22 November 2019
The University of Tokyo, Hongo Campus
Asia/Tokyo timezone

Contribution List

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  1. Ryu Sawada (University of Tokyo (JP))
    22/11/2019, 10:30
  2. Satoshi Shirai (Kavli IPMU)
    22/11/2019, 10:35
  3. Hideyuki Oide (Tokyo Institute of Technology (JP))
    22/11/2019, 10:55
  4. Shu-Yu Ho (Tohoku University)
    22/11/2019, 12:40
  5. Osamu Sato (Nagoya University (JP))
    22/11/2019, 13:05
  6. Shintaro Eijima (KEK)
    22/11/2019, 13:35
  7. Sreemanti Chakraborti (Indian Institute of Technology Guwahati)
    22/11/2019, 14:00
  8. Toshiaki Kaji (Waseda University (JP))
    22/11/2019, 14:25
  9. Satoshi Shirai (Kavli IPMU)
    22/11/2019, 15:25
  10. Atsushi Mizukami (High Energy Accelerator Research Organization (JP))
    22/11/2019, 15:50
  11. Arindam Das (Osaka University)
    22/11/2019, 16:15
  12. Shohei Shirabe (Tokyo Institute of Technology (JP))
    22/11/2019, 16:40
  13. Osamu Jinnouchi (Tokyo Institute of Technology (JP))
    22/11/2019, 17:20
  14. Sreemanti Chakraborti (Indian Institute of Technology, Guwahati)

    We present a scenario capable of addressing dark matter (DM) through freeze-in and freeze-out mechanisms, depending on the region of the parameter space considered. In DM dynamics, the model features an interplay of thermal production along with sizeable production through feeble decay of associated dark fermionic partner, which finally freezes out to right relic density for a wide range of...

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