21–22 Nov 2017
CERN
Europe/Zurich timezone
There is a live webcast for this event.

Contribution List

43 out of 43 displayed
Export to PDF
  1. Claude Vallee (Centre de Physique des Particules de Marseille)
    21/11/2017, 08:30
  2. Philip Schuster (Perimeter Institute for Theoretical Physics)
    21/11/2017, 09:00
  3. Joerg Jaeckel (ITP Heidelberg)
    21/11/2017, 09:30
    BSM

    Where we stand, possibilities, comparative reach

    Go to contribution page
  4. Richard Jacobsson (CERN)
    21/11/2017, 10:00
    BSM
  5. Tommaso Spadaro (INFN e Laboratori Nazionali di Frascati (IT))
    21/11/2017, 10:20
    BSM
  6. Cristina Lazzeroni (University of Birmingham (GB))
    21/11/2017, 11:10
    BSM
  7. Sergei Gninenko (Russian Academy of Sciences (RU))
    21/11/2017, 11:30
    BSM
  8. Axel Lindner (DESY)
    21/11/2017, 11:50
    BSM
  9. Yannis Semertzidis (CAPP/IBS and KAIST in South Korea)
    21/11/2017, 12:10
    BSM
  10. Igor Garcia Irastorza (Universidad de Zaragoza (ES))
    21/11/2017, 12:30
    BSM
  11. Gunar Schnell, Jan M. Pawlowski (University of Heidelberg), Markus Diehl
    21/11/2017, 14:00
    QCD

    Landscape, where we stand, possibilities, comparative reach

    Go to contribution page
  12. Giacomo Graziani (INFN, Sezione di Firenze (IT))
    21/11/2017, 14:30
    QCD
  13. Pasquale Di Nezza (INFN e Laboratori Nazionali di Frascati (IT))
    21/11/2017, 14:45
    QCD
  14. Laure Marie Massacrier (Université Paris-Saclay (FR))
    21/11/2017, 15:00
    QCD
  15. Jean-Philippe Lansberg (IPN Orsay, Paris Sud U. / IN2P3-CNRS)
    21/11/2017, 15:15
    QCD
  16. Achille Stocchi (Universite de Paris-Sud 11 (FR))
    21/11/2017, 16:00
    QCD
  17. Gianluca Usai (Universita e INFN, Cagliari (IT))
    21/11/2017, 16:15
    QCD
  18. Marek Gazdzicki (Johann-Wolfgang-Goethe Univ. (DE))
    21/11/2017, 16:30
    QCD
  19. Leonid Nemenov (Joint Institute for Nuclear Research (RU))
    21/11/2017, 16:45
    QCD
  20. Graziano Venanzoni (INFN e Laboratori Nazionali di Frascati (IT))
    21/11/2017, 17:00
    QCD
  21. Oleg Denisov (INFN, sezione di Torino)
    21/11/2017, 17:15
    QCD
  22. Mike Lamont (CERN)
    22/11/2017, 09:00
  23. Eirini Koukovini Platia (CERN)
    22/11/2017, 09:15
  24. Lau Gatignon (CERN)
    22/11/2017, 09:30
  25. Mieczyslaw Krasny (Centre National de la Recherche Scientifique (FR))
    22/11/2017, 09:50
  26. Jorg Pretz (Rheinisch Westfaelische Tech. Hoch. (DE))
    22/11/2017, 10:10
  27. Mike Lamont (CERN)
    22/11/2017, 11:00
  28. Massimiliano Ferro-Luzzi (CERN)
    22/11/2017, 11:20
  29. Edda Gschwendtner (CERN), Matthew Wing (University College London)
    22/11/2017, 11:40
  30. Kenneth Richard Long (Imperial College (GB))
    22/11/2017, 11:55
  31. Andrzej Siemko (CERN), Babette Dobrich (CERN)
    22/11/2017, 12:10
  32. Antonio Polosa (Sapienza Universita` di Roma)
    22/11/2017, 14:00

    Directional detection of Dark Matter particles in the MeV mass range could be accomplished by studying electron recoils in large arrays of parallel carbon nanotubes. In a scattering process with a lattice electron, a DM particle might transfer sufficient energy to eject it from the nanotube surface. An external electric field is added to drive the electron towards the open ends of the array,...

    Go to contribution page
  33. Paolo Spagnolo (INFN Sezione di Pisa, Universita' e Scuola Normale Superiore, P)
    22/11/2017, 14:15

    In Particle Physics, axions appear in very well motivated extensions of the Standard Model including the Peccei-Quinn mechanism proposed to solve the long-standing strong-CP problem. Together with the weakly interacting massive particles of supersymmetric theories, axions are also a favored candidate for resolving the Dark Matter issue.
    I propose a new detection scheme for the search of...

    Go to contribution page
  34. Guido Zavattini (Università di Ferrara)
    22/11/2017, 14:30

    For many years the PVLAS collaboration has been working on trying to measure vacuum magnetic birefringence using optical techniques. That electrodynamics in vacuum is non-linear was predicted in 1935 [H. Euler and B. Kockel, Naturwiss, 23, 246 (1935)] and the first experimental proposal to detect the leading nonlinear effect, namely vacuum magnetic birefringence closely related to...

    Go to contribution page
  35. Martin Gonzalez-Alonso (CERN), Stephan Malbrunot (CERN)
    22/11/2017, 14:45
  36. Fernando Martinez Vidal (IFIC - University of Valencia and CSIC (ES))
    22/11/2017, 15:10
  37. Matthew Wing (University College London)
    22/11/2017, 16:00
  38. Steinar Stapnes (CERN)
    22/11/2017, 16:20
  39. Roberto Carosi (INFN - National Institute for Nuclear Physics)
    22/11/2017, 16:40
  40. Martin Gonzalez-Alonso (CERN)

    I will discuss what kind of new phenomena can be probed through precision measurements in nuclear and neutron beta decays. Several of these experiments were carried out (or are planned/ongoing) at ISOLDE at CERN, a world-leading facility In the field of nuclear physics. Using a model-independent description I will review the interplay between the different experiments and which ones are the...

    Go to contribution page