Liste des Contributions

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  1. Dr Sami Caroff (LAPP)
    04/02/2026 09:00
  2. Giulia Gubitosi (University of Napoli Federico II and INFN)
    04/02/2026 09:10
  3. Tomislav Terzić (University of Rijeka, Faculty of Physics)
    04/02/2026 09:40
  4. 04/02/2026 10:10
  5. Cyann PLARD (LPNHE - CNRS), Cyann Plard (LAPP)
    04/02/2026 11:00

    One way of detecting or constraining Lorentz invariance violation (LIV) effects is by measuring time delays in the arrival of very high-energy (VHE) photons from astrophysical sources. Suitable targets are variable, distant and highly energetic objects such as pulsars, gamma-ray bursts (GRBs), and active galactic nuclei (AGN) flares. However, a major challenge arises from intrinsic time lags...

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  6. Jelena Strišković
    04/02/2026 11:30

    Robust tests of Lorentz invariance violation (LIV) require the combination of multiple datasets to disentangle intrinsic source effects from propagation-induced lags. In this talk, I present results and methods published in my PhD thesis, based on a joint LIV time-of-flight analysis of two BL Lacertae very-high-energy flares observed by imaging atmospheric Cherenkov telescopes: MAGIC (19–20...

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  7. 04/02/2026 12:00
  8. Filip Reščić (University of Rijeka)
    04/02/2026 14:00

    In this talk I will discuss the general phenomenological features of Lorentz Invariance Violation (LIV) and Doubly Special Relativity (DSR) frameworks. Particular attention will be given to anomalies in the flux of very-high-energy (VHE) and ultra-high-energy (UHE) gamma rays from astrophysical sources, arising from modifications of interaction thresholds induced in LIV and DSR scenarios. Such...

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  9. Alberto Rosales De Leon (Observatoire de Paris)
    04/02/2026 14:30

    Lorentz Invariance Violation (LIV) effects are predicted in some theories of Quantum Gravity (QG) and would manifest as energy-dependent modifications to particle kinematics. Such effects can alter the threshold of the electron–positron pair production process, leading to observable deviations in the absorption of very-high-energy photons by the Extragalactic Background Light (EBL). We exploit...

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  10. 04/02/2026 15:00
  11. Lara Nava (INAF)
    04/02/2026 16:00

    Gamma-ray bursts (GRB) are cosmoligocal sources with average redshift around 2, emitting radiation over the entire electromagnetic spectrum. Two different sites are responsible for the radiated emission: one internal to the relativistic jet (responsible for the prompt, higly-variable soft gamma-ray radiation detected over timescales of ms to tens of seconds) and one external, originated from...

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  12. Prof. Frédéric DAIGNE (Institut d'Astrophysique de Paris - Sorbonne Université)
    04/02/2026 16:30
  13. 04/02/2026 17:00
  14. Andreas Zech (LUTH - Observatoire de Paris)
    05/02/2026 09:00

    When using the light curves of rapid blazar flares for searches of propagation effects, it is important to understand the
    intrinsic temporal and spectral signatures introduced by the underlying particle acceleration and emission processes
    producing those flares. Unfortunately, the nature of these processes is not well known. Most scenarios place the emission
    region inside the relativistic...

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  15. Xavier Rodrigues (APC)
    05/02/2026 09:30

    The IceCube South Pole Observatory detects cosmic neutrinos up to a few PeV, and the KM3NeT experiment in the Mediterranean Sea has recently detected the first event above 100 PeV, inaugurating the era of ultra-high-energy neutrino astronomy. Active black holes, in particular blazar jets, are among the most promising candidate sources. In this talk, I summarize recent developments in...

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  16. 05/02/2026 10:00
  17. Guillaume Grolleron
    05/02/2026 11:00
  18. David Sanchez (LAPP/IN2P3)
    05/02/2026 11:30
  19. 05/02/2026 12:00
  20. Mauricio Bustamante Ramirez (Niels Bohr Institute, University of Copenhagen)
    05/02/2026 14:00

    High-energy cosmic neutrinos probe fundamental physics at scales of energy and distance otherwise unreachable, where new physics may manifest. Since the discovery of TeV-PeV cosmic neutrinos in 2013, we have explored this progressively more broadly and more precisely, thanks to a growing number of detected neutrinos and improvements in reconstruction and analysis techniques. Quantum gravity...

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  21. DENISE BONCIOLI (University of L'Aquila and INFN-LNGS)
    05/02/2026 14:30

    Searching for new phenomena predicted by quantum-gravity (QG) effects in high-energy astrophysics implies to be able to distinguish the signatures related to standard physics in sources and propagation from the ones coming from pure QG. In this contribution I will focus on the interpretation of ultra-high-energy cosmic ray (UHECR) data in terms of astrophysical scenarios for the fluxes of...

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  22. 05/02/2026 15:00
  23. Narek Sahakyan (ICRANet-Armenia)
    05/02/2026 16:00

    Multiwavelength and multimessenger observations, combining data across the electromagnetic spectrum with high-energy neutrinos, provide a uniquely powerful probe of the physical processes at work in the relativistic jets of blazars. Recent campaigns and coincident neutrino detections have reinforced the role of blazars as prime laboratories for studying particle acceleration and radiation in...

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  24. Rafael Alves Batista, Rafael Alves Batista (Sorbonne Université, Institut d'Astrophysique de Paris)
    05/02/2026 16:30

    What if there are already signatures of quantum gravity (QG) in the existing high-energy multi-messenger data -- would we be able to know that?
    In this talk, I discuss the complexities inherent in separating new physics from conventional astrophysical processes. Disentangling these two signals is not merely a technical challenge; it is an epistemic one. I argue that we are currently limited...

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  25. 05/02/2026 17:00
  26. HELENE SOL (LUTH)
    06/02/2026 09:00
  27. Dr Sami Caroff (LAPP)
    06/02/2026 09:15
  28. Dr Julien Bolmont (LPNHE - SU/CNRS-IN2P3)
    06/02/2026 10:00