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新学術領域「なぜ宇宙は加速するのか？- 徹底的究明と将来への挑戦-」(Why does the Universe accelerate?-Exhaustive study and challenge for the future)-MAR2019

3–4 Mar 2019
Asia/Tokyo timezone

Session

Morning session

3 Mar 2019, 09:30

Presentation materials

There are no materials yet.

  1. 1. opening remark
    Hitoshi Murayama (Berkeley/IPMU)
    03/03/2019, 09:30
  2. 2. A01 Update
    Misao Sasaki (Kavli IPMU)
    03/03/2019, 09:35
  3. 3. Clustering of Primordial Black Holes
    Yokoyama Shuichiro (Nagoya U.)
    03/03/2019, 10:05
  4. 4. Extended Cuscuton
    Tsutomu Kobayashi (Rikkyo U.)
    03/03/2019, 10:20
  5. 5. A02 Update (Summary)
    Fuminobu Takahashi (Tohoku U.)
    03/03/2019, 10:50
  6. 31. Primordial Black Hole in the Matter Dominated Universe
    Kazunori Kohri (KEK)
    03/03/2019, 11:00
  7. 6. Modeling evolution of dark matter substructure and annihilation boost
    Nagisa Hiroshima (U. Tokyo)
    03/03/2019, 11:20
  8. 7. Realization of the active pumping of the Thorium-229 isomeric state
    Takahiko Masuda (Okayama U.)
    03/03/2019, 11:35
  9. 35. Dark matter density profiles in the classical dwarf spheroidal galaxies in Milky Way
    Kohei Hayashi (ICRR)
    03/03/2019, 11:50
  10. 23. B03 update
    Masahiro Takada (Kavli IPMU)
    04/03/2019, 09:00
  11. 24. 大規模シミュレーションと次世代超広視野分光観測で解き明かすダークマターの正体
    Tomoaki Ishiyama (Chiba U.)
    04/03/2019, 09:30
  12. 25. Numerical simulation of cosmic relic neutrinos in the large-scale structure formation
    Kohji Yoshikawa (U. Tsukuba)
    04/03/2019, 09:45
  13. 26. B04 update
    Tomonori Usuda (NAOJ)
    04/03/2019, 10:00
  14. 27. D01 updaet
    Eiichiro Komatsu (MPA)
    04/03/2019, 10:45
  15. 28. Toward the detection of cosmological neutral-hydrogen 21cm radiation through cross-correlation with galaxies and CMB
    Keitaro Takahashi (Kumamoto U.)
    04/03/2019, 11:15
  16. 29. Discussion & Closing remark
    04/03/2019, 11:30
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