S'authentifier

IRN Terascale@Bruxelles

16–18 oct. 2019
Brussels
Fuseau horaire Europe/Paris

Session

Dark Universe

18 oct. 2019, 09:00
Salle Solvay (Brussels)

Salle Solvay

Brussels

Université Libre de Bruxelles Boulevard du Triomphe (Campus de la Plaine) 1050 Bruxelles Belgium

Documents de présentation

Aucun document.

  1. 45. DM-dark radiation, Lyman-alpha, and H0
    Deanna Hooper (RWTH Aachen, TTK)
    18/10/2019 09:00
  2. 44. Spontaneous Freeze-Out from Thermal Phase Transition of Heavy Dark-Matter
    Lucien Heurtier (University of Arizona)
    18/10/2019 09:23
  3. 47. Sub-GeV DM with Ge detectors
    Quentin ARNAUD (Institut de Physique Nucléaire de Lyon)
    18/10/2019 09:46
  4. 48. Recasting direct detection limits within micrOMEGAs and implication for non-standard Dark Matter scenarios
    Ali Mjallal (LAPTh)
    18/10/2019 10:09
  5. 46. Energy spectra for GeV and sub-GeV Dark Matter
    Peter Reimitz (Heidelberg University)
    18/10/2019 10:32
  6. 51. Combined search for dark matter from the Galactic Center with ANTARES and IceCube
    Nadège Iovine (ULB)
    18/10/2019 11:22
  7. 49. Dark matter capture in the Sun, uncertainties from the local dark matter distribution
    arturo nunez (Laboratoire d'Astrophysique de Marseille)
    18/10/2019 11:45
  8. 50. Statistics of the subhalo population in the Milky Way for the detection of dark matter point sources
    Gaétan Facchinetti (Laboratoire Univers et Particules Montpellier)
    18/10/2019 12:08
  9. 1. Dark matter constraints from dwarf galaxies: a data-driven analysis
    Pasquale Dario Serpico (LAPTh, Annecy-le-vieux)
  10. 2. Dark matter searches with the DarkSide LAr TPC
    Anyssa Navrer-Agasson (LPNHE)
  11. 4. First observation of two-neutrino double electron capture in 124Xe with XENON1T
    Dr Julien Masbou (SUBATECH)
  12. 5. Gravitational Waves from Dark Matter
    Dr Iason BALDES (ULB Bruxelles)
  13. 8. How to detect and produce dark matter from (dark) Freeze-in, the kinetic mixing portal example
    Laurent Vanderheyden (Université Libre de Bruxelles)

    Dark matter may belong to a hidden sector that is only feebly interacting with the Standard Model and may have never been in thermal equilibrium in the Early Universe. In this case, the observed abundance of dark matter particles could have been produced through a slow process. This applies to scenarios where Standard Model and Hidden Sector communicate through light mediator of mass less than...

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  14. 3. Prospects for heavy WIMP searches with H.E.S.S. and CTA
    Lucia Rinchiuso (SPP/Irfu)
  15. 7. Resummed photon spectrum from dark matter annihilation for intermediate and narrow energy resolution
    Martin Vollmann (Technische Universität München)
  16. 9. Update on the activities of the GPS on Dark Matter
    Dr Iason BALDES (ULB Bruxelles)
  17. 6. Voyager probes Dark Matter
    Mathieu Boudaud (LPTHE)
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