Seminarium poświęcone będzie technice pełnej absorpcji, będącej ważnym narzędziem w badaniach rozpadu beta egzotycznych jąder atomowych i towarzyszącego mu promieniowania gamma. W pierwszej części omówione zostaną podstawowe założenia techniki oraz powody, dla których stanowi ona skuteczną alternatywę dla klasycznych pomiarów spektroskopowych, m.in. w kontekście problemu Pandemonium.
W drugiej części seminarium zaprezentowane zostaną możliwości, jakie daje technika pełnej absorpcji w badaniach struktury jąder atomowych. Omówione zostaną przykłady eksperymentów, w których technika ta została wykorzystana w praktyce, w tym pomiary wykonane z użyciem detektora LUCRECIA w ISOLDE, CERN oraz układu MTAS w ośrodku FRIB. Pokazane wyniki zilustrują potencjał techniki pełnej absorpcji oraz jej znaczenie dla współczesnej fizyki jądrowej.
Zapraszamy na spotkanie o godzinie 10:15

Dr Cézar Domingo Pardo (Instituto de Física Corpuscular, Valencia, Hiszpania)
Neutron-capture reactions drive the nucleosynthesis of all elements heavier than iron, both via the slow (s-) neutron-capture process during the evolution of low-mass AGB- and massive stars, as well as in the rapid (r-) neutron-capture process during explosive stellar environments.
Unstable s-process branching isotopes offer a unique insight about this mechanism of nucleosynthesis. Neutron-capture measurements on radioactive isotopes, in combination with spectroscopic observations of stellar photospheres and isotopic analysis of primitive meteorites, help to gather unique information about the physical conditions of the stellar environment and the chemical evolution of our galaxy. Experimentally, however, measuring neutron-capture cross sections on radioactive isotopes represents yet one of the most remarkable challenges, mainly due to the difficulties ascribed to the production of a high-quality sample for such experiments, as well as to the sensitivity and selectivity required for the capture reaction channel of interest.
This contribution will present a brief summary about the main s-process branching isotopes measured at CERN n_TOF over the last two decades, thereby showing the corresponding astrophysical implications of the different studies. It will be shown how upgrades in the neutron-beam facility, as well as novel detector developments, have led to a stunning progress in the measurement of radioactive samples. However, in most cases, important limitations still exist related to the lowest accessible isotopic half-life (> few y), the covered neutron-energy ranges (< few keV) and the statistical accuracy (>10%). Some of the future plans at CERN n_TOF to advance further in this field will be presented along with novel initiatives and efforts for overcoming current limitations for the measurement of short-lived nuclei.
Dołącz do spotkania Zoom od godz. 10:00 AM Warszawa
https://uw-edu-pl.zoom.us/j/98722620830?pwd=2wB3UY5ZQbISaeE1D2EVcxH6elnbCr.1
Identyfikator spotkania: 987 2262 0830
Kod dostępu: 917334
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 10:15

dr hab. Radosław Ryblewski, prof. IFJ PAN (Kraków)
Relativistic hydrodynamics has become a central tool for describing the collective behavior of many-body systems on many different scales — from the quark–gluon plasma to astrophysical plasmas. Traditionally, however, hydrodynamics cares only about energy, momentum, and conserved charges, while an intrinsically quantum property of matter—spin—is averaged out. Recent measurements of spin polarization of particles emitted in relativistic heavy-ion collisions challenge this separation: the produced quark–gluon plasma appears not only to flow like a nearly perfect fluid, but also to carry a sizable, dynamically generated spin polarization aligned with its vorticity.
In this talk, I will discuss how these observations motivate an extension of relativistic hydrodynamics that treats spin as an active degree of freedom. I will outline the basic ingredients of such a “spin hydrodynamics” framework, highlight its connection to underlying quantum kinetic theory, and show how it can be applied to interpret spin polarization measurements in heavy-ion collisions. I will conclude with a brief overview of open questions.
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 10:15

Dr Yannen Jaganathen (NCBJ)
In this seminar, I will explore the phenomenon of genuine ternary fission, the spontaneous breakup of a nucleus into three medium-mass fragments, using fully self-consistent Hartree–Fock–BCS calculations with the SLy6 Skyrme interaction. Building on our earlier work in the actinide region, we extend the investigation to superheavy nuclei, where stronger Coulomb repulsion, extreme deformations, and elongated shapes may (or may not) offer new pathways to ternary breakup.
A central focus will be the construction of self-consistent energy landscapes for two distinct ternary geometries: collinear tripartition, in which fragments align along a single axis, and equatorial tripartition, where fragments emerge in a triangular arrangement. A simplified Langevin-based framework is used to estimate the dynamical competition between ternary and the overwhelmingly dominant binary fission. By combining these approaches for both heavy and superheavy systems, the seminar will address the broader question: to what extent can genuine ternary fission survive the strong dynamical suppression acting along its fission path?
Zapraszamy na spotkanie o godzinie 10:15

Oscar Le Noan (IPHC Strasbourg)
Understanding how atomic nuclei respond to electromagnetic perturbations provides key insights into their structure and dynamics. In this talk, I will introduce the concept of nuclear response functions, focusing on the electric dipole (E1) mode, one of the most fundamental collective excitations in nuclei. After a brief overview of the main types of nuclear modes (isoscalar vs. isovector, collective vs. single-particle), I will present how these can be theoretically described within the Configuration Interaction Shell Model (CI-SM) framework.
Using the CI-SM, we have systematically computed the E1 strength distributions for all long-lived nuclei in the sd- and p-shell regions. These calculations allow a detailed comparison with predictions from the Quasiparticle Random Phase Approximation (QRPA) and available photoabsorption data. Particular attention will be given to the Pygmy Dipole Resonance (PDR), a low-energy mode that reflects subtle aspects of neutron–proton dynamics. I will discuss how the structure and evolution of the PDR along the Neon and Oxygen isotopic chains shed light on its collectiveness and its classical interpretation as a neutron-skin oscillation mode.