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nuLC Collaboration
NUMERICAL SIMULATIONS
How do neutron stars cool?
ANALYTIC SOLUTIONS
How can we describe?
DATA ANALYSIS
How shall we understand?
What do we achieve?
"Observing Supernova Neutrino Light Curves with Super-Kamiokande. IV. Development of SPECIAL BLEND: A New Public Analysis Code for Supernova Neutrinos",
Harada, A., Suwa, Y., Harada, M., Koshio, Y., Mori, M., Nakanishi, F., Nakazato, K., Sumiyoshi, K., Wendell, R. A., The Astrophysical Journal, 954, 52 (2023)."Observing Supernova Neutrino Light Curves with Super-Kamiokande. III. Extraction of Mass and Radius of Neutron Stars from Synthetic Data",
Suwa, Y., Harada, A., Harada, M., Koshio, Y., Mori, M., Nakanishi, F., Nakazato, K., Sumiyoshi, K., Wendell, R. A., The Astrophysical Journal, 934, 15 (2022)."Observing Supernova Neutrino Light Curves with Super-Kamiokande. II. Impact of the Nuclear Equation of State",
Nakazato, K., Nakanishi, F., Harada, M., Koshio, Y., Suwa, Y., Sumiyoshi, K., Harada, A., Mori, M., Wendell, R. A., The Astrophysical Journal, 925, 98 (2022)."Developing an end-to-end simulation framework of supernova neutrino detection",
Mori, M., Suwa, Y., Nakazato, K., Sumiyoshi, K., Harada, M., Harada, A., Koshio, Y., Wendell, R. A., Progress of Theoretical and Experimental Physics, 2021, 023E01 (2021)."Analytic solutions for neutrino-light curves of core-collapse supernovae",
Suwa, Y., Harada, A., Nakazato, K., Sumiyoshi, K., Progress of Theoretical and Experimental Physics, 2021, 013E01 (2021)."Observing Supernova Neutrino Light Curves with Super-Kamiokande: Expected Event Number over 10 s",
Suwa, Y., Sumiyoshi, K., Nakazato, K., Takahira, Y., Koshio, Y., Mori, M., Wendell, R. A., The Astrophysical Journal, 881, 139 (2019).
Resources
Who are we?
(as of May. 2024)
Ryuichiro Akaho (Waseda U)
Akira Harada (NIT, Ibaraki)
Masayuki Harada (ICRR)
Yusuke Koshio (Okayama U)
Masamitsu Mori (NAOJ)
Fumi Nakanishi (Okayama U)
Ken'ichiro Nakazato (Kyushu U)
Kohsuke Sumiyoshi (NIT, Numazu)
Yudai Suwa (U of Tokyo)
Roger Wendell (Kyoto U)