Jun 21 – 24, 2016
Roma
Europe/Rome timezone

Session

Posters

Jun 23, 2016, 7:10 PM
Roma

Roma

Presentation materials

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  1. Dr Vincenzo Vitale (ROMA2)
    6/23/16, 7:15 PM
    The China Seismo-Electromagnetic Satellite (CSES) has the purpose to measure electromagnetic waves emissions, plasma properties and particles fluxes in the Earth ionosphere and magnetosphere, to investigate the possible correlation with seismic events. Phenomena related to the solar-terrestrial interactions, such as Coronal Mass Ejections (CMEs), and the study of low energy cosmic rays are...
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  2. Mr Carlo Romoli (Dublin Institute for Advanced Studies)
    6/23/16, 7:16 PM
  3. Dr Pramod Kumar Purohit (National Institute of Technical Teachers’ Training and Research, Bhopal – 462002, MP, India.)
    6/23/16, 7:17 PM
  4. Dr Federico Fraschetti (University of Arizona)
    6/23/16, 7:18 PM
  5. Dr Izabela Anna Kochanek (LNGS)
    6/23/16, 7:19 PM
  6. Dr Elena Orlando (Stanford University)
    6/23/16, 7:20 PM
  7. Silvia Raino' (BA)
    6/23/16, 7:21 PM
  8. Ms Iryna Lypova
    6/23/16, 7:22 PM
  9. Dr Eugenio Bottacini (Stanford University)
    6/23/16, 7:23 PM
  10. Elisabetta Bissaldi (BA)
    6/23/16, 7:24 PM
  11. Elisabetta Bissaldi (BA)
    6/23/16, 7:25 PM
  12. Elisabetta Bissaldi (BA)
    6/23/16, 7:26 PM
  13. Giulia De Bonis (ROMA1)
    6/23/16, 7:27 PM
  14. Emanuele Leonora (CT)
    6/23/16, 7:28 PM
  15. Dr Ralf Wischnewski (DESY)
    6/23/16, 7:29 PM
  16. Ms Maíra Dutra (Laboratoire de Physique Théorique)
    6/23/16, 7:30 PM
    While astrophysical evidences for the existence of dark matter (DM) have been accumulated during the past decades, it is still not understood the fundamental physics involved. No unambiguous positive signal of DM particles have been found in searches specially dedicated to the well motivated WIMP candidates, whose mass vary from GeV to a few TeV. This encourage us to consider non-standard...
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  17. Dr Andrea Rappoldi (PV)
    6/23/16, 7:31 PM
    There are several suggestions to probe space-time fuzziness (also space-time foam) due to the quantum mechanics nature of space-time. These effects are predicted to be very small, being related to the Planck length, so that the only hope to experimentally detect them is to look at propagation of particles along cosmological distances. A fenomenological approach suggests that photons from...
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  18. Paolo Walter Cattaneo (PV)
    6/23/16, 7:32 PM
    The direct observation of high-energy cosmic rays, up to the PeV region needs highly performing calorimeters. Space operation requires great effort in optimizing size and mass. Calocube is a homogeneous calorimeter whose basic geometry is cubic and isotropic, so as to detect particles from every direction, maximizing the acceptance. High ranularity is obtained by filling the volume with...
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  19. Gonzalo Rodriguez Fernandez (ROMA2)
    6/23/16, 7:33 PM
  20. Silvia Celli (GSSI)
    6/23/16, 7:34 PM
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