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Tag Archives: Evento scientifico

Isolated photons measurements with the ALICE electromagnetic calorimeter at the LHC Run1 and 2

Speaker: Gustavo Conesa Balbastre (LPSC-CNRS Grenoble) The ALICE experiment at the LHC is devoted to test QCD predictions, and in particular, the measurement of the properties of the Quark-Gluon plasma created in ultra-relativistic heavy-ion collisions. Among the different probes that the experiment explores, neutral mesons and isolated photons are useful to study the jet-quenching effect in the QGP: the loss of energy of high energy partons (quarks and gluons) produced at the initial stages of the collision traversing the strongly interacting plasma. Such probes are measured in ALICE by its electromagnetic calorimeters PHOS and EMCal, combined with the central tracking systems. The Frascati-LNF-INFN and Grenoble-LPSC-CNRS groups had a strong involvement in the construction and exploitation of the EMCal calorimeter where I was involved. In this presentation I will present the different results obtained with the calorimeter during the LHC Run 1 and 2 data, concentrating on the isolated photons production.

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Plasma Wakefield Acceleration – the long and winding road from proof-of-principle experiments to colliders

Speaker: Livio Verra (Istituto Nazionale di Fisica Nucleare) The extremely large accelerating fields that can be excited in plasmas are orders of magnitudes larger than in conventional accelerators, and they could be used to miniaturise the ever-increasing footprint of light sources and high-energy physics facilities. In this seminar I will review the concepts of plasma wakefield acceleration, present the main experimental results of the field, and discuss the challenges on the path towards applications for high-energy physics.

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Hadronisation corrections with ARES

Speaker: Andrea Banfi (University of Sussex) Jet observables such as event-shape distributions and jet rates are widely used for precision determinations of the strong coupling. The accuracy of perturbative calculations for such observables is very high, and poorly known hadronisation corrections limit the precision of such determination. I present a general method, based on the existing theoretical framework ARES (Automated Resummer for Event Shapes), to estimate hadronisation corrections up to a single universal non-perturbative parameter, which can be determined from data. The method can be applied to an arbitrary observable and gives promise to impact future determinations of the strong coupling with jet observables.    

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Learning with uncertainty for computer vision

Speaker: Fabio Galasso (Roma La Sapienza Univ.) Representation learning is an important part of modern computer vision. Literature assumes a default Euclidean space, thus a manifold based on regular grids. Only most recently, hyperbolic spaces have enabled techniques to reach and surpass the state-of-the-art, supporting learning with hierarchical structures and uncertainty, also a by-product of hyperbolic representation learning. I will introduce our most recent work that leverages Hyperbolic Neural Networks for anomaly detection, self-supervised learning of actions, active learning of semantic segmentation, and reinforcement learning of robot navigation in social environments.

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Flavor physics: open problems and recent developments

Speaker: Gino Isidori (UZH) What is the origin of the different masses for quarks and leptons is one of the big open questions in particle physics. I will briefly review this problem, illustrating its central role in achieving a deeper understanding of fundamental interactions. I will also outline some recent theoretical ideas on how to address it, focusing in particular on the concept of “flavor deconstruction”, and finally discuss how these ideas can be tested through current and future flavor-physics experiments.

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PADME results on X17 from Run-III data

Speaker: Tommaso Spadaro (Istituto Nazionale di Fisica Nucleare) The PADME experiment at the Frascati National Laboratory of INFN has performed a search for the hypothetical X17 particle, by observing the product of the collisions of the positron beam from the DAΦNE LINAC on a diamond fixed target. The beam energy has been varied in the range 265–300 MeV, corresponding to values of √s between 16.4 and 17.5 MeV, completely covering the center of mass region identified by the ATOMKI collaboration as significant for observing the postulated X17 particle. In my talk I will present the result of the analysis of these data, and briefly discuss the physics potential of the forthcoming PADME run, with an improved detector.

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Hunting axion dark matter with anti-ferromagnets: a case study with nickel oxide

Speaker: Pier Giuseppe Catinari (Istituto Nazionale di Fisica Nucleare) In this talk, I will explore how effective field theories (EFTs) provide a powerful framework for describing interactions—particularly non-linear couplings—between dark matter particles and the collective excitations of target materials. I will focus specifically on the interaction between axion dark matter and magnons, which are quasiparticles arising from spin-wave excitations in antiferromagnetic materials. Materials such as nickel oxide emerge as optimal candidates for detecting sub-MeV dark matter with spin-dependent interactions, as well as for the absorption of meV-scale QCD axions.  

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Sudakov resummation of thrust distribution in electron-positron annihilation

Speaker: Giancarlo Ferrera (Istituto Nazionale di Fisica Nucleare) We present a resummed QCD calculation of the thrust distribution in electron-positron annihilation in the back-to-back region up to N^4LL accuracy, matched to fixed-order results up to NNLO. We perform the resummation of the large Sudakov logarithms in the Laplace-conjugated space, and we show that the results differ significantly from those obtained through resummation in thrust space. We include non-perturbative corrections using an analytic hadronization model that depends on two free parameters. Finally, we present a comparison of our predictions with experimental data at the Z-boson peak, and we extract a value for the QCD coupling that is fully consistent with the world average.

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Determination of the charged kaon mass by laser spectroscopy of kaonic helium atoms at DAPHNE

Speaker: Masaki Hori (Imperial College London) We propose the first laser spectroscopy of an atom containing a kaon at DAPHNE, which may eventually allow the precision on the charged kaon mass to be improved by 2 to 3 orders of magnitude compared to now, and establish upper limits on beyond-the-standard model forces that may arise between kaons and the other constituent particles of the atom. Metastable kaonic helium is a three-body atom consisting of a helium nucleus, an electron, and kaon occupying a Rydberg state. The atom has an anomalously long lifetime of 10 ns which makes it amenable to laser spectroscopy. Quantum electrodynamics calculations for these atoms currently achieve parts-per-billion scale precision. We have carried out similar experiments at the Antiproton Decelerator of CERN for many years and determined the antiproton-to-electron mass ratio to a precision of 8 parts in 10^10; laser spectroscopy of pionic helium atoms which have a lifetime of 7 ns was also recently achieved at the 590 MeV/c ring cyclotron facility of Paul Scherrer Institute. This increases our confidence that laser spectroscopy of the kaonic variety is now possible, utilizing the modern advances in laser technology. The experiment critically relies on the low-energy kaons of small energy spread which are only available at DAPHNE. Some of the technical challenges of achieving this goal in DAPHNE will be described.  

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Searching for Axion Dark Matter with Radio Telescopes

Speaker: Prof. Luca Visinelli (Shanghai Jiao Tong University) The QCD axion, originally proposed to resolve the strong CP problem, is also a compelling dark matter (DM) candidate. In strong magnetic fields, such as those surrounding neutron stars, axions can convert into photons, potentially generating detectable radio signals. This axion-photon coupling offers a unique avenue for experimental searches in a well-defined mass range. In this seminar, I will present an observational study using the Green Bank Telescope (GBT) to search for transient radio signals from axion-photon conversion. Focusing on the core of Andromeda, we employ the VErsatile GBT Astronomical Spectrometer (VEGAS) and the X-band receiver (8–10 GHz) to probe axions with masses between 33 and 42 μeV, achieving a mass resolution of 3.8 × 10^-4 μeV. We describe our observational strategy and analysis techniques, which reach an instrumental sensitivity of 2 mJy per spectral channel. While no candidate signals exceeding the 5σ threshold were detected, I will discuss future improvements, including expanding the search to additional frequency bands and refining theoretical models, to strengthen constraints on axion DM scenarios.

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