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]
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]
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]
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]
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]
Abundances of uranium and thorium elements in Earth estimated by geoneutrino spectroscopy,
S. Abe et al.(KamLAND),
arXiv:2205.14934, 2022. [KamLAND:2022vbm]
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]
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]
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]
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]
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]
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]
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]
Limits on astrophysical antineutrinos with the KamLAND experiment,
S. Abe et al.(KamLAND),
Astrophys.J. 925 (2022) 14,arXiv:2108.08527.
[KamLAND:2021gvi]
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]
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]
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]
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]
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]
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]
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]
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]
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]
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]
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]
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]
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]
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]
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]
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]
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]
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]
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]
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]
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]
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]
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]
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]
Recent Results from KamLAND,
J. Detwiler(KamLAND),
eConf C0307282 (2003) TW04,arXiv:hep-ex/0311007.
SLAC Summer Institute, July 2003. [Detwiler:2003fb]
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]
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]
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]
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]
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]
KamLAND: A reactor neutrino experiment testing the solar neutrino anomaly,
A. Piepke(KamLAND),
Nucl. Phys. Proc. Suppl. 91 (2001) 99-104. [Piepke:2001tg]
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]