28 October 2024 to 1 November 2024
Kavli IPMU
Asia/Tokyo timezone
Stay tuned! We will be announcing our speakers soon. In the meantime, we are open for participant registrations. If you are interested in presenting your work, please contact us. We look forward to your participation!

Kashiwa-no-ha Dark Matter and Cosmology Symposium (Satellite workshop of COSMO 2024)

Rationale

The Kashiwanoha Dark Matter and Cosmology Symposium is a continuation of the Kashiwa Dark Matter Symposium. The Kashiwa Dark Matter Symposium is a yearly conference that started in 2019 sponsored by ICRR (+grants). From 2024, this conference is organized by IPMU and while maintaining the original goals, we are also expanding the scope to include topics relevant for the researchers at IPMU. The Kashiwanoha Dark Matter and Cosmology symposium series has the goal to regularly bring together international researchers from all relevant experimental and theoretical fields in current and future dark matter searches and cosmology. This year, we will have a special symposium since we are combining it with the “Satellite workshop of COSMO 2024” which will bring international researchers attending COSMO 2024 in Kyoto to IPMU. We believe this is a great opportunity to have a very strong line up of speakers and participants in cosmology and dark matter at IPMU.

Dates

October 28 – November 1, 2024

Topics

  • Early Universe Cosmology
  • Large Scale Structure
  • Gravitational Waves
  • Modified Gravity & Dark Energy
  • Observational Cosmology
  • Numerical Cosmology
  • Near Field Cosmology
  • Dark Matter Theory
  • Dark Matter Experiments

Speaker List

Invited speaker list (as of 2024-06-28):

  • Alexander Kusenko - University of California, Los Angeles (UCLA), Kavli IPMU
  • Ana Achucarro - Leiden Univ.
  • Angelo Carvano - Paris, Inst. Astrophys.
  • Camila P. Novaes - Sao Jose, INPE
  • Gabi Sato-Polito - Institute for Advanced Study
  • Gonzalo Palma - Universidad de Chile
  • Laura Baudis - Zurich Univ.
  • Leah Jenks - Chicago U., KICP
  • Lu Yin - Asia Pacific Center for Theoretical Physics (APCTP)
  • Meng-Xiang Lin - University of Pennsylvania
  • Miho Ishigaki - National Astronomical Observatory of Japan, Kavli IPMU
  • Noriko Y. Yamasaki - QUP, ISAS/JAXA
  • Oksana Iarygina - Nordita
  • Shinji Mukohyama - Kyoto University, Yukawa Institute for Theoretical Physics (YITP), Kavli IPMU, Institute for Cosmic Ray Research (ICRR)
  • Tanvi Karwal - Chicago U. 
  • Thomas Siegert - Julius-Maximilians-Universität Würzburg
  • Tomohiro Fujita - Ochanomizu University
  • Yuko Urakawa - (KEK, Tsukuba and Sokendai, Tsukuba)

On-site Venue

The on-site symposium will take place at the Lecture Hall of Kavli IPMU, The University of Tokyo, Kashiwanoha Campus (5-1-5, Kashiwanoha, Kashiwa-shi, Chiba, 277-8584, Japan).

Online Venue

This symposium will be held in a hybrid format. Details will be announced soon.

Organizers

  • Shigeki Matsumoto (chair, IPMU)
  • Elisa Ferreira (chair, IPMU)
  • Ippei Obata (chair, IPMU)
  • Kento Asai (ICRR)
  • Andrew Eberhardt (IPMU)
  • Kohei Hayashi (Sendai)
  • Anamaria Hell (IPMU)
  • Nagisa Hiroshima (YNU)
  • Shunichi Horigome (IPMU)
  • Qiuyue Liang (IPMU)
  • Maria Mylova (IPMU)
  • Tadayuki Takahashi (IPMU)

Sponsors

WPI logo IPMU logo

This symposium is supported in part by:

  • MEXT Grant-in-Aid for Scientific Research (A)
    • 20H00153 for Tadayuki Takahashi (PI), Shigeki Matsumoto (co-PI)
    • 24H00244 for Tadayuki Takahashi (PI)
  • MEXT Grant-in-Aid for Scientific Research (B)
    • 20H01895 for Shigeki Matsumoto (PI), Kohei Hayashi (co-PI)
  • MEXT Grant-in-Aid for Scientific Research (Early-Career Scientists)
  • MEXT Grant-in-Aid for Transformative Research Area A (Open-solicited Research)
Starts
Ends
Asia/Tokyo
Kavli IPMU
Lecture Hall
Kavli Institute for the Physics and Mathematics of the Universe, The University of Tokyo 5-1-5 Kashiwanoha, Kashiwa, Chiba, 277-8583, Japan
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Registration
Registration for this event is currently open.
The call for abstracts is open
You can submit an abstract for reviewing.