13–17 May 2024
CERN
Europe/Zurich timezone

Session

Unexplored signatures & wildcard ideas

8
14 May 2024, 09:00
40/S2-D01 - Salle Dirac (CERN)

40/S2-D01 - Salle Dirac

CERN

95
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Conveners

Unexplored signatures & wildcard ideas

  • Giuliano Gustavino (Sapienza Universita e INFN, Roma I (IT))
  • Monika Blanke (Karlsruhe Institute of Technology)
  • Alexander Grohsjean (Hamburg University (DE))

Presentation materials

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  1. Dr Atri Dey (Dublin Institute for Advanced Studies)
    14/05/2024, 09:00
  2. Prof. Alexander Belyaev (University of Southampton & Rutherford Appleton Laboratory)
    14/05/2024, 09:30

    We suggest a new class of models - Fermionic Portal Vector Dark Matter (FPVDM) which extends the Standard Model (SM) with SU(2)_D dark gauge sector. While FPVDM does not require kinetic mixing and Higgs portal. It is based on the Vector-Like (VL) fermionic doublet which couples the dark sector with the SM sector through the Yukawa interaction. The FPVDM framework provides a vector Dark Matter...

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  3. Max Fieg (University of California Irvine (US))
    14/05/2024, 10:00
  4. Thea Aarrestad (ETH Zurich (CH))
    14/05/2024, 10:30
  5. Jnanadeva Maharana (National Institute of Science Education and Research (IN))
    14/05/2024, 11:30
    Unexplored signatures & wildcard ideas

    t has been proposed that, in the large radius compactification (LRC) scenario, the Kaluza-Klein states might be considered as dark matter (DM) candidates. The universal extra dimension (UED) hypothesis, together with the LRC paradigm, holds the prospect of observing KK states at LHC if masses lie in the accessible LHC energy scale. If observed, they might be possible DM candidates, provided...

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  6. Konstantin Zioutas (University of Patras (GR))
    14/05/2024, 11:45
    Unexplored signatures & wildcard ideas

    Anti-quark nuggets, AQNs, (ZHITNITSKY, 2003), have been suggested to solve the dark matter (DM) and the missing antimatter problem in the universe, and have been proposed as an explanation of various observations.

    Their size is in the μm range and their density equal to the nuclear density with an expected flux of about 1 / km2 / year. For the typical velocity of DM constituents (~250...

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  7. James Pinfold (University of Alberta (CA))
    14/05/2024, 12:00

    The MoEDAL-MAPP experiment at Run-3 incorporates the MoEDAL and MAPP-1 (MoEDAL Apparatus for Penetrating Particles) detectors deployed at IP8 and in the UA83 tunnel on the LHC Ring, respectively. The passive, triggerless, MoEDAL detector has been taking data at Run-1 and Run-2 and is a world leader in the direct search for Highly Ionizing Particles (HIPs) at a Collider. HIP avatars of new...

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  8. Spyros Argyropoulos (Albert Ludwigs Universitaet Freiburg (DE))
    14/05/2024, 12:15
  9. Alvaro Lopez Solis (Deutsches Elektronen-Synchrotron (DE)), Marawan Barakat (Deutsches Elektronen-Synchrotron (DE)), Priscilla Pani (Deutsches Elektronen-Synchrotron (DE))
    Unexplored signatures & wildcard ideas

    The existence of a new type of non-baryonic matter in the Universe, also called Dark Matter (DM), is supported by compelling astrophysical and cosmological evidence. Considerations on its measured relic density favour the hypothesis that Dark Matter is composed primarily of Weakly Interacting Massive Particles (WIMPs). Unfortunately, numerous experiments targeting the detection of these DM...

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  10. James Pinfold (University of Alberta (CA))
    Unexplored signatures & wildcard ideas

    The MoEDAL-MAPP experiment at Run-3 incorporates the MoEDAL and MAPP-1 (MoEDAL Apparatus for Penetrating Particles) detectors deployed at IP8 and in the UA83 tunnel on the LHC Ring, respectively. The passive, triggerless, MoEDAL detector has been taking data at Run-1 and Run-2 and is a world leader in the direct search for Highly Ionizing Particles (HIPs) at a Collider. HIP avatars of new...

    Go to contribution page
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