Cover Image

Limits on the Low-Energy Electron Antineutrino Flux from the Brightest GRB of All Time

Fuente: arXiv

Saved in:

Bibliographic Details
Main Authors:	Araki, T., Chauhan, S., Chiba, K., Eda, T., Eizuka, M., Funahashi, Y., Furuto, A., Gando, A., Gando, Y., Goto, S., Hachiya, T., Hata, K., Ichimura, K., Ikeda, H., Inoue, K., Ishidoshiro, K., Kamei, Y., Kawada, N., Kishimoto, Y., Koga, M., Marthe, A., Matsumoto, Y., Mitsui, T., Miyake, H., Morita, D., Nakajima, R., Nakamura, K., Nakamura, R., Nakane, J., Ono, T., Ozaki, H., Saito, K., Sakai, T., Shimizu, I., Shirai, J., Shiraishi, K., Suzuki, A., Tachibana, K., Tamae, K., Watanabe, H., Watanabe, K., Kurosawa, S., Urano, Y., Yoshida, S., Umehara, S., Fushimi, K., Kotera, K., Berger, B. E., Fujikawa, B. K., Learned, J. G., Maricic, J., Fu, Z., Ghosh, S., Smolsky, J., Winslow, L. A., Efremenko, Y., Karwowski, H. J., Markoff, D. M., Tornow, W., Delloro, S., Odonnell, T., Detwiler, J. A., Enomoto, S., Decowski, M. P., Weerman, K. M., Grant, C., Penek, Ö., Song, H., Li, A., Axani, S. N., Garcia, M., Sarfraz, M.
Format:	Preprint
Published:	2024
Subjects:	High Energy Astrophysical Phenomena
Online Access:	Acceder al recurso
Tags:	Add Tag No Tags, Be the first to tag this record!

_version_	1866910659658121216
author	Araki, T. Chauhan, S. Chiba, K. Eda, T. Eizuka, M. Funahashi, Y. Furuto, A. Gando, A. Gando, Y. Goto, S. Hachiya, T. Hata, K. Ichimura, K. Ikeda, H. Inoue, K. Ishidoshiro, K. Kamei, Y. Kawada, N. Kishimoto, Y. Koga, M. Marthe, A. Matsumoto, Y. Mitsui, T. Miyake, H. Morita, D. Nakajima, R. Nakamura, K. Nakamura, R. Nakamura, R. Nakane, J. Ono, T. Ozaki, H. Saito, K. Sakai, T. Shimizu, I. Shirai, J. Shiraishi, K. Suzuki, A. Tachibana, K. Tamae, K. Watanabe, H. Watanabe, K. Kurosawa, S. Urano, Y. Yoshida, S. Umehara, S. Fushimi, K. Kotera, K. Berger, B. E. Fujikawa, B. K. Learned, J. G. Maricic, J. Fu, Z. Ghosh, S. Smolsky, J. Winslow, L. A. Efremenko, Y. Karwowski, H. J. Markoff, D. M. Tornow, W. Delloro, S. Odonnell, T. Detwiler, J. A. Enomoto, S. Decowski, M. P. Weerman, K. M. Grant, C. Penek, Ö. Song, H. Li, A. Axani, S. N. Garcia, M. Sarfraz, M.
author_facet	Araki, T. Chauhan, S. Chiba, K. Eda, T. Eizuka, M. Funahashi, Y. Furuto, A. Gando, A. Gando, Y. Goto, S. Hachiya, T. Hata, K. Ichimura, K. Ikeda, H. Inoue, K. Ishidoshiro, K. Kamei, Y. Kawada, N. Kishimoto, Y. Koga, M. Marthe, A. Matsumoto, Y. Mitsui, T. Miyake, H. Morita, D. Nakajima, R. Nakamura, K. Nakamura, R. Nakamura, R. Nakane, J. Ono, T. Ozaki, H. Saito, K. Sakai, T. Shimizu, I. Shirai, J. Shiraishi, K. Suzuki, A. Tachibana, K. Tamae, K. Watanabe, H. Watanabe, K. Kurosawa, S. Urano, Y. Yoshida, S. Umehara, S. Fushimi, K. Kotera, K. Berger, B. E. Fujikawa, B. K. Learned, J. G. Maricic, J. Fu, Z. Ghosh, S. Smolsky, J. Winslow, L. A. Efremenko, Y. Karwowski, H. J. Markoff, D. M. Tornow, W. Delloro, S. Odonnell, T. Detwiler, J. A. Enomoto, S. Decowski, M. P. Weerman, K. M. Grant, C. Penek, Ö. Song, H. Li, A. Axani, S. N. Garcia, M. Sarfraz, M.
contents	The electron antinuetrino flux limits are presented for the brightest gamma-ray burst (GRB) of all time, GRB221009A, over a range of 1.8-200 MeV using the Kamioka Liquid Scintillator Anti Neutrino Detector (KamLAND). Using a variety of time windows to search for electron antineutrinos coincident with the GRB, we set an upper limit on the flux under the assumption of various neutrino source spectra. No excess was observed in any time windows ranging from seconds to days around the event trigger time. The limits are compared to the results presented by IceCube.
format	Preprint
id	arxiv_https___arxiv_org_abs_2410_01996
institution	arXiv
publishDate	2024
record_format	arxiv
spellingShingle	Limits on the Low-Energy Electron Antineutrino Flux from the Brightest GRB of All Time Araki, T. Chauhan, S. Chiba, K. Eda, T. Eizuka, M. Funahashi, Y. Furuto, A. Gando, A. Gando, Y. Goto, S. Hachiya, T. Hata, K. Ichimura, K. Ikeda, H. Inoue, K. Ishidoshiro, K. Kamei, Y. Kawada, N. Kishimoto, Y. Koga, M. Marthe, A. Matsumoto, Y. Mitsui, T. Miyake, H. Morita, D. Nakajima, R. Nakamura, K. Nakamura, R. Nakamura, R. Nakane, J. Ono, T. Ozaki, H. Saito, K. Sakai, T. Shimizu, I. Shirai, J. Shiraishi, K. Suzuki, A. Tachibana, K. Tamae, K. Watanabe, H. Watanabe, K. Kurosawa, S. Urano, Y. Yoshida, S. Umehara, S. Fushimi, K. Kotera, K. Berger, B. E. Fujikawa, B. K. Learned, J. G. Maricic, J. Fu, Z. Ghosh, S. Smolsky, J. Winslow, L. A. Efremenko, Y. Karwowski, H. J. Markoff, D. M. Tornow, W. Delloro, S. Odonnell, T. Detwiler, J. A. Enomoto, S. Decowski, M. P. Weerman, K. M. Grant, C. Penek, Ö. Song, H. Li, A. Axani, S. N. Garcia, M. Sarfraz, M. High Energy Astrophysical Phenomena The electron antinuetrino flux limits are presented for the brightest gamma-ray burst (GRB) of all time, GRB221009A, over a range of 1.8-200 MeV using the Kamioka Liquid Scintillator Anti Neutrino Detector (KamLAND). Using a variety of time windows to search for electron antineutrinos coincident with the GRB, we set an upper limit on the flux under the assumption of various neutrino source spectra. No excess was observed in any time windows ranging from seconds to days around the event trigger time. The limits are compared to the results presented by IceCube.
title	Limits on the Low-Energy Electron Antineutrino Flux from the Brightest GRB of All Time
topic	High Energy Astrophysical Phenomena
url	https://arxiv.org/abs/2410.01996