Session

plenary

18 Feb 2025, 10:10
seminar hall (Building 3)

seminar hall

Building 3

KEK, Tsukuba campus

Conveners

plenary: Christophe Grojean

  • Ryuichiro Kitano

plenary: Ian Low

  • Ryuichiro Kitano

plenary: Shigeki Hirose, Koji Hashimoto

  • Ian Low

plenary: Zoltan Ligeti, Abner Soffer

  • Motoi Endo

plenary: Sokratis Trifinopoulos, Shingo Kazama

  • Motoi Endo

plenary: Takeo Moroi, Motoko Fujiwara

  • Kyohei Mukaida

plenary: Wen Yin, Akito Kusaka

  • Kyohei Mukaida

plenary: Jacob Moritz

  • Yuta Hamada

plenary: Kyohei Mukaida, Jorinde van de Vis

  • Yuta Hamada

Presentation materials

There are no materials yet.

  1. Christophe Grojean
    18/02/2025, 10:10
  2. Ian Low
    18/02/2025, 11:10
  3. Shigeki Hirose
    18/02/2025, 13:30
  4. Koji Hashimoto
    18/02/2025, 14:10
  5. Zoltan Ligeti
    19/02/2025, 09:00
  6. Abner Soffer
    19/02/2025, 09:40

    I will report recent results and prospects for future results from the Belle II experiment

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  7. Sokratis Trifinopoulos
    19/02/2025, 10:30

    The Cabibbo-Kobayashi-Maskawa (CKM) matrix, which controls flavor mixing between the three generations of quark fermions, is a key input to the Standard Model of particle physics. In this paper, we identify a surprising connection between quantum entanglement and the degree of quark mixing. Focusing on a specific limit of 2→2 quark scattering mediated by electroweak bosons, we find that the...

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  8. Shingo Kazama
    19/02/2025, 11:10
  9. Takeo Moroi
    20/02/2025, 09:00

    I will discuss a possibility to use quantum bits (qubits) for wave-like-dark-matter detection. I will explain the basic idea and show the expected sensitivity. I will also discuss an idea to enhance the sensitivity using quantum nature of the qubits.

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  10. Motoko Fujiwara
    20/02/2025, 09:40

    Electroweakly interacting stable particles in the (1 − 10) TeV mass range can be a dark matter candidate with rich testability.
    In particular, gamma-ray line-like features are expected to be a smoking-gun signature for indirect detection.
    In this framework, one fundamental question follows; how to distinguish DM spin among DM candidates with the same electroweak interaction by contrasting...

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  11. Wen Yin
    20/02/2025, 10:30

    I will present a low-cost experimental proposal for axion searches at synchrotron radiation facilities, such as SPring-8, NanoTerasu, and Photon Factory. Specifically, I will discuss the method for calculating axion production in an undulator, a type of light source widely used across various fields. By positioning an axion detector outside the shield used in the primary experiments, we can...

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  12. Akito Kusaka
    20/02/2025, 11:10
  13. Jacob Moritz
    21/02/2025, 09:00
  14. Kyohei Mukaida
    21/02/2025, 11:00
  15. Jorinde van de Vis
    21/02/2025, 11:40

    Cosmological first order phase transitions are a promising source of gravitational waves, and a possible explanation of the baryon asymmetry and dark matter abundance.
    Predicting the phenomenological consequences of such phase transitions requires knowledge of the expansion velocity of the bubbles formed in a phase transition.
    In this talk, I will present WallGo, a software package for the...

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