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Journées de Rencontre des Jeunes Chercheurs 2019

24–30 nov. 2019
Centre Moulin Mer
Fuseau horaire Europe/Paris

Secrétariat

Session

Theoretical Physics

25 nov. 2019, 16:00
Centre Moulin Mer

Centre Moulin Mer

Route du centre nautique, 29460 Logonna-Daoulas www.moulin-mer.fr/ https://goo.gl/maps/zfearb173UxabXPFA (English) The centre is located at about 30 minutes drive from Brest. We will provide transport from Brest airport and train station to the centre Moulin Mer. The shuttle will leave the airport at 18h30 and the station at 19h on the 24th November and arrive at the airport at 8h and the station at 8h30 on the 30th November. (Français) Le centre est situé pas loin de la ville de Brest. Il y aura une navette entre l'aéroport/la gare et le centre Moulin Mer. La navette partira de l'aéroport à 18h30 et de la gare à 19h le 24 novembre et arrivera à l'aéroport à 8h et à la gare vers 8h30 le 30 novembre.

Présidents de session

Theoretical Physics: Session I

  • ANDREAS GOUDELIS (LPC - Clermont Ferrand)

Documents de présentation

Aucun document.

  1. 147. Introduction
    Andreas Goudelis (LPC - Clermont Ferrand)
    25/11/2019 16:00
  2. 148. Hadronic vacuum polarization contribution to the muon magnetic anomaly from lattice QCD
    Letizia Parato (Aix-Marseille Université)
    25/11/2019 16:30

    Anomalous magnetic moments have guided the evolution of quantum field theory ever since its earliest stages, serving both as a stringent test of the theory at increasingly higher levels of precision and as a possible window to new physics. After decades of perfect agreement, the measured muon magnetic moment (which is known to a precision of about 0.5 parts per million both from theory and...

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  3. 118. Recasting Direct Detection Limits Within MicrOMEGAs And Implication For Non-Standard Dark Matter Scenarios
    Ali Mjallal (LAPTh)
    25/11/2019 17:00

    Direct detection experiments present 90% exclusion cross-sections for point-like spin-independent Dark Matter interaction with nucleons for fixed cosmological parameters. In this presentation, we discuss a possibility to extend obtained results of such experiments on model with arbitrary cosmological parameters, different form factors of spin-dependent interaction, interactions via light...

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  4. 130. Dark matter searches towards WLM dwarf irregular galaxy with H.E.S.S.
    Celine Armand (LAPP & LAPTh)
    25/11/2019 17:30

    In the indirect dark matter (DM) detection framework, the DM particles would produce some signals by self-annihilating and creating standard model products such as $\gamma$ rays, which might be detected by ground-based telescopes.
    Dwarf irregular galaxies represent promising targets for the search for DM as they are assumed to be dark matter dominated.
    In 2018, the H.E.S.S. telescopes...

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  5. 146. Introduction
    Andreas Goudelis (LPC - Clermont Ferrand)
Ordre du jour en construction...