Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Roger A. Wendell"'
Autor:
Akira Harada, Yudai Suwa, Masayuki Harada, Yusuke Koshio, Masamitsu Mori, Fumi Nakanishi, Ken’ichiro Nakazato, Kohsuke Sumiyoshi, Roger A. Wendell
Publikováno v:
The Astrophysical Journal, Vol 954, Iss 1, p 52 (2023)
Supernova neutrinos are invaluable signals that offer information about the interior of supernovae. Because a nearby supernova can occur at any time, preparing for future supernova neutrino observation is an urgent task. For the prompt analysis of su
Externí odkaz:
https://doaj.org/article/0dc477a71d3a40b1b4f47302e80c9e91
Autor:
Yudai Suwa, Akira Harada, Masayuki Harada, Yusuke Koshio, Masamitsu Mori, Fumi Nakanishi, Ken’ichiro Nakazato, Kohsuke Sumiyoshi, Roger A. Wendell
Neutrinos are guaranteed to be observable from the next galactic supernova (SN). Optical light and gravitational waves are also observable, but may be difficult to observe if the location of the SN in the galaxy or the details of the explosion are un
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::290cbc08541cb021b58839d460217d41
http://arxiv.org/abs/2204.08363
http://arxiv.org/abs/2204.08363
Autor:
Ken’ichiro Nakazato, Fumi Nakanishi, Masayuki Harada, Yusuke Koshio, Yudai Suwa, Kohsuke Sumiyoshi, Akira Harada, Masamitsu Mori, Roger A. Wendell
The late-time evolution of the neutrino event rate from supernovae is evaluated for Super-Kamiokande using simulated results of proto-neutron star (PNS) cooling. In the present work we extend the result of Suwa et al. (2019) [arXiv:1904.09996], which
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::335e978482e1a10465ae72c878fe7b2c
http://arxiv.org/abs/2108.03009
http://arxiv.org/abs/2108.03009
Autor:
Yudai Suwa, Kohsuke Sumiyoshi, Ken’ichiro Nakazato, Yasufumi Takahira, Yusuke Koshio, Masamitsu Mori, Roger A. Wendell
Publikováno v:
Astrophysical Journal; 8/20/2019, Vol. 881 Issue 2, p1-1, 1p