activity
20022025
most citedFirst Results from KamLAND: Evidence for Reactor Anti-Neutrino Disappearance

2.7k citations · 7.5k across the 32 of their papers we have counts for

collaborators

32 papers

physics.ins-det2025

Background stability and annual modulation test using PICOLON ultra-pure NaI(Tl) detector

PICOLON Collaboration, K. Kotera, D. Chernyak +20

The dark matter observation claimed by the DAMA/LIBRA experiment has been a long-standing puzzle within the particle physics community. NaI(Tl) crystals with radiopurity comparable…

astro-ph.IM2024★ 1 cited

Present status of PICOLON project

K. Fushimi, D. Chernyak, H. Ejiri +24

The existence of cosmic dark matter and neutrino properties are long-standing problems in cosmology and particle physics. These problems have been investigated by using radiation d…

physics.ins-det2023★ 1 cited

Radiopurity of NaI(Tl) crystals for PICOLON dark matter experiment

K. Kotera, D. Chernyak, H. Ejiri +19

The dark matter observation claim by the DAMA/LIBRA collaboration has been a long-standing puzzle within the particle physics community. Efforts of other research groups to verify…

hep-ex2022★ 243 cited

Search for the Majorana Nature of Neutrinos in the Inverted Mass Ordering Region with KamLAND-Zen

Zen Collaboration, S. Abe, S. Asami +70

The KamLAND-Zen experiment has provided stringent constraints on the neutrinoless double-beta () decay half-life in Xe using a xenon-loaded liquid scintillator. We re…

astro-ph.IM2021★ 7 cited

PICOLON dark matter search project

K. Fushimi, D. Chernyak, H. Ejiri +21

PICOLON (Pure Inorganic Crystal Observatory for LOw-energy Neutr(al)ino) aims to search for cosmic dark matter by high purity NaI(Tl) scintillator. We developed extremely pure NaI(…

astro-ph.HE2021★ 44 cited

Limits on astrophysical antineutrinos with the KamLAND experiment

S. Abe, S. Asami, A. Gando +66

We report on a search for electron antineutrinos () from astrophysical sources in the neutrino energy range 8.3 to 30.8 MeV with the KamLAND detector. In an exposure of 6.…