Research field (1):
Theoretical studies related to particle-, nuclear-, cosmic ray and astro-physics
Research keywords (4):
インフレーション
, 素粒子論的宇宙論
, 超対称理論
, 暗黒物質
Research theme for competitive and other funds (7):
2020 - 2025 極弱相互作用を持つ軽い新粒子の描く新宇宙描像とその実験的検証
2018 - 2023 ニュートリノで探る対称性と宇宙像
2017 - 2021 New physics from dark matter and Higgs
2017 - 2021 Cosmological Evolution and Search for Light New Particles with Ultraweak Interactions
2017 - 2019 超対称素粒子模型の真空構造解明とインフレーション宇宙の新展開
2010 - 2012 宇宙線およびLHC実験にもとづく標準模型を越えた物理の研究
2007 - 2009 超対称素粒子模型を用いた宇宙暗黒物質問題の解明
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Papers (53):
Yoshihiro Gunji, Koji Ishiwata, Takahiro Yoshida. Supersymmetric baryogenesis in a hybrid inflation model. Journal of High Energy Physics. 2023. 2023. 8
Koji Ishiwata. Topology-insensitive axion mass in magnetic topological insulators. Physical Review B. 2022. 106. 19
Shin’ichiro Ando, Nagisa Hiroshima, Koji Ishiwata. Constraining the primordial curvature perturbation using dark matter substructure. Physical Review D. 2022. 106. 10
Yoshihiro Gunji, Koji Ishiwata, Takahiro Yoshida. Subcritical regime of hybrid inflation with modular A4 symmetry. Journal of High Energy Physics. 2022. 2022. 11
Koji Ishiwata, Eiichiro Komatsu, Ippei Obata. Axion-gauge field dynamics with backreaction. Journal of Cosmology and Astroparticle Physics. 2022. 2022. 03. 010-010
Junji Hisano, Koji Ishiwata, Natsumi Nagata, Masato Yamanaka. Direct detection of vector dark matter (vol 126, pg 435, 2011). PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS. 2015. 10
Ishiwata Koji. 24aGE-4 Cosmic gamma-ray from inverse Compton process in unstable dark matter scenario. Meeting abstracts of the Physical Society of Japan. 2012. 67. 1. 3-3
Ishiwata Koji, Matsumoto Shigeki, Moroi Takeo. 13pSJ-4 Cosmic Gamma-ray from Inverse Compton Process in Unstable Dark Matter Scenario. Meeting abstracts of the Physical Society of Japan. 2009. 64. 2. 18-18
Ishiwata Koji, Ito Takumi, Moroi Takeo. 27aVP-7 Long-Lived Unstable Superparticles at the LHC. Meeting abstracts of the Physical Society of Japan. 2009. 64. 1. 3-3