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Supernova relic neutrino search at super-Kamiokande

Authors :
P. Mijakowski
K. Martens
G. Mitsuka
Michael Litos
Yoshitaka Itow
K. Ueshima
T. Tanaka
Y. Takeuchi
J. G. Learned
Song Chen
L. Marti
Y. Takenaga
Joshua Hignight
Yoshihiro Suzuki
M. Dziomba
S. Nakayama
R. A. Wendell
M. Miura
L. R. Sulak
J. Imber
A. T. Suzuki
T. McLachlan
C. Regis
Y. Totsuka
T. Nakadaira
M. B. Smy
Hirokazu Ishino
Koh Ueno
T. Wongjirad
J. L. Raaf
A. L. Renshaw
J. S. Jang
Makoto Sakuda
Atsushi Takeda
T. Iida
K. Connolly
H. W. Sobel
Y. Heng
C. W. Walter
H. Toyota
A. Minamino
I. Taylor
A. Kibayashi
K. S. Ganezer
M. Miyake
T. Tsukamoto
Yuichi Oyama
Hiroyuki Sekiya
John Hill
M. R. Vagins
Y. Fukuda
S. Moriyama
Masayuki Nakahata
K. Abe
T. Yokozawa
Y. Obayashi
K. Sakashita
A. Murakami
W. E. Keig
B. S. Yang
T. Ishida
I. T. Lim
K. P. Lee
H. Kaji
K. Nishikawa
T. Ishii
C. Yanagisawa
M. Koshiba
Ko Okumura
E. Kearns
Kodai Matsuoka
K. Nishijima
W. R. Kropp
Masashi Yokoyama
S. Yamada
T. Ishizuka
Tsuyoshi Nakaya
R. J. Wilkes
L. Labarga
T. Kobayashi
C. K. Jung
H. Okazawa
M. Ikeda
Masato Shiozawa
Y. Choi
Takaaki Kajita
Zishuo Yang
Kate Scholberg
Haoxiong Zhang
S. Matsuno
Shigeki Tasaka
S. Mine
Takehisa Hasegawa
Justin Albert
Y. Kuno
S. Mino
K. Iyogi
S. N. Smith
Takaaki Mori
J. L. Stone
K. Kaneyuki
Koji Nakamura
T. Sekiguchi
K. Bays
Y. Hayato
Sunghoon Cho
Yusuke Koshio
S. B. Kim
J. Y. Kim
J. Kameda
UAM. Departamento de Física Teórica
Source :
Biblos-e Archivo. Repositorio Institucional de la UAM, instname
Publication Year :
2012

Abstract

Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM<br />A new Super-Kamiokande search for supernova relic neutrinos was conducted using 2853 live days of data. Sensitivity is now greatly improved compared to the 2003 Super-Kamiokande result, which placed a flux limit near many theoretical predictions. This more detailed analysis includes a variety of improvements such as increased efficiency, a lower energy threshold, and an expanded data set. New combined upper limits on supernova relic neutrino flux are between 2.8 and 3.1ν̄e cm-2 s-1 > 16 MeV total positron energy (17.3 MeV Eν)<br />The Super-Kamiokande experiment has been built and operated from funding by the Japanese Ministry of Education, Culture, Sports, Science and Technology, the United States Department of Energy, and the U.S. National Science Foundation. Some of us have been supported by funds from the Korean Research Foundation (BK21), the National Research Foundation of Korea (NRF- 20110024009), the Japan Society for the Promotion of Science, and the National Natural Science Foundation of China (Grants No. 10875062 and No. 10911140109)

Details

Database :
OpenAIRE
Journal :
Biblos-e Archivo. Repositorio Institucional de la UAM, instname
Accession number :
edsair.doi.dedup.....363b6e503cfd35084bd8ad836c5bc1e8