Tag Archives: Evento scientifico

Speaker: Yury Cherepennikov Based on own experience, this seminar presents a summary of research activities conducted by the author within International collaborations since 2012 in the field of applied X-ray optics and imaging, followed by the discussion on prospective research directions at LNF. The presentation addresses the development of compact accelerator-based X-ray sources and advanced X-ray optical systems, such as adaptive crystal monochromators controlled by external stimuli and polycapillary optics for the generation of high-intensity monochromatic radiation. Their implementation in applied X-ray imaging and analytical techniques for industrial applications is discussed. Particular attention is given to the use of polycapillary optics in advanced imaging systems and to the integration of 3D printing technologies for the fabrication of customized components for radiation imaging and radiation therapy setups.

This one‑afternoon workshop brings together researchers working at the interface of axion physics and Lattice QCD. Owing to the recent developments, predictions for the axion mass have been significantly improved and the role of cosmological aspects clarified. Particular attention will be devoted to topology, θ‑dependence, topological susceptibility, and onto the possibility of recent lattice advances to further sharpening predictions in these areas. Moreover, the workshop will address the recent challenge posed by a proposed GeV‑scale axion scenario in which the up‑quark mass arises dynamically from the QCD condensate, implying that the axion could be hidden among known pseudoscalar resonances. Resolving this question conclusively will require dedicated lattice studies of the corresponding deformed QCD theory. The workshop aims to highlight recent progress, clarify open problems, and identify opportunities for new breakthroughs at the intersection of axion theory and Lattice QCD. This activity is part of the Theoretical Phenomenology Visiting Institute @ LNF, running from 23 to 27 March 2026 and from 7 to 10 April 2026, and supported by CSN4 to promote the participation of early-career scientists.  

Speaker: Claudio Bonanno (IFIC) I will review the current state of affairs concerning non-perturbative QCD inputs for axion phenomenology. I will provide a systematic survey of existing lattice QCD results, and I will outline how they compare with up-to-date predictions coming from chiral effective theories and semiclassics. I will conclude delineating the future challenges that await this field in the near future, and what are the current perspectives to meet them.

Speaker: Ruben Gargiulo (La Sapienza Univ., Roma) Future colliders, including proposed Higgs factories, pose demanding requirements on calorimetry. In particular, precision measurements of Higgs boson properties and multi-jet final states require significant improvements in jet energy resolution. These requirements can be addressed through fine transverse granularity, longitudinal segmentation, and optical dual-readout. Such features allow efficient particle-flow jet reconstruction, photon and neutral pion separation, and reduced fluctuations in the reconstructed energy of hadronic showers due to invisible energy lost in nuclear breakup and reactions. This talk reviews the physics motivations behind the stringent jet energy resolution requirements of Higgs factories and discusses detector concepts currently being explored, including ongoing activities within the DRD6 collaboration. Particular emphasis is placed on how jet energy resolution requirements influence the design of the electromagnetic section of calorimeters while maintaining excellent electromagnetic energy resolution and timing performance. A significant example is the R&D on the CRILIN electromagnetic calorimeter, based on small Cherenkov crystals with longitudinal segmentation and a timing resolution of about 20 ps, developed at LNF for the muon collider but suitable for several future colliders  

Speaker: Davide Giusti With the advancement of precision physics in the Flavor sector, tests of the unitarity of the Cabibbo-Kobayashi-Maskawa (CKM) quark mixing matrix are playing an increasingly significant and impactful role in understanding the limits of the Standard Model of particle physics. Achieving exquisite precision in current and future experiments requires theoretical predictions to better control low-energy hadronic effects, which, thanks to the growing potential of supercomputing and advances in non-perturbative techniques, can now be achieved by the most modern numerical simulations of lattice QCD, including the effects of long-range electromagnetic interaction. After a review of the state of the art in the field for the accurate extraction of the elements of the CKM matrix, in this seminar I will illustrate some new lattice results, using domain wall chiral fermions, on the form factors contributing to the amplitudes of radiative leptonic decays of light and heavy mesons, $H \to \ell \nu_\ell \gamma$, including multiple virtualities of the emitted photon for the study of rare four-lepton decays, such as $H \to \ell^{\prime +} \ell^{\prime -} \ell \nu_\ell$ or $H \to \ell^{\prime +} \ell^{\prime -} \ell^+ \ell^-$. In addition, I will present some recent efforts and the new program of the BMW collaboration in the study of the unitarity of the first row of the CKM matrix. This activity is part of the Theoretical Phenomenology Visiting Institute@LNF, running from 23 March to 27 March 2026, and supported by CSN4 to promote the participation of early-career scientists.

This workshop aims to bring together theorists and experimentalists working on various aspects of kaon decays, with a focus on fostering interdisciplinary collaboration and advancing precision studies in flavor physics. Topics will include radiative kaon decays, rare processes, multi-lepton final states, and future prospects in K​ measurements. Special attention will be given to novel lattice QCD approaches and their phenomenological implications. The program will feature a hands-on session on Monte Carlo generators and radiative corrections, aimed at clarifying current methodologies and enhancing analysis tools. Contributions from major experimental collaborations—including NA62, KLOE/KLOE-2, E36, and LHCb—will be complemented by theoretical insights from lattice groups such as BMW, ETMC, RBC, and UKQCD. This activity is part of the Theoretical Phenomenology Visiting Institute @ LNF, running from 23 March to 27 March 2026, and supported by CSN4 to promote the participation of early-career scientists across three scientific events. The Theoretical Phenomenology Visiting Institute @ LNF initiative is chaired by Federico Mescia. The workshop will take place in the Salvini Auditorium (Building 36, access via the LNF secondary entrance at Via E. Fermi, 60 – see map). (Talks by invitation only)

The recent result published by the PADME Collaboration at LNF, has strengthened the interest in the searches for the hypothetical X17 particle, whose existence has been firstly suggested by nuclear physics experiments performed at ATOMKI. The aim of the Workshop is to provide a comprehensive review of the current experimental activities, and of the possible future developments in this field. Emphasis will be given to searches at particle’s accelerators.  

(Advanced LinEar collider study GROup) Workshop

Speaker: Cristina Lazzeroni (University of Birmingham) The main aim of the proposed KOTO II experiment at JPARC is the measurement of the ultra-rare decay KL to pi0 nu nu. This decay is heavily suppressed and its branching is very well predicted by the SM (3x 10-11 with about 2% uncertainty), thereby exhibiting an exceptional sensitivity to new physics. The design includes a new beamline with a 5-degree extraction angle, and a new detector with a 12-meter-long signal decay region and a 3-meter diameter calorimeter. A discovery of the KL to pi0 nu nu decay with 5σ significance is achievable for the SM value of the branching ratio. The design, expected performance, and current status of the KOTO II experiment will be presented.

Speaker: Alfredo Stanzione (La Sapienza Univ., Roma) An interesting feature of a cosmological phase transition can be a stage of exponential expansion (supercooling). The modified expansion history and the entropy injection at reheating, can affect the final energy fraction of dark matter. In this paper, we revisit the calculation of the freeze-out and freeze-in dynamics, showing additional effects on top of the standard dilution factor if the dark matter production is completed during the supercooling stage. We show for the first time how these effects can be particularly interesting for direct detection, as the parameter space for WIMP-like candidates shifts from excluded to allowed regions, and freeze-in candidates get closer to experimental reach. A phenomenological motivation to consider supercooling is the associated gravitational wave background. The implications of a finite-duration reheating stage, when the equation of state is close to matter-domination, are a peculiar low-frequency spectrum, and its shift to lower frequencies. These effects are a complementary test of the dynamics that we study for dark matter production, and remarkably can link direct detection of dark matter and gravitational wave astronomy.