PAN)30/09/2026, 11:20Invited lecture
Atomic nuclei exhibit fundamental collective vibrational modes, such as Giant Resonances (GR) and Pygmy Dipole Resonances (PDR), which provide insights into many-body nuclear dynamics, the nuclear equation of state, and astrophysical processes. In recent years, the proton facility at the Cyclotron Centre Bronowice (CCB) of the Henryk Niewodniczański Institute of Nuclear Physics PAN in Kraków...
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Hritik Gogoi (IFJ PAN)30/09/2026, 11:50Seminar
The FINESSE program at the European Spallation Source (ESS) in Lund, Sweden, is a high-precision experimental project designed to search for physics beyond the Standard Model. It aims at neutron-to-antineutron ($n\to\bar{n}$) and neutron-to-sterile/mirror-neutron oscillations ($n\to n'$), corresponding to baryon number violations of $\Delta B = 2$ and $\Delta B = 1$, respectively. Moreover, a...
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Gabriel Pietraszek (Uniwersytet Marii Curie-Skłodowskiej)30/09/2026, 12:10Short seminar
The Pacific Ocean Neutrino Experiment (P-ONE) is a next-generation neutrino telescope currently under development. It will detect the faint flashes of Cherenkov light produced when high-energy neutrinos interact in seawater. One of the major challenges in neutrino detection is distinguishing genuine physics signals from various sources of optical background noise. In this project. I...
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Paweł Strepikowski (Warsaw University of Technology)30/09/2026, 12:20Short seminar
In heavy-ion collisions, primary focus is often given to the participant zone and particles created there. However, recent research demonstrates that spectators that survive the collision play a crucial role in analyzing the Quark-Gluon plasma (QGP) and the trajectories of the particles produced [1,2] due to electromagnetic interaction. Studying de-excitation processes such as evaporation,...
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Igor Ciarciński (Politechnika Warszawska)30/09/2026, 12:30Short seminar
In ultrarelativistic heavy ion collisions, apart from the quark-gluon
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plasma being produced, part of the projectile or target nucleus may
survive the collision without directly participating in the interaction.
This nucleus is referred to as a spectator.
The particles could be created within participant zone but also during
the deexcitation of the hot spectators. Space-time evolution of...
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