Study of electron anti-neutrinos associated with gamma-ray bursts using KamLAND
K. Asakura, A. Gando, Y. Gando, T. Hachiya, S. Hayashida, H. Ikeda, K., Inoue, K. Ishidoshiro, T. Ishikawa, S. Ishio, M. Koga, S. Matsuda, T. Mitsui,, D. Motoki, K. Nakamura, S. Obara, Y. Oki, T. Oura, I. Shimizu, Y. Shirahata,, J. Shirai, A. Suzuki, H. Tachibana, K. Tamae

TL;DR
This study used KamLAND data from 2002 to 2013 to search for electron anti-neutrinos from gamma-ray bursts, setting new upper limits on their fluence and constraining their luminosity-temperature relation.
Contribution
It provides the first constraints on the relation between anti-neutrino luminosity and temperature from GRBs and sets the tightest upper limits on anti-neutrino fluence below 7 MeV.
Findings
No significant anti-neutrino excess detected.
Established the tightest upper limits on anti-neutrino fluence below 7 MeV.
First constraints on anti-neutrino luminosity-temperature relation from GRBs.
Abstract
We search for electron anti-neutrinos () from long and short-duration gamma-ray bursts~(GRBs) using data taken by the KamLAND detector from August 2002 to June 2013. No statistically significant excess over the background level is found. We place the tightest upper limits on fluence from GRBs below 7 MeV and place first constraints on the relation between luminosity and effective temperature.
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