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PPC 2025: XVIII International Conference on Interconnections between Particle Physics and Cosmology

Jun 23 – 27, 2025
SpringHill Suites Conference Center Deadwood
US/Mountain timezone

Local Organizing Committee

Session

PPC Presentations

Jun 25, 2025, 8:30 AM
Roosevelt Room I (SpringHill Suites Conference Center Deadwood)

Roosevelt Room I

SpringHill Suites Conference Center Deadwood

Cadillac Jack's Resort 360 Main St, Deadwood, SD 57732

Conveners

PPC Presentations: Wednesday AM: Plenary

  • Valentina De Romeri

Presentation materials

There are no materials yet.

  1. 151. Plenary: Cosmic Concordance Across Scales
    Vera Gluscevic
    6/25/25, 8:30 AM

    Author and Presenter: Vera Gluscevic

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  2. 48. Plenary: Dark Matter and Dark Sector Searches in the First KM3NeT Data
    Sara Rebecca Gozzini (IFIC, CSIC-UV)
    6/25/25, 9:00 AM

    Author and Presenter: SaraRebecca Gozzini
    Abstract: KM3NeT is a multi-purpose neutrino observatory composed of underwater Cherenkov arrays with different geometries. Currently, two KM3NeT detectors are under construction in the Mediterranean Sea: ORCA, a compact and dense detector optimised for the high-statistic measurement of atmospheric neutrino physics, and ARCA, a set of two telescopes...

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  3. 106. Plenary: IceCube - The Experiment, Its Data and Science
    Xinhua Bai (SDSMT)
    6/25/25, 9:30 AM

    Author: Xinhua Bai
    Presenter: Xinhua Bai
    Abstract: IceCube, a cubic kilometer neutrino observatory at the South Pole has accumulated an unprecedented amount of data since its completion in 2010-2011. Besides its primary science goal of neutrino astronomy, IceCube data support a variety of cutting-edge research in high-energy cosmic rays, particle interactions, neutrino physics, dark matter...

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  4. 112. Plenary: Sub-GeV Dark Matter Direct Detection with Neutrino Observatories
    Rebecca Leane (SLAC)
    6/25/25, 10:00 AM

    Author and Presenter: Rebecca Leane
    Abstract: I will present a new opportunity for sub-GeV dark matter (DM) detection using large-volume neutrino detectors. DM-electron scattering in an observatory can excite or ionize target molecules, which then produce light that can be detected by the photomultiplier tubes (PMTs). While individual DM scatterings are undetectable, the aggregate rate from...

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