Prochains séminaires


18 mai 2026
Visualisation framework
Nico SCHUSTER
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Description :
Abstract: ...
Début :
lundi 18 mai 2026, 14:00:00 heure d’été d’Europe centrale
Fin :
lundi 18 mai 2026, 16:00:00 heure d’été d’Europe centrale
1 juin 2026
Pokemon Standard Model (TBC)
Camille Sironneau (APC lab)
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Début :
lundi 1 juin 2026, 14:00:00 heure d’été d’Europe centrale
Fin :
lundi 1 juin 2026, 16:00:00 heure d’été d’Europe centrale
15 juin 2026
Journalistes et scientifiques, pourquoi tant de haine ?
Pauline Amiel (amU)
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Description :

Les experts du "vrai" menacés dans un contexte de guerre informationnelle et de post-vérité.

Résumé : Nous dresserons dans un premier temps l'état des menaces et attaques semblables contre la liberté d'informer et la liberté académique, dans un contexte international de désinformation massive, d'IA, d'accaparement des ressources, de "post-vérité" etc. Les journalistes, pourtant piliers de la démocratie en tant que "4e pouvoir", sont menacés. En parallèle, le rôle social des chercheurs, eux-aussi acteurs centraux de notre espace public démocratique, est remis en cause. Et pourtant, ces deux professions que tout rassemble ont bien du mal à se parler...Dans un deuxième temps, nous explorerons toutes les causes de l'incompréhension entre scientifiques et journalistes, qui pourtant partagent tant de points communs. Différences de publics, de méthodes, de temporalités et de discours, ces deux professions qui ont pour objectif de produire "le vrai", renforcer le savoir et la connaissance, ont pourtant bien des difficultés à communiquer.

 

Pauline Amiel est maitresse de conférences en information-communication, spécialiste du journalisme et des médias, à l'EJCAM (école de journalisme et de communication de l'université d'Aix Marseille), qu'elle dirige depuis 2022. Également vice-présidente communication d'amU, elle participe à la stratégie de rayonnement de cette université.

Début :
lundi 15 juin 2026, 14:00:00 heure d’été d’Europe centrale
Fin :
lundi 15 juin 2026, 16:00:00 heure d’été d’Europe centrale
24 juin 2026
Quantum entanglement in High Energy Physics
Fabio Maltoni (Università di Bologna)
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Début :
mercredi 24 juin 2026, 14:00:00 heure d’été d’Europe centrale
Fin :
mercredi 24 juin 2026, 16:00:00 heure d’été d’Europe centrale

5 derniers séminaires


24 avr. 2026
The Future Circular Collider project: a long-term vision for particle physics (with a focus on flavour physics)
Stephane Monteil (Laboratoire de Physique de Clermont - UCA/IN2P3)
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Description :
Abstract: this seminar will introduce the Future Circular Colliders project, highlight some results of the Feasibility Study and discuss the next steps towards approval. The FCC project features a 90 km long tunnel in the Geneva basin where an electron-positron collider crossing four relevant electroweak thresholds (Z, WW, HZ and tt) shall be installed first. A longer term energy frontier proton collider, defining the infrastructures, is envisaged to be hosted in the very same
tunnel. The exquisite luminosity of the electron circular machine at each energy can challenge the electroweak observables precision consistency test and offer, in particular at the Z pole but not only there, a continuation of the exploration of the Flavour Physics case beyond the vibrant LHCb and Belle II programmes. We’ll review these Physics opportunities introducing the newly established Flavoured Circular Collider Workshop and discuss some of the related detector requirements and detector R&D.
Début :
vendredi 24 avril 2026, 14:00:00 heure d’été d’Europe centrale
Fin :
vendredi 24 avril 2026, 16:00:00 heure d’été d’Europe centrale
20 avr. 2026
Vers la détection de l'invisible : la matière sombre
Marie-Cécile Piro (University of Alberta)
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Description :
Résumé :
Malgré les avancées remarquables dans les domaines de la science, de la physique et de l’astronomie, nous ne comprenons toujours pas près de 85 % de la masse de l’Univers. Les observations astronomiques et cosmologiques suggèrent l’existence d’une matière invisible, différente de celle que nous connaissons et qui serait cinq fois plus abondante « la matière sombre ». Pourtant, à ce jour, elle demeure indétectable par nos instruments actuels sur Terre, ce qui en fait l’un des plus grands mystères non résolus de la cosmologie moderne. Ce mystère est au cœur de nombreuses recherches à travers le monde, car la matière sombre est considérée comme un élément clé pour expliquer la formation de l’Univers et pourrait révéler une nouvelle physique, au-delà du modèle standard. Après avoir exposé l’importance de la matière sombre et les preuves de son existence, je présenterai diverses technologies actuelles utilisées pour la détecter, les défis auxquels nous sommes confrontés, ainsi que les innovations nécessaires pour percer enfin ce mystère.
 
Biographie :
Marie-Cécile Piro est professeure agrégée en physique à l’Université de l’Alberta et professeure auxiliaire au Département des sciences de la Terre et de l’atmosphère à l’Université Dalhousie. Elle a obtenu son doctorat en physique expérimentale des particules à l’Université de Montréal, dans le cadre du projet PICASSO installé au laboratoire souterrain de SNOLAB au Canada, où elle a étudié la détection de la matière sombre à l’aide de chambre à bulles. Elle a ensuite mené des recherches postdoctorales en France sur les bolomètres au germanium de l’expérience EDELWEISS au Laboratoire Souterrain de Modane, puis a travaillé aux États-Unis et en Italie en tant que chercheuse associée au sein de la collaboration XENON1T au Laboratoire National du Gran Sasso. Lauréate en 2024 de la bourse nationale Dorothy Killam pour ses avancées sur la détection de la matière sombre, elle contribue également à des projets de paléo-topométrie et d’imagerie muonique appliqués aux sciences de la Terre.
Début :
lundi 20 avril 2026, 14:00:00 heure d’été d’Europe centrale
Fin :
lundi 20 avril 2026, 16:00:00 heure d’été d’Europe centrale
26 janv. 2026
Testing general relativity with cosmic density and velocity fields: first results with the DESI Peculiar Velocity Survey
Julian Bautista (CPPM, Aix-Marseille Université, CNRS/IN2P3)
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Description :
Abstract: In this talk, I will first introduce how to measure dark energy in cosmology, then focus on galaxy surveys. Galaxy surveys provide us with maps of the cosmic density field. The statistical properties of the density field are tightly connected to the cosmological evolution and the amounts of dark energy, dark matter, etc. I will also show how it is possible to measure the radial peculiar velocities of galaxies in the nearby Universe, increasing the precision on cosmological constraints relative to density-only constraints. The DESI Peculiar Velocity survey released its first measurements in Dec 2025. I will highlight some key aspects of this analysis that make it robust. Finally, I will give some highlights on similar work being developed in CPPM with supernova surveys such as ZTF and LSST. 
Début :
lundi 26 janvier 2026, 14:00:00 heure normale d’Europe centrale
Fin :
lundi 26 janvier 2026, 16:00:00 heure normale d’Europe centrale
8 déc. 2025
3rd year PhD students - Part III
Leonardo Splendori (CPPM, Aix-Marseille Université, CNRS/IN2P3)
Christian Mavungu Tsava (CNRS)
Melissa LEROY (Centre de Physique des Particules de Marseille)
Francesco Magnani (cppm)
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Description :

Speaker 1: Leonardo Splendori

Title: Developments in b-tagging for the ATLAS upgrade and their impact on di-Higgs sensitivity

Abstract: The upcoming High Luminosity LHC (HL-LHC) era is expected to bring opportunities for studies involving rare processes, including di-Higgs production. Flavour tagging is going to play a crucial role in the analysis of such processes. This talk will explore the challenges we expect to encounter for flavour tagging in the HL-LHC era, with its higher luminosity, increased pile-up and upgraded ATLAS detector. The focus will be on the expected behaviour of current flavour tagging neural networks (GN2) when trained and evaluated on simulated Run 4 samples. To determine its performance and robustness against the harsher conditions associated with higher pileup. From this we will be able to compare the same model between Run 3 and Run 4 and produce predictions on the impact this new environment will have on di-Higgs analyses.

Speaker 2: Mélissa Leroy

Title: A Comprehensive Simulation Framework for Cadmium Telluride Hybrid Pixels
 
Abstract: Understanding and predicting the behavior of CdTe-based X-ray detectors is essential for optimizing and designing the next generation of high-performance imaging systems. However, the simulation of hybrid pixel sensors remains a challenge due to physical phenomena occurring during their operation. In the context of a CIFRE thesis carried out in partnership with Detection Technology, a manufacturer of X-ray detection systems for security, medical, and industrial applications, I will present a comprehensive simulation framework for X-ray hybrid pixels.The simulator reproduces interactions between X-rays and the sensor are modeled using Geant4-based Monte Carlo simulations, while charge drift, repulsion, and diffusion are described with an analytical approach derived from the charge continuity equation. The simulated spectra are validated against experimental data acquired with the XPAD3.2-S/CdTe hybrid pixel detector under synchrotron irradiation. The results show good agreement with measurements, demonstrating the relevance of this framework to reproduce complex physical effects such as fluorescence escape and charge sharing that strongly impact detector performance.

Speaker 3: Christian Tsava

Title: Search of Higgs Boson Pair Production in the bbττ Final State using b-jet triggers with the ATLAS Detector at the LHC

Abstract: This work summarizes the use of the b-jet trigger in the ATLAS search for non-resonant Higgs boson pair production in the bbττ final state using Run 2 and partial Run 3 data, with the aim of measuring the Higgs potential via the Higgs self-coupling. The event selection targets events with one or two hadronically decaying τ leptons. The objective is to study the impact of adding and calibrating the b-jet trigger in the analysis. This work provides a detailed overview of all the necessary steps for the inclusion and calibration required for the bbττ analysis.

Speaker 4: Francesco Magnani

Title: Multi-messenger astronomy with KM3NeT and COLIBRÍ
 
Abstract: Multi-messenger astronomy combines signals from different cosmic messengers emitted by the same astrophysical source. Neutrinos, in particular, travel unimpeded from their production site and can directly trace hadronic processes in extreme environments where electromagnetic observations are often challenging. This makes them ideal probes for systems where particle acceleration is still poorly understood, such as microquasars—compact binaries in which a compact object accretes matter from a companion star and can launch powerful relativistic jets, recently confirmed as high-energy emitters.
Part of this thesis focuses on the search for neutrino emission from microquasars using KM3NeT, the neutrino telescope under construction in the Mediterranean Sea, which spans energies from a few GeV to several hundred PeV thanks to its ORCA and ARCA detectors. In parallel, we are initiating an optical monitoring campaign with COLIBRÍ, a robotic 1.3-m telescope in San Pedro Mártir (Mexico). Optical data are expected to be crucial, as microquasar outbursts often show precursors in the optical band days before the X-ray flare. Combining both datasets will enable us to track the full evolution of an outburst and correlate the different emission channels to investigate its origin.
Début :
lundi 8 décembre 2025, 14:00:00 heure normale d’Europe centrale
Fin :
lundi 8 décembre 2025, 16:00:00 heure normale d’Europe centrale
24 nov. 2025
3rd year PhD students - Part II
Diane Joly (Aix-Marseille Université, CPPM)
Isaac Consigny (CPPM)
Grigorii TOLKACHEV (CPPM, Aix-Marseille Université, CNRS/IN2P3 (FR))
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Description :

Speaker 1 : Grigorii TOLKACHEV

Title: Search for doubly resonant beyond the Standard Model process with one Higgs boson and one scalar resonance in the final state in the $b\bar{b}\gamma\gamma$ channel in the ATLAS experiment at the LHC.

Abstract: Although the Standard Model (SM) provides an exceptionally accurate description of a wide range of experimental observations, it is nevertheless an incomplete theory. Many theories go beyond the SM (BSM), introducing additional particles and interactions to address its incompleteness. Some BSM models predict the existence of new scalar particles in the Higgs sector, denoted as X and S, which could be produced in proton-proton collisions in association with a Higgs boson: $ pp \rightarrow X \rightarrow SH$. Searches for such particles have been conducted by several analysis teams within the ATLAS and CMS experiments. Notably, one analysis reported a local (global) excess of 3.5$\sigma$ (2.0$\sigma$) for $m_X = 575$ GeV and $m_S = 200$ GeV compared to the background-only hypothesis in the decay channel $X \rightarrow SH \rightarrow b\bar{b}\gamma\gamma$, using 140 fb$^{-1}$ of ATLAS Run 2 data at $\sqrt{s} = 13$ TeV. While this excess is below the discovery threshold of $5\sigma$, it may suggest a possible deviation from Standard Model predictions. This talk will present an update of this search using ATLAS Run 2 data at $\sqrt{s} = 13$ TeV and part of Run 3 data at $\sqrt{s} = 13.6$ TeV (2022-2023). The new search follows a similar strategy to the Run 2 analysis, with several improvements.

 

Speaker 2: Diane JOLY

Title: Measuring neutrino oscillations with KM3NeT/ORCA

Abstract: KM3NeT is a next-generation neutrino observatory being constructed in the Mediterranean Sea. It consists of two main detector configurations: ORCA, optimized for low-energy (GeV) neutrinos and mass-hierarchy studies, and ARCA, designed for high-energy (TeV) cosmic neutrinos for astrophysical purposes. Currently, the ORCA detector has 33 detection lines deployed, with 18 optical modules on each line, with plans to eventually reach a full configuration of 115 lines. In the first physics analyses performed with the partially completed ORCA, the results are already competitive with current measurements, demonstrating strong sensitivity to neutrino oscillation parameters. However, these measurements remain limited by several sources of systematic uncertainty, particularly in modeling the detector response. The objective of my PhD thesis is to improve the estimation of these systematic uncertainties, taking into account the quantum efficiency of the optical modules, and the water absorption length. By developing more accurate models of the detector response, I aim to reduce the dominant systematic errors and enhance the precision of future ORCA analyses.

 

Speaker 3: Isaac-Paul CONSIGNY

Title: Search for lepton flavor violating decay B0 → ρ0τ ℓ at Belle II

Abstract: Lepton flavour conservation is an accidental symmetry of the Standard Model (SM).  
However, the discovery of neutrino oscillations has already demonstrated that this symmetry is not exact,
implying that lepton flavour can be violated in nature.
Many extensions of the SM naturally predict additional sources of lepton flavour violation (LFV) with enhanced branching fractions for processes involving the third generation of leptons, making searches for such effects an important probe for new physics. Searches for related processes such as b → sτ ℓ had been extensively studied at Belle II but b → dτ ℓ remains uncovered. This work presents the first investigation of lepton flavour violation in B → ρ0τ ℓ decay modes, using the combined datasets of Belle and Belle II experiments.

Début :
lundi 24 novembre 2025, 14:00:00 heure normale d’Europe centrale
Fin :
lundi 24 novembre 2025, 16:00:00 heure normale d’Europe centrale