KamLAND

(KAMioka Liquid scintillator Anti-Neutrino Detector)

Other Web pages: LBL, Hawaii, Stanford, INSPIRE

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References

1 - Reviews

[1-1]
Antineutrino Science in KamLAND, Atsuto Suzuki, Eur.Phys.J. C74 (2014) 3094, arXiv:1409.4515.
[Suzuki:2014woa]

2 - Habilitation, PhD and Master Theses

[2-1]
Measurement of neutrino oscillation with KamLAND, Jason A. Detwiler, 2005. UMI-31-62394. http://kamland.stanford.edu/TalksAndPublications/DetwilerThesis.pdf.
[Detwiler:2005hj]

3 - Neutrino Oscillations

[3-1]
Reactor On-Off Antineutrino Measurement with KamLAND, A. Gando et al. (KamLAND), Phys. Rev. D88 (2013) 033001, arXiv:1303.4667.
[KamLAND:2013rgu]
[3-2]
Enhanced Constraints on $\theta_{13}$ from A Three-Flavor Oscillation Analysis of Reactor Antineutrinos at KamLAND, A. Gando et al. (KamLAND), Phys. Rev. D83 (2011) 052002, arXiv:1009.4771.
[KamLAND:2010fvi]
[3-3]
Precision Measurement of Neutrino Oscillation Parameters with KamLAND, S. Abe et al. (KamLAND), Phys. Rev. Lett. 100 (2008) 221803, arXiv:0801.4589.
From the article: The spectrum indicates almost two cycles of the periodic feature expected from neutrino oscillation.
[KamLAND:2008dgz]
[3-4]
Measurement of Neutrino Oscillation with KamLAND: Evidence of Spectral Distortion, T. Araki et al. (KamLAND), Phys. Rev. Lett. 94 (2005) 081801, arXiv:hep-ex/0406035.
[KamLAND:2004mhv]
[3-5]
First Results from KamLAND: Evidence for Reactor Anti-Neutrino Disappearance, K. Eguchi et al. (KamLAND), Phys. Rev. Lett. 90 (2003) 021802, arXiv:hep-ex/0212021.
[KamLAND:2002uet]

4 - Solar Neutrinos

[4-1]
Search for Solar Flare Neutrinos with the KamLAND detector, S. Abe et al. (KamLAND), Astrophys.J. 924 (2022) 103, arXiv:2105.02458.
[KamLAND:2021sda]
[4-2]
7Be Solar Neutrino Measurement with KamLAND, A. Gando et al. (KamLAND), Phys.Rev. C92 (2015) 055808, arXiv:1405.6190.
[KamLAND:2014gul]
[4-3]
Measurement of the 8B Solar Neutrino Flux with KamLAND, S. Abe et al. (KamLAND), Phys. Rev. C84 (2011) 035804, arXiv:1106.0861.
[KamLAND:2011fld]
[4-4]
A High Sensitivity Search for $\bar{\nu}_{e}$'s from the Sun and Other Sources at KamLAND, K. Eguchi et al. (KamLAND), Phys. Rev. Lett. 92 (2004) 071301, arXiv:hep-ex/0310047.
[KamLAND:2003gfh]

5 - Geo-Neutrinos

[5-1]
Abundances of uranium and thorium elements in Earth estimated by geoneutrino spectroscopy, S. Abe et al. (KamLAND), arXiv:2205.14934, 2022.
[KamLAND:2022vbm]
[5-2]
Experimental investigation of geologically produced antineutrinos with KamLAND, T. Araki et al. (KamLAND), Nature 436 (2005) 499-503. http://www.nature.com/nature/journal/v436/n7050/abs/nature03980.html;jsessionid=2B54E1F6E002C96A8C0F0275FB860964.
From the article: ... a 'rate only' analysis gives $ 25 {}^{+19}_{-18} $ geoneutrino candidates from the $^{238}\text{U}$ and $^{232}\text{Th}$ decay chains. Dividing by the detection efficiency, live-time, and number of target protons, the total geoneutrino detected rate obtained is $ 5.1 {}^{+3.9}_{-3.6} \times 10^{-31} $ $\bar{\nu}_e$ per target proton per year.
...
The 99\% confidence upper limit obtained on the total detected $^{238}\text{U}$ and $^{232}\text{Th}$ geoneutrino rate is $ 1.45 \times 10^{-30} $ $\bar{\nu}_e$ per target proton per year, corresponding to a flux at KamLAND of $ 1.62 \times 10^7 \,\text{cm}^{-2} \,\text{s}^{-1}$. On the basis of our reference model, this corresponds to an upper limit on the radiogenic power from $^{238}\text{U}$ and $^{232}\text{Th}$ decay of 60 TW.

[KamLAND-Nature436-499-2005]

6 - Astrophysics

[6-1]
Search for Diffuse Supernova Neutrino Background in the Full KamLAND Dataset with Neural-Network-Based Event Classification, D. Chernyak et al., arXiv:2606.29381, 2026.
[Chernyak:2026xhc]
[6-2]
Limits on the Low-Energy Electron Antineutrino Flux from the Brightest GRB of All Time, T. Araki et al. (KamLAND), Astrophys.J. 981 (2025) 192, arXiv:2410.01996.
[KamLAND:2024bll]
[6-3]
Combined Pre-supernova Alert System with KamLAND and Super-Kamiokande, Seisho Abe et al. (KamLAND, Super-Kamiokande), Astrophys. J. 973 (2024) 140, arXiv:2404.09920.
[KamLAND:2024uia]
[6-4]
Search for supernova neutrinos and constraint on the galactic star formation rate with the KamLAND data, S. Abe et al. (KamLAND), Astrophys.J. 934 (2022) 85, arXiv:2204.12065.
[KamLAND:2022sqb]
[6-5]
KamLAND's search for correlated low-energy electron antineutrinos with astrophysical neutrinos from IceCube, S. Abe et al. (KamLAND), Astropart.Phys. 143 (2022) 102758, arXiv:2202.07345.
[Abe:2022ovx]
[6-6]
A search for correlated low-energy electron antineutrinos in KamLAND with \gamma-ray bursts, S. Abe et al. (KamLAND), Astrophys.J. 927 (2022) 69, arXiv:2112.04918.
[KamLAND:2021osm]
[6-7]
Limits on astrophysical antineutrinos with the KamLAND experiment, S. Abe et al. (KamLAND), Astrophys.J. 925 (2022) 14, arXiv:2108.08527.
[KamLAND:2021gvi]
[6-8]
Search for Low-energy Electron Antineutrinos in KamLAND Associated with Gravitational Wave Events, S. Abe et al. (KamLAND), Astrophys.J. 909 (2021) 116, arXiv:2012.12053.
[KamLAND:2020ses]
[6-9]
Search for electron antineutrinos associated with gravitational wave events GW150914 and GW151226 using KamLAND, A. Gando et al. (KamLAND), Astrophys.J. 829 (2016) L34, arXiv:1606.07155.
[KamLAND:2016wvk]
[6-10]
Study of electron anti-neutrinos associated with \gamma-ray bursts using KamLAND, K. Asakura et al. (KamLAND), Astrophys.J. 806 (2015) 87, arXiv:1503.02137.
[KamLAND:2015zyu]
[6-11]
A study of extraterrestrial antineutrino sources with the KamLAND detector, A. Gando et al. (KamLAND), Astrophys. J. 745 (2012) 193, arXiv:1105.3516.
[KamLAND:2011bnd]

7 - Double Beta Decay

[7-1]
Search for Majorana Neutrinos with the Complete KamLAND-Zen Dataset, S. Abe et al., Phys.Rev.Lett. 135 (2025) 262501, arXiv:2406.11438.
[KamLAND-Zen:2024eml]
[7-2]
First Search for the Majorana Nature of Neutrinos in the Inverted Mass Ordering Region with KamLAND-Zen, S. Abe et al. (KamLAND-Zen), Phys.Rev.Lett. 130 (2023) 051801, arXiv:2203.02139.
[KamLAND-Zen:2022tow]
[7-3]
Precision measurement of the $^{136}$Xe two-neutrino $\beta\beta$ spectrum in KamLAND-Zen and its impact on the quenching of nuclear matrix elements, A. Gando et al. (KamLAND-Zen), Phys.Rev.Lett. 122 (2019) 192501, arXiv:1901.03871.
[KamLAND-Zen:2019imh]
[7-4]
Search for Majorana Neutrinos near the Inverted Mass Hierarchy region with KamLAND-Zen, A. Gando et al. (KamLAND-Zen), Phys. Rev. Lett. 117 (2016) 082503, arXiv:1605.02889.
[KamLAND-Zen:2016pfg]
[7-5]
Limit on Neutrinoless $\beta\beta$ Decay of Xe-136 from the First Phase of KamLAND-Zen and Comparison with the Positive Claim in Ge-76, A. Gando et al. (KamLAND-Zen), Phys. Rev. Lett. 110 (2013) 062502, arXiv:1211.3863.
[KamLAND-Zen:2012mmx]
[7-6]
Limits on Majoron-Emitting Double-Beta Decays of Xe-136 in KamLAND-Zen, A. Gando et al. (KamLAND-Zen), Phys. Rev. C86 (2012) 021601, arXiv:1205.6372.
[KamLAND-Zen:2012uen]
[7-7]
Measurement of the Double-Beta Decay Half-life of $^{136}$Xe in KamLAND-Zen, KamLAND-Zen (KamLAND-Zen), Phys. Rev. C85 (2012) 045504, arXiv:1201.4664.
[KamLAND-Zen:2012vpv]

8 - Double Beta Decay - Talks

[8-1]
Results from KamLAND-Zen, K. Asakura et al. (KamLAND-Zen), AIP Conf. Proc. 1666 (2015) 170003, arXiv:1409.0077. XXVI Conference on Neutrino Physics and Astrophysics (Neutrino 2014).
[KamLAND-Zen:2014hhc]
[8-2]
First result from KamLAND-Zen : Double $\beta$ decay with 136-Xe, A. Gando (KamLAND-Zen), arXiv:1205.6130, 2012. Moriond 2012 EW session.
[Gando:2012jr]

9 - Physics

[9-1]
First measurement of the strange axial coupling constant using neutral-current quasi-elastic interactions of atmospheric neutrinos at KamLAND, S. Abe et al. (KamLAND), Phys.Rev.D 107 (2023) 072006, arXiv:2211.13911.
[KamLAND:2022ptk]
[9-2]
Search for the Proton Decay Mode $p \rightarrow \overline\nu K^{+}$ with KamLAND, K. Asakura et al. (KamLAND-Zen), Phys. Rev. D92 (2015) 052006, arXiv:1505.03612.
[KamLAND:2015pvi]
[9-3]
Study of the Production of Radioactive Isotopes through Cosmic Muon Spallation in KamLAND, S. Abe et al. (KamLAND), Phys. Rev. C81 (2010) 025807, arXiv:0907.0066.
[KamLAND:2009zwo]
[9-4]
Search for the invisible decay of neutrons with KamLAND, T. Araki et al. (KamLAND), Phys. Rev. Lett. 96 (2006) 101802, arXiv:hep-ex/0512059.
[KamLAND:2005pen]

10 - Neutrino Flux

[10-1]
A simple model of reactor cores for reactor neutrino flux calculations for the KamLAND experiment, K. Nakajima et al., Nucl.Instrum.Meth. A569 (2006) 837-844, arXiv:physics/0607126.
[Nakajima:2006re]

11 - Detector

[11-1]
Real-time Position Reconstruction for the KamLAND-Zen Experiment using Hardware-AI Co-design, Alexander Migala, Eugene Ku, Zepeng Li, Aobo Li, arXiv:2410.02991, 2024.
[Migala:2024ael]
[11-2]
KamNet: An Integrated Spatiotemporal Deep Neural Network for Rare Event Search in KamLAND-Zen, Aobo Li, Zhenghao Fu, Lindley A. Winslow, Christopher P. Grant, Hasung Song, Hideyoshi Ozaki, Itaru Shimizu, Atsuto Takeuchi, Phys.Rev.C 107 (2023) 014323, arXiv:2203.01870.
[Li:2022frp]
[11-3]
The nylon balloon for xenon loaded liquid scintillator in KamLAND-Zen 800 neutrinoless double-$\beta$ decay search experiment, Y. Gando et al. (KamLAND-Zen), JINST 16 () P08023, arXiv:2104.10452.
[KamLAND-Zen:2021aha]
[11-4]
A compact ultra-clean system for deploying radioactive sources inside the KamLAND detector, T.I. Banks et al., Nucl.Instrum.Meth. A769 (2014) 88-96, arXiv:1407.0413.
[Banks:2014hra]
[11-5]
The KamLAND Full-Volume Calibration System, B.E. Berger et al. (KamLAND), JINST 4 (2009) P04017, arXiv:0903.0441.
[KamLAND:2009ply]
[11-6]
A C-13(\alpha,n)O-16 calibration source for KamLAND, David W. McKee, Jerome K. Busenitz, Igor Ostrovskiy, Nucl. Instrum. Meth. A587 (2008) 272-276, arXiv:0711.3624.
[McKee:2007bk]
[11-7]
Online monitoring system and data management for KamLAND, M.Motoki, F.Suekane, K.Tada, Y.Tsuda, Nucl. Instrum. Meth. A534 (2004) 59, arXiv:hep-ex/0405074.
[Motoki:2004ci]

12 - Sterile Neutrinos

[12-1]
IsoDAR@KamLAND:A Conceptual Design Report for the Conventional Facilities, Jose R. Alonso (IsoDAR), arXiv:1710.09325, 2017.
[Alonso:2017fci]
[12-2]
IsoDAR@KamLAND: A Conceptual Design Report for the Technical Facility, M. Abs et al., arXiv:1511.05130, 2015.
[Abs:2015tbh]

13 - Background

[13-1]
Measurement of cosmic-ray muon spallation products in a xenon-loaded liquid scintillator with KamLAND, S. Abe et al. (KamLAND-Zen), Phys.Rev.C 107 (2023) 054612, arXiv:2301.09307.
[KamLAND-Zen:2023spw]
[13-2]
Muon Simulations for Super-Kamiokande, KamLAND and CHOOZ, Alfred Tang, Glenn Horton-Smith, Vitaly A. Kudryavtsev, Alessandra Tonazzo, Phys. Rev. D74 (2006) 053007, arXiv:hep-ph/0604078.
[Tang:2006uu]

14 - Proposal

[14-1]
Proposal for US Participation in KamLAND, J. Busenitz et al., 1999. http://kamland.lbl.gov/TalksPaper/Papers/KamLAND.US.Proposal.pdf.
[Proposal-US-Participation-KamLAND-1999]

15 - Talks

[15-1]
Recent Results from KamLAND, Koichi Ichimura, for the KamLAND Collaboration (KamLAND), arXiv:0810.3448, 2008. ICHEP08.
[Ichimura:2008km]
[15-2]
High Sensitivity Anti-Neutrino Detection by KamLAND, S. Hatakeyama et al. (KamLAND), arXiv:hep-ex/0405001, 2004. Moriond EW04.
[Hatakeyama:2004gm]
[15-3]
An Overview of the KamLAND 1-kiloton Liquid Scintillator, F. Suekane et al., arXiv:physics/0404071, 2004. 'KEK-RCNP International School and Mini-Workshop for Scintillating Crystals and their Applications in Particle and Nuclear Physics'. (Nov. 17-18, 2003, KEK, Japan).
[Suekane:2004ny]
[15-4]
Results from the KamLAND experiment, G. Gratta (KamLAND), 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/monday/gratta.pdf.
[Gratta-Nu2004]
[15-5]
KamLAND: updated results, K. Inoue, 2004. Neutrino Oscillation Workshop NOW 2004, September 11-17, 2004, Conca Specchiulla (Otranto, Italy). http://www.ba.infn.it/~now2004/talks/12_09_04/plen/KamLAND.pdf.
[Inoue:2004]
[15-6]
Recent Results from KamLAND, J. Detwiler (KamLAND), eConf C0307282 (2003) TW04, arXiv:hep-ex/0311007. SLAC Summer Institute, July 2003.
[Detwiler:2003fb]
[15-7]
KamLAND results, K. Inoue, arXiv:hep-ex/0307030, 2003. XXXVIII Rencontres de Moriond on Electroweak Interactions and Unified Theories Les Arcs, France, 15-22 March 2003.
[Inoue:2003qs]
[15-8]
KamLAND Results, K. Inoue, 2003. The 4th Workshop on Neutrino Oscillations and their Origin (NOON2003), February 10-14, 2003, Ishikawa Kousei Nenkin Kaikan, Kanazawa, Japan. http://www-sk.icrr.u-tokyo.ac.jp/noon2003/transparencies/10/Inoue-KamLAND.pdf.
[Inoue:NOON2003]
[15-9]
First KamLAND Results, Y. Kamyshkov, 2003. IV INTERNATIONAL CONFERENCE on NON-ACCELERATOR NEW PHYSICS - NANP 2003 - Dubna, Russia, June 23-28, 2003. http://nanp.dubna.ru/talks/kamyshkov.pdf.
Comment: Slide n. 41 shows comparison of data (13 bins) with 2-$\nu$ oscillation, best fit $\chi^2 = 2.8$, and with no oscillation - constant flux suppression, $\chi^2 = 5.3$. (M.L.).
[Kamyshkov:NANP2003]
[15-10]
An update on progress at KamLAND, S. A. Dazeley (KamLAND), arXiv:hep-ex/0205041, 2002.
[Dazeley:2002yf]
[15-11]
The KamLAND detector and backgrounds for solar neutrino detection, K. Furuno, 2002. IIIrd International Workshop on Low Energy Solar Neutrinos - LOW NU 2002, 22-24 May 2002, Heidelberg, Germany. http://www.mpi-hd.mpg.de/nubis/www_lownu2002/transparency/furuno_lownu_2002.pdf.
[Furuno-LowNu2002]
[15-12]
First Results from KamLAND: Evidence for \bar{\nu}_e$ disappearance, G. Gratta (Kamland), 2002. SLAC Colloquium, December 2002. http://hep.stanford.edu/neutrino/KamLAND/TalksAndPublications/KamLAND_FirstResults_SLAC_Colloq.pdf.
[Gratta:SLAC2002]
[15-13]
Start of Kamland, J. Shirai (Kamland), 2002. TXXth International Conference on Neutrino Physics and Astrophysics May 25 - 30, 2002, Munich, Germany. http://neutrino2002.ph.tum.de/pages/transparencies/suzuki.
[Shirai-Nu2002]
[15-14]
Status of KAMLAND Project, F. Suekane (Kamland), 2002. Conference on Physics beyond the Standard Model - BEYOND THE DESERT 02 - Oulu, Finland, 2-7 June 2002. http://cupp.oulu.fi/trans/Suekane.pdf.
[Suekane-Oulu2002]
[15-15]
KamLAND: Examination of the LMA solution with reactor neutrinos, A. Suzuki (Kamland), 2002. XVI International Conference on Particles and Nuclei, Osaka, Japan, September 30 - October 4, 2002. http://www.rcnp.osaka-u.ac.jp/Divisions/np2/PaNic02/Suzuki.pdf.
[Suzuki-Panic02]
[15-16]
Commissioning the KamLAND experiment, N. Tolik, 2002. The April Meeting 2002 of the American Physical Society. http://www.awa.tohoku.ac.jp/KamLAND/APS_April2002.pdf.
[Tolik-APS2002]
[15-17]
Kamland, j. Goldman, 2001. 3rd Workshop on Neutrino Oscillations and their Origin: NOON01. http://www-sk.icrr.u-tokyo.ac.jp/noon2001/transparency/dec05/goldman/goldman.pdf.
[Goldman-talk:2001a]
[15-18]
Kamland, K. Ishihara, 2001. The Third International Workshop on Neutrino Factories based on Muon Storage Rings (NuFACT'01) May 24th - May 30th, 2001, Tsukuba, Japan. http://www-prism.kek.jp/nufact01/May26/WG1/26wg1_ishihara.pdf.
[Ishihara-NuFACT01]
[15-19]
KamLAND: A reactor neutrino experiment testing the solar neutrino anomaly, A. Piepke (KamLAND), Nucl. Phys. Proc. Suppl. 91 (2001) 99-104.
[Piepke:2001tg]
[15-20]
Neutrino physics with the KamLAND detector, L. De Braeckeleer (KamLAND), Nucl. Phys. Proc. Suppl. 87 (2000) 312-314.
[DeBraeckeleer:2000eu]
[15-21]
The present status of KamLAND, A. Suzuki (KamLAND), Nucl. Phys. Proc. Suppl. 77 (1999) 171-176.
[Suzuki:1999dg]
[15-22]
KamLAND experiment: Exploring low energy neutrino physics, J. Shirai, 1998.
[Shirai:1998gr]
[15-23]
Physics opportunities with the KamLAND experiment, Yi Fang Wang (KamLAND), 1998. Talk given at 29th International Conference on High-Energy Physics (ICHEP 98), Vancouver, Canada, 23-29 Jul 1998.
[Wang:1998jr]
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Neutrino Unbound Home

Authors:
Stefano Gariazzo / gariazzo@to.infn.it
Carlo Giunti / giunti@to.infn.it
Marco Laveder / marco.laveder@pd.infn.it
Last Update: Thu 15 Oct 2026, 12:29:52 CET