Double beta decay is among the rarest radioactive processes, observed only in a few even–even nuclei near the valley of stability. Although the phenomenon itself is well established, it provides a stringent consistency test for nuclear states predicted within contemporary theoretical frameworks. Such validation is of paramount importance for reliable modeling of the yet unobserved neutrinoless double beta (0νββ) decay process.
The presentation focuses on the foundations of 2νββ decay and on the the- oretical treatment of spherical (48Ca) and highly triaxial (76Ge) 2νββ-active nuclei within a Skyrme SV density-functional No-Core CI (DFT-NCCI) frame- work developed by our group. The approach restores rotational symmetry and mixes states projected from self-consistent mean-field configurations obtained by solving the Hartree–Fock equations with a density-independent local Skyrme interaction.
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 10:15

dr Olga Polak (Narodowe Centrum Badań Jądrowych)
Multi-humped fission barriers, as they occur in the actinide region, give rise to fission isomerism. Such barrier shapes can be described within various theoretical models. Experimentally measured observables of nuclear fission isomers—such as the half-life, excitation energy of the fission isomer, kinetic energy of the fission fragments, and the isomer-to-ground-state population ratio—allow for testing theoretical predictions and verifying the role of shell effects in nuclear structure.
Studies of the fission isomer properties of 240,242Am were performed at the IGISOL facility at the JYFL Accelerator Laboratory, University of Jyväskylä, Finland. Fission isomeric states were populated via deuteron-induced fusion–evaporation reactions on a 242Pu target. The decays of the fission isomers were detected using silicon detectors calibrated with a 252Cf fission source.
The measurements provided detailed information on kinetic energy spectra, total kinetic energies, and mass distributions for 240,242Am. A new method was proposed to derive post-neutron-emission mass distributions, as well as proton- and neutron-number multiplicity distributions of the fission fragments, from their kinetic energy distributions. In addition, the emission probabilities of prompt neutrons in the fission process were extracted. Using data for the 252Cf fission isomer as a reference, the validity of the method was verified.
The obtained results for 240,242Am and 252Cf are consistent with GEF model predictions and previous measurements. These findings contribute to a better understanding of shell effects and fission barrier structures in the actinide region.
Zapraszamy do sali 1.01, ul. Pasteura 5 o godzinie 10:15

dr Aleksandra Fijałkowska (IFD, UW)
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