BEGIN:VCALENDAR VERSION:2.0 PRODID:-//CERN//INDICO//EN BEGIN:VEVENT SUMMARY:Finding colliding galaxies in big data DTSTART;VALUE=DATE-TIME:20260305T081500Z DTEND;VALUE=DATE-TIME:20260305T091500Z DTSTAMP;VALUE=DATE-TIME:20260309T061742Z UID:indico-contribution-436-1939@events.ncbj.gov.pl DESCRIPTION:Speakers: Aidan Cotter ()\nIn the ΛCDM cosmological model\, t he evolution and mass build-up of galaxies is highly influenced by mergers . Key processes\, such as starbursts and active galactic nuclei\, along wi th major morphological changes are triggered by mergers. In order to effec tively study their role in the era of peta-byte scale galaxy surveys\, eff icient and reliable methods for identifying galactic mergers are essential . In this seminar I will review the most common methods of classifying mer gers in order to provide context for my work on designing updated and nove l identification techniques. This review will have a focus on the applicat ion of non-parametric morphological statistics which are a core aspect of my thesis. Using a set of HSC style mock images from the IllustrisTNG suit e of simulations\, I will benchmark the performance of statistical merger classification techniques against state-of-the-art machine learning method s. This analysis sets the stage for ongoing work developing new statistics to better classify merging galaxies in upcoming surveys such as Euclid an d LSST.\n\nhttps://events.ncbj.gov.pl/event/436/contributions/1939/ LOCATION:NCBJ Room 207 URL:https://events.ncbj.gov.pl/event/436/contributions/1939/ END:VEVENT BEGIN:VEVENT SUMMARY:First dust and gas insight in late stage galaxy evolution DTSTART;VALUE=DATE-TIME:20260122T081500Z DTEND;VALUE=DATE-TIME:20260122T091500Z DTSTAMP;VALUE=DATE-TIME:20260309T061742Z UID:indico-contribution-436-1887@events.ncbj.gov.pl DESCRIPTION:Speakers: Giuliano Lorenzon (NCBJ)\nQuiescent galaxies (QGs) h ave traditionally been viewed as the endpoint of galaxy evolution\, charac terized by the cessation of star formation and the rapid depletion of gas and dust in the interstellar medium (ISM). However\, over the past decade\ , infrared and sub-millimeter observations have challenged this picture by revealing the presence of dust or cold gas in a subset of quiescent syste ms\, particularly at high redshift.\nThe James Webb Space Telescope (JWST) began operations at the start of my PhD and has since transformed this fi eld by uncovering a larger and earlier population of QGs than previously e xpected. These discoveries have opened new questions about QGs: how do the y form? Do they evolve after quenching? Does quiescence truly represent a terminal phase of galaxy evolution?\nIn this short seminar\, I will provid e an overview of this emerging field and its implications for galaxy evolu tion and population studies. I will place particular emphasis on the surve y we performed with the sub-mm ALMA telescope\, which constitutes the firs t large sample of quiescent galaxies with simultaneous detections of both cold molecular gas and dust beyond the local universe. I will discuss how these data\, in synergy with JWST observations and state-of-the-art simula tions\, offer new insight into the residual ISM of quiescent galaxies and its role in their post-quenching evolution.\n\nhttps://events.ncbj.gov.pl/ event/436/contributions/1887/ LOCATION:NCBJ Room 207 URL:https://events.ncbj.gov.pl/event/436/contributions/1887/ END:VEVENT BEGIN:VEVENT SUMMARY:From theory to automation: Decoupling renormalization for BSM Higg s decays DTSTART;VALUE=DATE-TIME:20260115T081500Z DTEND;VALUE=DATE-TIME:20260115T091500Z DTSTAMP;VALUE=DATE-TIME:20260309T061742Z UID:indico-contribution-436-1883@events.ncbj.gov.pl DESCRIPTION:Speakers: Jonas Lang (National Center for Nuclear Research Pol and)\nHigh-precision calculations of Higgs boson observables can be used t o constrain models of Beyond the Standard Model (BSM) physics. Motivated b y the non-observation of light BSM particles at the LHC\, in this talk I w ill discuss a renormalization scheme for precise predictions of Higgs boso n decays in the presence of moderately heavy BSM physics at the 1-loop lev el. I will cover the basics of regularization and renormalization. Special focus will be on the decoupling renormalization scheme\, where I will pre sent the renormalization conditions for a generic model. I will also show application of the decoupling scheme in the two Higgs doublet model (THDM) to explore its caveats and effects. Finally\, I will sketch how this calc ulation becomes automatized as a part of FlexibleSUSY spectrum-generator g enerator.\n\nhttps://events.ncbj.gov.pl/event/436/contributions/1883/ LOCATION:NCBJ Room 207 URL:https://events.ncbj.gov.pl/event/436/contributions/1883/ END:VEVENT BEGIN:VEVENT SUMMARY:Hierarchical Cosmology Constraints through Strong Gravitational Le nsing DTSTART;VALUE=DATE-TIME:20260108T081500Z DTEND;VALUE=DATE-TIME:20260108T091500Z DTSTAMP;VALUE=DATE-TIME:20260309T061742Z UID:indico-contribution-436-1878@events.ncbj.gov.pl DESCRIPTION:Speakers: Shuaibo Geng (National Center for Nuclear Research)\ nStrong gravitational lensing\, a phenomenon where the gravitational field of a massive foreground galaxy distorts and magnifies the light from a di stant background source\, provides a unique astrophysical laboratory. It u niquely bridges studies of the very large and the very small\, enabling si multaneous investigation of the internal structure of galaxies and the glo bal geometry of the universe. This dual capability makes it a powerful too l for probing the two most significant constituents of the modern universe : dark matter and dark energy. Research on galaxy mass distributions via s trong lensing pertains to the nature of dark matter\, while the use of len sing as a cosmological probe informs our understanding of dark energy. How ever\, these two lines of inquiry are inherently intertwined.\nThis thesis focuses on developing a self-consistent framework to investigate both the redshift evolution of galaxy mass distributions and cosmological paramete rs\, with the aim of decoupling their mutual dependencies. We first presen t a model-independent method to study the mass profile evolution in lens g alaxies. By training a non-parametric artificial neural network (ANN) on T ype Ia supernova data to reconstruct the distance-redshift relation\, we c ompare the inferred distance ratios with predictions from lens models. App lied to a combined sample of 161 lenses\, this approach measures a signifi cant redshift evolution in the extended power-law mass density slope\, wit h the total mass profile steepening at lower redshifts. The method was val idated with mock data based on LSST forecasts\, which also project high pr ecision for future large samples.\nWe subsequently extend this framework t o a hierarchical cosmological analysis using distance ratios derived from strong lensing. A Fisher-based sensitivity study identifies "sensitivity v alleys" in the lens-source redshift plane where cosmological constraining power diminishes. By incorporating the prior on mass-profile evolution cal ibrated in the first part of the study\, we reconstruct distance ratios fr om lensing observables and compare them to cosmological predictions. This hierarchical scheme allows for joint constraints on both mass-profile evol ution and cosmological parameters within a single\, unified analysis. The degeneracies between these probes are broken by incorporating external dat asets. In a flat $w$CDM model\, combining strong lensing distance ratios w ith \\textit{Planck} CMB data yields a constraint on the dark energy equat ion of state parameter of $w=-1.52^{+0.18}_{-0.19}$. In the flat $w_{\\phi }$CDM model\, adding DESI BAO data provides a measurement of the matter de nsity parameter $\\Omega_m=0.256^{+0.031}_{-0.018}$. This work establishes a robust\, integrated methodology for advancing our understanding of gala xy evolution and cosmology through the large sample of strong gravitationa l lensing.\n\nhttps://events.ncbj.gov.pl/event/436/contributions/1878/ LOCATION:NCBJ Room 207 URL:https://events.ncbj.gov.pl/event/436/contributions/1878/ END:VEVENT BEGIN:VEVENT SUMMARY:Study of the Vector Boson Scattering $W^{\\pm}W^{\\pm}$ production at $\\sqrt{s}=13.6~\\mathrm{TeV}$ DTSTART;VALUE=DATE-TIME:20251218T081500Z DTEND;VALUE=DATE-TIME:20251218T091500Z DTSTAMP;VALUE=DATE-TIME:20260309T061742Z UID:indico-contribution-436-1877@events.ncbj.gov.pl DESCRIPTION:Speakers: Monika Ghimiray ()\nIn this seminar\, I will present a study of Vector Boson Scattering (VBS) at the Compact Muon Solenoid (CM S) experiment at CERN\, focusing on same-sign $W^{\\pm}W^{\\pm}$ scatterin g and its sensitivity to physics beyond the Standard Model. The analysis t argets the leptonic final state with two same-sign charged leptons\, two n eutrinos\, and two forward tagging jets\, providing a clean handle on the electroweak nature of VBS and its characteristic event topology. I will ou tline the main experimental challenges\, emphasizing the dominant backgrou nd contributions and the strategies used to control them — particularly reducible backgrounds from non-prompt leptons\, which are among the most s ignificant sources of contamination. I will also present the expected cros s-section measurements for this channel. Finally\, I will introduce the in terpretation within the Standard Model Effective Field Theory (SMEFT) fram ework\, highlighting some preliminary results from the phenomenology part of my project\, and conclude with an outlook on future SMEFT studies.\n\nh ttps://events.ncbj.gov.pl/event/436/contributions/1877/ LOCATION:NCBJ Room 207 URL:https://events.ncbj.gov.pl/event/436/contributions/1877/ END:VEVENT BEGIN:VEVENT SUMMARY:Study of recurrent activity in radio sources DTSTART;VALUE=DATE-TIME:20251211T081500Z DTEND;VALUE=DATE-TIME:20251211T091500Z DTSTAMP;VALUE=DATE-TIME:20260309T061742Z UID:indico-contribution-436-1875@events.ncbj.gov.pl DESCRIPTION:Speakers: ANUPAMA MOHANAN ()\nPeaked-spectrum (PS) radio sourc es are widely regarded as tracers of the earliest stages of radio jet evol ution. Milliarcsecond VLBI imaging frequently reveals compact double morph ologies embedded within kiloparsec-scale cocoons\, suggesting that many PS sources have the potential to grow into large FR I or FR II radio galaxie s. However\, a key open question remains: Do PS sources typically evolve i nto large-scale radio galaxies\, or do they instead undergo short\, interm ittent bursts of activity separated by long quiescent phases? Over the pas t three decades\, only a handful of PS AGN have been found inside older\, faint radio cocoons\, leaving the duty cycle of young radio jets poorly co nstrained. Earlier wide-area surveys lacked the surface-brightness sensiti vity and angular resolution to identify these “compact core + relic emis sion” systems in statistically significant numbers. Recent advances in l ow-frequency radio interferometry have made it possible to detect faint\, low-surface-brightness emission that was previously inaccessible. In this talk\, I will first introduce the fundamental concepts of radio astronomy\ , AGN\, radio galaxy morphology\, and the evolutionary role of compact pea ked-spectrum sources. I will then present the motivation and scientific go als of my PhD research\, which aims to probe the duty cycle and restarted activity of radio sources. Using multi-frequency radio surveys\, including LoTSS\, we search for diffuse\, relic emission around compact PS cores pr oviding direct evidence of earlier cycles of jet activity and offering new insights into the episodic nature of young radio galaxies.\n\nhttps://eve nts.ncbj.gov.pl/event/436/contributions/1875/ LOCATION:NCBJ Room 207 URL:https://events.ncbj.gov.pl/event/436/contributions/1875/ END:VEVENT BEGIN:VEVENT SUMMARY:Search for hadron exotics in the new decay modes of the $B^0$ meso n at LHCb DTSTART;VALUE=DATE-TIME:20251204T081500Z DTEND;VALUE=DATE-TIME:20251204T083500Z DTSTAMP;VALUE=DATE-TIME:20260309T061742Z UID:indico-contribution-436-1874@events.ncbj.gov.pl DESCRIPTION:Speakers: Salil Joshi (NCBJ)\nSpectroscopic studies of multi-q uark hadrons in the charmonium sector are crucial in providing powerful in sights into the intricacies of quantum chromodynamics (QCD) in the non-per turbative regime. Describing these hadrons as bound quark systems from fir st principles is challenging\, but experimental observations in the last 2 0 years have driven the progress\, with the discovery of nearly 30 exotic hadron candidates. It is this pattern of one unexpected result after anoth er\, with the emergence of desperately few connections\, that has characte rized the studies in this field. The LHCb experiment\, with its unique cap ability to cover the large heavy-quark production cross-section at the LHC \, offers a great window of opportunity to explore heavy hadron spectrosco py\, in both the conventional and exotic sectors.\n\nThis presentation is a synopsis of our work in search of QCD exotica in two new decay modes of the $B^0$ meson\, which are $B^0 \\rightarrow J/\\psi\\pi^+\\pi^-\\pi^0K^- \\pi^+$ and $B^0 \\rightarrow J/\\psi\\omega K^-\\pi^+$. In each case we m easure the Branching fraction and search for higher charmonium exotics as intermediate states in the LHCb data\, collected from Run 1 (2011-2012) an d Run 2 (2015-2018) in proton-proton collisions.\n\nhttps://events.ncbj.go v.pl/event/436/contributions/1874/ LOCATION:NCBJ Room 207 URL:https://events.ncbj.gov.pl/event/436/contributions/1874/ END:VEVENT BEGIN:VEVENT SUMMARY:Probes of light dark matter in relativistic regime DTSTART;VALUE=DATE-TIME:20251127T080000Z DTEND;VALUE=DATE-TIME:20251127T090000Z DTSTAMP;VALUE=DATE-TIME:20260309T061742Z UID:indico-contribution-436-1873@events.ncbj.gov.pl DESCRIPTION:Speakers: Jyotismita Adhikary (NCBJ)\nDark matter interactions are traditionally probed in the non-relativistic regime characteristic of cold DM in the present-day universe. However\, this strategy is insuffici ent for probing a class of important thermal DM targets for which non-rela tivistic scattering rates are highly suppressed. This opens an unexplored region of parameter space and motivates the development of detection strat egies specifically tailored to low-mass dark matter. In this talk\, I will discuss examples of such models and outline novel detection strategies de signed to probe them — either directly\, or indirectly through the detec tion of light dark-sector mediators.\n\nhttps://events.ncbj.gov.pl/event/4 36/contributions/1873/ LOCATION:NCBJ Room 207 URL:https://events.ncbj.gov.pl/event/436/contributions/1873/ END:VEVENT BEGIN:VEVENT SUMMARY:Multidimensional Framework for Modeling Fusion and Fission of Heav iest Nuclei DTSTART;VALUE=DATE-TIME:20251120T081500Z DTEND;VALUE=DATE-TIME:20251120T091500Z DTSTAMP;VALUE=DATE-TIME:20260309T061742Z UID:indico-contribution-436-1872@events.ncbj.gov.pl DESCRIPTION:Speakers: Aleksander Augustyn (NCBJ)\nThis work presents the d evelopment of a comprehensive computational framework for modeling fusion and fission processes in heavy and superheavy nuclei (Z ≥ 90). The frame work is based on the Warsaw Macroscopic-Microscopic Model (WMMM)\, extende d to incorporate multiple shape parameterizations\, including the traditio nal beta parameterization and the Fourier-over-Spheroid (FoS) approach\, w hich enables description of nuclear shapes from compact configurations to scission.\n\nThe framework combines several methodological advances in sha pe parameterization conversion\, model modernization\, and large-scale com putational capabilities to generate multidimensional potential energy surf aces spanning over 100 million configurations per nucleus. Stochastic shap e evolution is described through both simplified and sophisticated formali sms\, enabling predictions of fusion probabilities\, ground state properti es\, fission barriers\, and mass fragment distributions. Applications to s uperheavy elements and actinide systematics demonstrate the framework's ab ility to reproduce experimental observables without parameter fitting\, su ggesting promising prospects for a unified theoretical description of fusi on-fission dynamics across the heavy element region.\n\nhttps://events.ncb j.gov.pl/event/436/contributions/1872/ LOCATION:NCBJ Room 207 URL:https://events.ncbj.gov.pl/event/436/contributions/1872/ END:VEVENT BEGIN:VEVENT SUMMARY:Ultra-Diffuse Galaxies study DTSTART;VALUE=DATE-TIME:20251113T081500Z DTEND;VALUE=DATE-TIME:20251113T091500Z DTSTAMP;VALUE=DATE-TIME:20260309T061742Z UID:indico-contribution-436-1869@events.ncbj.gov.pl DESCRIPTION:Speakers: Antonio Vanzanella (National Centre for the Nuclear Research\, Pasteura 7\, 02-093 Warsaw\, Poland)\nLow Surface Brightness Ga laxies (LSBGs) are defined as galaxies with an average central surface bri ghtness\, 𝜇(0\,r)\, below the typical level of the night sky. LSBGs are estimated to contribute less than 1% to the luminosity of the local obser vable universe\; however\, their contribution to the total number density of galaxies is estimated to be around 40% to 50%. Exploring the standard e volution of LSBGs and investigating the reasons behind their faint nature could be crucial to understanding our universe. Among LSBGs\, a subsample of objects has been identified: classified as Ultra Diffuse Galaxies (UDGs )\, which are LSBGs having a central surface brightness measured in g-band \, 𝜇(0\,g)\, larger than 24 mag per arcsec² and an extended half-light radius\, r{1/2}\, larger than 1.5 kpc. UDGs populate the distribution tai l of the LSBGs' luminosity profile\, inhabiting field\, group and cluster environments. Previous studies have established substantial differences in the properties of UDGs according to their host environment. Comparing pro perties in different UDGs hosting environments would allow us to find the most likely evolutionary path of these galaxies\, factoring out the episod ic events due to their surroundings. In our work\, we validated the perfor mance of a Machine Learning model developed to find LSBGs and UDGs\, extra cting also physical properties of LSBGs/UDGs through redshift measurements such as star formation rates (SFRs) and stellar masses(Mstar).\n\nhttps:/ /events.ncbj.gov.pl/event/436/contributions/1869/ LOCATION:NCBJ Room 207 URL:https://events.ncbj.gov.pl/event/436/contributions/1869/ END:VEVENT BEGIN:VEVENT SUMMARY:From gravitational symmetries to the area law DTSTART;VALUE=DATE-TIME:20251106T081500Z DTEND;VALUE=DATE-TIME:20251106T091500Z DTSTAMP;VALUE=DATE-TIME:20260309T061742Z UID:indico-contribution-436-1868@events.ncbj.gov.pl DESCRIPTION:Speakers: Ludovic Varrin ()\nThe complete structure of quantum gravity remains unknown to this day. A recent line of research proposes u sing the symmetries of gravity as a guiding principle in the search for it s quantum formulation. In this talk\, I will present our approach\, which employs these symmetries to classify the possible quantum gravitational st ates associated with a subregion of spacetime. I will further show that ou r formalism naturally leads to a computation of the entanglement entropy o f such subregions. Finally\, I will argue that\, in the classical limit\, the leading term of this entanglement entropy scales with the area of the subregion’s boundary\, thus recovering the famous Bekenstein–Hawking a rea law and strengthening the case for a symmetry-based approach to quantu m gravity.\n\nhttps://events.ncbj.gov.pl/event/436/contributions/1868/ LOCATION:NCBJ Room 207 URL:https://events.ncbj.gov.pl/event/436/contributions/1868/ END:VEVENT BEGIN:VEVENT SUMMARY:CMB Lensing with TEReSiTA DTSTART;VALUE=DATE-TIME:20251030T081500Z DTEND;VALUE=DATE-TIME:20251030T091500Z DTSTAMP;VALUE=DATE-TIME:20260309T061742Z UID:indico-contribution-436-1866@events.ncbj.gov.pl DESCRIPTION:Speakers: Nicola Principi (NCBJ)\nWe are currently living in t he most scientifically active era of the human kind: cosmology makes no ex ception. Our understanding of the Universe has radically changed during th e last decades. However\, while many long-standing questions about the nat ure of the Universe have been answered\, many others have emerged. Why is the Universe's expansion accelerating? What is dark energy? What is dark m atter? How does inflation work?\nThe study of the Cosmic Microwave Backgro und\, together with other cosmological probes\, is one of the ways we can answer these new questions. In particular\, studying the weak gravitationa l lensing effect of large-scale structure on the CMB photons\, we can obta in information about both the primordial and the late-time Universe. I wil l show how.\nIn this talk\, I present the Tomographic Ensamble of Realisti c Simulations of Tracers and Anisotropies (TEReSiTA): a set of simulations of correlated galaxy catalogues and CMB observations. TEReSiTA\, my origi nal work\, is a very useful and versatile tool for testing new paths in th e quest for high-precision cosmological parameter estimation.\n\nhttps://e vents.ncbj.gov.pl/event/436/contributions/1866/ LOCATION:NCBJ Room 207 URL:https://events.ncbj.gov.pl/event/436/contributions/1866/ END:VEVENT BEGIN:VEVENT SUMMARY:Study of direct photon production in Pb-Pb collisions at $\\sqrt { s_{NN}}$ = 5.02 TeV with ALICE experiment’s Photon Spectrometer (PHOS) a t Large Hadron Collider DTSTART;VALUE=DATE-TIME:20251023T071500Z DTEND;VALUE=DATE-TIME:20251023T073500Z DTSTAMP;VALUE=DATE-TIME:20260309T061742Z UID:indico-contribution-436-1862@events.ncbj.gov.pl DESCRIPTION:Speakers: Sushobhan Mandal (NCBJ)\nThe Quark-Gluon Plasma (QGP )\, a state of deconfined quarks and gluons\, is believed to have existed in the early Universe shortly after the Big Bang. As the QGP cools\, it tr ansitions into the hadronic matter we observe today. In laboratory setting s\, small-scale "Big Bangs" are created through high-energy heavy-ion coll isions\, which heat the hadronic matter above the transition temperature\, approximately 150 MeV\, resulting in the formation of the QGP. Direct pho tons serve as unique probes in high-energy proton-proton and nucleus-nucle us collisions due to their weak interaction with the dense and hot quark-g luon medium. These photons escape the medium unaltered\, providing undisto rted information about the collision's evolution.\nIn the ALICE experiment at the Large Hadron Collider (LHC)\, photons from lead-lead collisions ar e measured using techniques such as the Photon Conversion Method and Elect romagnetic Calorimeter. The Photon Spectrometer (PHOS)\, offering high-pre cision photon detection\, was used for our analysis (with Run 2 data in Pb -Pb collisions at $\\sqrt {s_{NN}}$ = 5.02 TeV) to measure inclusive photo ns and simulate decay photons\, aiding in the derivation of direct photon spectra. By disentangling the contributions of decay\, prompt and thermal photons emitted during these collisions\, we can estimate the effects of c old and hot nuclear matter and gain insights into the temperature\, correl ations\, and collective phenomena within the QGP.\n\nhttps://events.ncbj.g ov.pl/event/436/contributions/1862/ LOCATION:NCBJ Room 207 URL:https://events.ncbj.gov.pl/event/436/contributions/1862/ END:VEVENT BEGIN:VEVENT SUMMARY:Production of Self Interacting Scalars in the Early Universe DTSTART;VALUE=DATE-TIME:20251016T071500Z DTEND;VALUE=DATE-TIME:20251016T073500Z DTSTAMP;VALUE=DATE-TIME:20260309T061742Z UID:indico-contribution-436-1861@events.ncbj.gov.pl DESCRIPTION:Speakers: Juan Esau Cervantes Hernandez (NCBJ Warsaw)\nIn this talk\, I will present an overview of my research on Dark Matter (DM). I w ill begin with a brief introduction to the study of DM across different ap proaches\, before focusing on Cannibal DM produced via the freeze-in mecha nism in the early Universe. I will discuss the non-trivial thermal dynamic s of this scenario and the importance of tracking the DM temperature evolu tion. I will then outline the resulting detectability prospects\, which be come viable in non-standard cosmological histories\, particularly when the early Universe is dominated by a cold inflaton field. In the second part\ , I will turn to cosmological phase transitions\, emphasizing how first-or der transitions can generate observable gravitational waves (GWs). Finally \, I will show that an inverse phase transition can occur within the freez e-in framework\, where cannibalization dynamics crucially modify the evolu tion of the transition and the associated GW phenomenology\, potentially w ithin reach of future interferometer experiments.\n\nhttps://events.ncbj.g ov.pl/event/436/contributions/1861/ LOCATION:NCBJ Room 207 URL:https://events.ncbj.gov.pl/event/436/contributions/1861/ END:VEVENT BEGIN:VEVENT SUMMARY:Discussion about the goals and organization of the PhD seminar¶ DTSTART;VALUE=DATE-TIME:20251009T073500Z DTEND;VALUE=DATE-TIME:20251009T075500Z DTSTAMP;VALUE=DATE-TIME:20260309T061742Z UID:indico-contribution-436-1852@events.ncbj.gov.pl DESCRIPTION:Speakers: Anna Durkalec (National Centre for Nuclear Research) \, Jakub Wagner (National Centre for Nuclear Research)\, Michal Bluj (NCBJ )\nhttps://events.ncbj.gov.pl/event/436/contributions/1852/ LOCATION:NCBJ Room 207 URL:https://events.ncbj.gov.pl/event/436/contributions/1852/ END:VEVENT BEGIN:VEVENT SUMMARY:Welcoming Talk of the Graduate School Director¶ DTSTART;VALUE=DATE-TIME:20251009T071500Z DTEND;VALUE=DATE-TIME:20251009T073500Z DTSTAMP;VALUE=DATE-TIME:20260309T061742Z UID:indico-contribution-436-1851@events.ncbj.gov.pl DESCRIPTION:Speakers: Michał Spaliński ()\nhttps://events.ncbj.gov.pl/ev ent/436/contributions/1851/ LOCATION:NCBJ Room 207 URL:https://events.ncbj.gov.pl/event/436/contributions/1851/ END:VEVENT END:VCALENDAR