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Dark Matter

Dark Matter

These are UTokyo reserch groups aiming to search for Dark Matter Particles with world-leading experiments of highest sensitivity and to develop new search methods. See more details at each group page.

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XENONnT Experiment UTokyo Group

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暗黒物質検出器開発1

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暗黒物質検出器開発2

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XMASS Experiment (Completed)

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Research Fields

Neutrino

Neutrino

Elucidate an Elementary Particle, Neutrino and Observe the Universe by Neutrino

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Gravitational Wave

Gravitational Wave

Promote Gravitational Wave Astronomy with Large-scale Cryogenic Gravitational Wave Telescope, KAGRA as a Part of World Gravitational Wave Observation Network

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Gamma Ray

Gamma Ray

Explore the Universe at High Energies by Observing Gamma Rays, Very-High-Energy, Short-Wavelength Form of Electromagnetic Waves

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Cosmic Rays（Charged Particles）

Cosmic Rays（Charged Particles）

Detect Air Showers Produced by Cosmic Rays (Charged Particles) to Search for Their Origins

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Dark Matter

Dark Matter

Serch for Dark Matter Particles with World-Leading Experiments of Highest Sensitivity

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Electromagnetic Waves（IR/Optical, X-ray）

Electromagnetic Waves（IR/Optical, X-ray）

Detect Electromagnetic Waves Whose Spectrum Ranges from Low Energies of Radio Waves to Mid-range Energies Found in Infrared, Optical (Visible) and Ultraviolet Light to Very Highest Energies of X-rays

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Simulation & Theory

Simulation & Theory

Study Various High-energy Astrophysical Objects, which are Sources of Cosmic Rays, via Numerical Simulation and Theoretical Methods

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