Présidents de session
Astroparticle
- Sami Caroff (LAPP)
Astroparticle
- Sami Caroff (LAPP)
Astroparticle
- Sami Caroff (LAPP)
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Dr Sami Caroff (LAPP)26/10/2023 14:00
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Vijay Dabhi (CPPM, Marseille)26/10/2023 14:30Astroparticle
Dark matter is one of the major puzzles in fundamental physics. Axions are among the best-motivated dark matter candidates. MADMAX experiment will search for axions in the mass range around 100 $\mu$eV, which is favored by theory. Traditional axion cavity experiments are unable to access this mass range. Therefore, a novel detector called dielectric haloscope will be utilised for this...
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M. Guillaume Grolleron (LPNHE (CNRS))26/10/2023 15:00Astroparticle
Active Galactic Nuclei (AGN) stand as enigmatic cosmic powerhouses, harboring supermassive black holes at their centers. Blazars are AGN with a jet oriented toward the observer. Their emission spans from radio to very high-energy gamma rays. Understanding their spectral variability provides crucial insights into the underlying physics governing these astrophysical phenomena. The Cherenkov...
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Cyann Plard (LAPP IN2P3 CNRS)26/10/2023 15:30Astroparticle
The flares of active galactic nuclei (AGNs) can be used to detect or constrain Lorentz invariance violation (LIV) by measuring time lags in detection of high energetic photons. An important source of uncertainty is our lack of knowledge of source intrinsic processes. However, combining flares and sources allows us to increase the precision of these measurements as well as to limit the noise of...
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Cervane GRIMAUD (LAPP)26/10/2023 16:30Astroparticle
Virgo is a gravitational wave detector located near Pisa in Italy. It is composed of a Fabry-Perot Michelson Interferometer and allows to detect gravitational wave passing through it using the interference dark fringe signal going out of the interferometer.
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Virgo is an instrument that needs to be controlled and calibrated with great accuracy in order to achieve the precision required to... -
Thibault NGUYEN TRUNG (IJCLab)26/10/2023 17:00Astroparticle
The interstellar medium is made up of gas and dust. This medium is traversed by cosmic radiation and irradiated by stellar UV, except in dense clouds where UV is absent. The interaction of these rays with the dust and gas is crucial to the chemical evolution of interstellar and circumstellar environments. Heavy and slow cosmic rays interact with very small dust particles (-100 atoms) and...
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Mlle Yongyu PAN26/10/2023 17:30Astroparticle
The mysterious nature of Dark Matter (DM) has puzzled physicists the world over. One well-motivated class of DM candidates is Weakly Interacting Massive Particles (WIMPs). The XENON Dark Matter Project for direct search for WIMPs currently operates XENONnT experiment, lying a dual-phase (liquid & gas) xenon time projection chamber (TPC), situated in the underground LNGS in Italy.
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This... -
Marie-Sophie Carrasco (Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France)27/10/2023 10:00Astroparticle
The quest for PeVatrons, sources of cosmic rays accelerated up to PeV energies, saw an exciting development in 2021 when LHAASO detected 12 ultra-high energy (UHE) gamma-ray Galactic sources. Among those sources, the supernova remnant G106.3+2.7 (also called the Boomerang SNR) is a promising candidate to both hadronic and leptonic scenarios for the UHE emissions.
Gamma-ray astronomy...
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Marie-Sophie Carrasco (Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France)
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Vijay Dabhi (CPPM, Marseille)
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Guillaume Grolleron
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Thibault NGUYEN TRUNG (IJCLab)
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Yongyu PAN
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Cyann Plard (LAPP IN2P3 CNRS)
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Lucas Gréaux (IJCLab)