Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
UIUC & Osaka U.
Osaka University
University of Tokyo
Univ. of Tokyo
Osaka & UIUC
Univ. Tokyo
Kyoto U.
Department of Earth and Space Science, Faculty of Science, Osaka University, Toyonaka, Osaka 560, Japan
Department of Earth and Space Science, Graduate School of Science, Osaka University, Toyonaka, Osaka 560, Japan
Graduate School of Arts and Sciences, University of Tokyo, Komaba, Meguro, Tokyo 153-8902, Japan
Department of Earth and Space Science, Osaka University, Toyonaka 560-0043, Japan
Department of Physics, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801
Graduate School of Arts and Science, The University of Tokyo, Komaba, Meguro, Tokyo 153-8902, Japan
Department of Physics, Kyoto University, Kyoto 606-01, Japan
Graduate School of Arts and Sciences, University of Tokyo, Komaba, Tokyo 153-8902, Japan
Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502, Japan
High Energy Accelerator Research Organization
The Tibet AS gamma Collaboration
NA61 / SHINE Collaboration
The Tibet ASgamma Collaboration
Yokohama National University, Yokohama, Kanagawa, Japan
Nuclear Science Division, Institute for Chemical Research, Kyoto University, Uji, Kyoto 611, Japan
Faculty of Engineering, Yokohama National University, Yokohama 240-8501, Japan
Faculty of Education, Yokohama National University, Japan
Faculty of Education, Yokohama National University, Yokohama, Japan
Faculty of Engineering, Yokohama National University, Yokohama 240-0067, Japan
Department of Energy Engineering and Science, Nagoya University, Nagoya 464-8603, Japan
Department of Phy
3D Numerical Simulation of Black Hole Formation Using Collisionless Particles --- Triplane Symmetric Case---
A coupled microwave-cavity system in the Rydberg-atom cavity detector for dark matter axions
A Formation Mechanism of Collapsar Black Hole -- early evolution phase
A large underground water Cherenkov muon detector array with the Tibet air shower array for Gamma-ray astronomy in the 100 TeV region: detector design and simulation
A large underground water Cherenkov muon detector array with the Tibet air shower array for the Gamma-ray astronomy in the 100 TeV region: Overview and physics goal
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