Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientist
Physics
High Energy Physics
High Energy Physics - Phenomenology
Scientist
Deutsches Elektronen Synchrotron DESY, Notkestrasse 85, 22603 Hamburg, Germany
Deutsches Elektronen Synchrotron DESY, Notkestrasse 85, 22607, Hamburg, Germany
Dep't Earth & Planet. Sci. Tokyo Inst. Tech., Tokyo, Japan
Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Tokyo, Japan
Tokyo Institute of Technology, Tokyo, Japan;
Tokyo Institute of Technology, Meguro-ku, Japan;
Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Tokyo, Japan;
Ministry of Posts and Telecommunications, Radio Research Laboratories, Tokyo, Japan
Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo, 152-8551 Japan
Onagawa Magnnetic Observatory, Faculty of Science, Tohoku University, Sendai 980 Japan
Ministry of Posts and Telecommunications, Radio Research Laboratories, Kashima, Japan
Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro, 152-8551, Japan
Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Meguro, Tokyo, 152-8551, Japan
Dep't Earth & Plante. Sci., Tokyo Inst. Tech., 2-12-1, Oookayama, Meguro, Tokyo, 152-8551, Japan
Department of Earth and Planetary Sciences, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo, 152-8550, Japan
Department of Earth and Planetary Sciences, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551, Japan
Department of Earth and Planetary Sciences, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, 152-8551, Tokyo, Japan
Department of Earth and Planetary Sciences, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo, 152-8551, Japan
Tokyo Institute of Technology, Meguro-ku, Japan
Dept Earth & Env. Sci., Kumamoto Univ, Kumamoto, Ja
511 keV line from Q balls in the Galactic Center
A note on "The Affleck-Dine Mechanism in Conformally Sequestered Supersymmetry Breaking"
A numerical dynamo benchmark
A numerical study on magnetic polarity transition in an MHD dynamo model
A possible anthropic solution to the Strong CP problem
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