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Seventeenth Marcel Grossmann Meeting

7–12 Jul 2024
Aurum, the ‘Gabriele d’Annunzio’ University and ICRANet
Europe/Rome timezone

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Session

Dark matter detection

DM1
12 Jul 2024, 15:00
Aurum, the ‘Gabriele d’Annunzio’ University and ICRANet

Aurum, the ‘Gabriele d’Annunzio’ University and ICRANet

Pescara, Italy

Conveners

Dark matter detection: Friday block 1

  • Ning Zhou (Shanghai Jiao Tong University)
  • Qian Yue (Tsinghua University)
  • Qiang Yuan (Purple Mountain Observatory, Chinese Academy of Sciences)

Description

Dark matter detection has been an exciting frontier over the past twenty years. Particle physicists and astrophysicists are probing wide mass ranges to hunt for different dark matter (DM) candidates. In this parallel session, the speakers are welcome to present the experimental and theoretical works on both direct and indirect DM detection as well as the collider detection of DM, including such as WIMP candidates and beyond.

Presentation materials

There are no materials yet.

  1. 250. The Galileo for Science Project (G4S_2.0): Domain Wall Dark Matter and Atomic Clocks
    Dr Massimo Visco (IAPS-INAF)
    12/07/2024, 15:00
    Dark matter detection
    Invited talk in a parallel session

    G4S_2.0 (Galileo for Science) is an ongoing project funded by the Italian Space Agency (ASI) and carried out by the Center for Space Geodesy (ASI-CGS) in Matera, the Istituto di Astrofisica e Planetologia Spaziali (IAPS/INAF) in Rome, and the Politecnico di Torino (POLITO). The project's goal is to address several intriguing challenges, including Fundamental Physics measurements using the...

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  2. 382. Ultralight scalar and axion dark matter detection with long-baseline atom interferometers
    Dr Wei Zhao (Shandong University of Aeronautics)
    12/07/2024, 15:25
    Dark matter detection
    Talk in a parallel session

    The detection of dark matter is a challenging problem in modern physics.
    We provide a proposal to detect the coupling of ultralight scalar dark matter to quarks and gluons as well as the coupling of ultralight axion dark matter to gluons with long-baseline atom interferometers. The ultralight scalar and axion dark matter could induce the oscillation of the nuclear charge radii and then...

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  3. 5. Who knows what dark matter lurks in the heart of M87: The shadow knows, and so does the ringdown.
    Dr Ramin Daghigh (Metropolitan State University)
    12/07/2024, 15:45
    Dark matter detection
    Talk in a parallel session

    We calculate the effect of dark matter on the ringdown waveform and shadow of supermassive black holes at the core of galaxies. Our main focus is on the supermassive black hole at the core of M87, which is large enough to allow for viable observational data. We compare the effects of a dark matter spike to those expected from a galactic halo of the same mass. Our calculation for the halo...

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