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
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Christophe Grojean18/02/2025, 10:10
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Ian Low18/02/2025, 11:10
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Shigeki Hirose18/02/2025, 13:30
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Koji Hashimoto18/02/2025, 14:10
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Zoltan Ligeti19/02/2025, 09:00
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Abner Soffer19/02/2025, 09:40
I will report recent results and prospects for future results from the Belle II experiment
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Sokratis Trifinopoulos19/02/2025, 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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Shingo Kazama19/02/2025, 11:10
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Takeo Moroi20/02/2025, 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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Motoko Fujiwara20/02/2025, 09:40
Electroweakly interacting stable particles in the (1 − 10) TeV mass range can be a dark matter candidate with rich testability.
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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... -
Wen Yin20/02/2025, 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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Akito Kusaka20/02/2025, 11:10
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Jacob Moritz21/02/2025, 09:00
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Kyohei Mukaida21/02/2025, 11:00
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Jorinde van de Vis21/02/2025, 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.
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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...