A Abusleme, T Adam, S Ahmad, R Ahmed… - arXiv preprint arXiv …, 2021 - arxiv.org
The Jiangmen Underground Neutrino Observatory (JUNO) is a 20 kton LS detector at 700-m underground. An excellent energy resolution and a large fiducial volume offer exciting …
F An, G An, Q An, V Antonelli, E Baussan… - Journal of Physics G …, 2016 - iopscience.iop.org
Abstract The Jiangmen Underground Neutrino Observatory (JUNO), a 20 kton multi-purpose underground liquid scintillator detector, was proposed with the determination of the neutrino …
A Mirizzi, I Tamborra, HT Janka, N Saviano… - La Rivista del Nuovo …, 2016 - Springer
Neutrinos play a crucial role in the collapse and explosion of massive stars, governing the infall dynamics of the stellar core, triggering and fueling the explosion and driving the …
This review demonstrates the unique role of the neutrino by discussing in detail the physics of and with neutrinos. We deal with neutrino sources, neutrino oscillations, absolute masses …
C Giunti, YF Li, CA Ternes, Z Xin - Physics Letters B, 2022 - Elsevier
We study the status of the reactor antineutrino anomaly in light of recent reactor flux models obtained with the conversion and summation methods. We present a new improved …
K Abe, C Bronner, Y Hayato, K Hiraide, M Ikeda… - Physical Review D, 2021 - APS
We have conducted a new search for the diffuse supernova neutrino background (DSNB) flux at Super-Kamiokande (SK), with a 22.5× 2970-kton· day exposure from its fourth …
T Sato, Y Iwamoto, S Hashimoto, T Ogawa… - Journal of Nuclear …, 2024 - Taylor & Francis
ABSTRACT The Particle and Heavy Ion Transport code System (PHITS) is a general- purpose Monte Carlo radiation transport code that can simulate the behavior of most particle …
The next core-collapse supernova in the Milky Way or its satellites will represent a once-in-a- generation opportunity to obtain detailed information about the explosion of a star and …
M Harada, K Abe, C Bronner, Y Hayato… - The Astrophysical …, 2023 - iopscience.iop.org
We report the first search result for the flux of astrophysical electron antineutrinos for energies () 10 MeV in the gadolinium-loaded Super-Kamiokande (SK) detector. In 2020 …