Login

Dark Ghosts - 3rd GNN Workshop on Indirect Dark Matter Searches with Neutrino Telescopes

31 March 2022 to 1 April 2022
Faculty of Science - University of Granada
Europe/Madrid timezone

Contribution List

30 out of 30 displayed
Export to PDF
  1. 6. DM searches with ANTARES/KM3NeT
    Sara Rebecca Gozzini
    31/03/2022, 10:00
  2. 7. DM searches with IceCube
    Stephan Meighen-Berger (Technical University of Munich (TUM))
    31/03/2022, 10:20
  3. 8. DM searches with GVD
    Olga Suvorova
    31/03/2022, 10:40
  4. 9. In memoriam Tom Gaisser
    Juan Antonio Aguilar Sanchez (Université Libre de Bruxelles)
    31/03/2022, 11:00
  5. 10. Multi-messenger lifetime constraints on heavy decaying dark matter
    Mr Rasmi Hajjar (IFIC (CSIC-UV))
    31/03/2022, 11:55
  6. 11. Neutrino lines in DM searches
    Juan Antonio Aguilar Sanchez (Université Libre de Bruxelles)
    31/03/2022, 12:15
  7. 12. Why secluded DM at neutrino telescopes?
    Filippo Sala (CNRS and Sorbonne University)
    31/03/2022, 12:35
  8. 13. Dark Matter Decay and Annihilation to Neutrinos
    Diyaselis Delgado Lopez (Harvard University (US))
    31/03/2022, 12:55
  9. 14. Constraining EeV-Scale Dark Matter with Neutrino Observatories Using Tau Regeneration
    Jeffrey Lazar (University of Wisconsin-Madison)
    31/03/2022, 14:45
  10. 15. DM searches in the Galactic Centre with IceCube
    Dr Nadege Iovine (Université libre de Bruxelles (ULB))
    31/03/2022, 15:05
  11. 16. Dark matter evaporation from celestial bodies
    Sergio Palomares-Ruiz (IFIC-Valencia)
    31/03/2022, 15:25
  12. 17. Limits for Dark Matter annihilation in the Sun with ANTARES neutrino telescope
    Chiara Poirè (UPV)
    31/03/2022, 15:45
  13. 18. PPPC4
    Marco Cirelli (CNRS LPTHE Jussieu)
    31/03/2022, 16:35
  14. 20. Warm dark matter searches from the Galactic halo
    Ariane Dekker (University of Amsterdam)
    31/03/2022, 16:55
  15. 19. Higgs portals to DM
    Abdelhak Djouadi (University of Granada)
    31/03/2022, 17:15
  16. 21. Searches with gamma-rays
    Javier Rico (IFAE)
    01/04/2022, 10:00
  17. 22. Future dark matter searches
    Bradley Kavanagh
    01/04/2022, 10:20
  18. 23. Direct searches of dark matter
    Maria Martinez (Universidad de Zaragoza)
    01/04/2022, 10:40
  19. 24. Decaying Dark Matter at IceCube and its Signature in High-Energy Gamma-Ray Experiments
    Barbara Skrzypek
    01/04/2022, 11:00
  20. 25. Solar atmospheric neutrinos with ANTARES
    Daniel Lopez-Coto (ANTARES, KM3NeT, Universidad de Granada)
    01/04/2022, 11:50
  21. 26. Dark ghosts from the solar disk
    Manuel Masip (Universidad de Granada)
    01/04/2022, 12:10
  22. 27. DM from the center of the Earth with IceCube
    Giovanni Renzi
    01/04/2022, 12:30
  23. 28. Gambit
    Aaron Vincent (Durham University)
    01/04/2022, 14:30
  24. 29. Charon: A Tool for Neutrino Flux Generation from WIMPs
    Jeffrey Lazar (University of Wisconsin-Madison)
    01/04/2022, 14:50
  25. 30. Simplified DM models, Application of DD & collider experiments
    Sven Heinemeyer (CSIC (Madrid, ES))
    01/04/2022, 15:10
  26. 2. Charon: A Tool for Neutrino Flux Generation from WIMPs
    Jeffrey Lazar (University of Wisconsin-Madison)

    Indirect searches for signatures of corpuscular dark matter have been performed using all cosmic messengers: gamma rays, cosmic rays, and neutrinos. The search for dark matter from neutrinos is of particular importance since they are the only courier that can reach detectors from dark matter processes in dense environments, such as the core of the Sun or Earth, or from the edge of the...

    Go to contribution page
  27. 3. Constraining EeV-Scale Dark Matter with Neutrino Observatories Using Tau Regeneration
    Jeffrey Lazar (University of Wisconsin-Madison)

    In 2016 and 2018, the ANITA collaboration reported the observation of two anomalous events, with polarizations consistent with up-going neutrinos, but coming from too far below the horizon to have traversed Earth given their energies. While all Standard Model (SM) explanations of these events have been ruled out, explanations from beyond Standard Model scenarios have been put forth in the...

    Go to contribution page
  28. 1. Dark Matter Decay and Annihilation to Neutrinos
    Diyaselis Delgado Lopez (Harvard University (US))

    Dark matter particles are predicted to decay or annihilate into Standard Model particles which would produce signals of neutrinos, gamma-rays, and other secondary particles. As no such signal has yet been detected, we turn to the least constrained channel where neutrinos provide an avenue to probe astrophysical sources of dark matter particles. We review the decay and annihilation of dark...

    Go to contribution page
  29. 4. Decaying Dark Matter at IceCube and its Signature in High-Energy Gamma-Ray Experiments
    Barbara Skrzypek

    The measurement of ultra-high energy starting event neutrinos in the TeV-PeV range in IceCube has afforded us with the possibility of answering questions through multimessenger efforts in astroparticle physics. However, the origin and nature of these astrophysical neutrinos is still largely unresolved. Among existing tensions, for example, is the excess of neutrinos observed in the energy...

    Go to contribution page
  30. 5. Limits for Dark Matter annihilation in the Sun with ANTARES neutrino telescope
    Chiara Poirè (UPV)

    One of the most popular candidate of Dark Matter (DM) particle are the Weakly Interacting Massive Particles (WIMPs). These, once gravitationally captured in massive celestial objects and annihilating between them into Standard Model particles, can be indirectly detected. The centre of those massive objects is, therefore, a place where to look for a possible neutrino excess from DM...

    Go to contribution page