L. F. Thompson

collaborators

3 papers

hep-ex2026

Search for proton decay via $p \to e^{+} I ¨ ^{0} I ¨ ^{0}$ and $p \to I^¼^{+} I ¨ ^{0} I ¨ ^{0}$ in 0.401 megaton-years exposure of Super-Kamiokande I-V

Kamiokande Collaboration, K. Abe, S. Abe +310

We searched for proton decay via $p \to e^{+} I ¨ ^{0} I ¨ ^{0}$ and $p \to I^¼^{+} I ¨ ^{0} I ¨ ^{0}$ in 0.401 megaton-years of data collected in all pure water detector phases of Super-Kamiok…

astro-ph.IM2024

Development of a data overflow protection system for Super-Kamiokande to maximize data from nearby supernovae

M. Mori, K. Abe, Y. Hayato +252

Neutrinos from very nearby supernovae, such as Betelgeuse, are expected to generate more than ten million events over 10\,s in Super-Kamokande (SK). At such large event rates, the…

hep-ex2024

Combined Pre-Supernova Alert System with Kamland and Super-Kamiokande

KamLAND, Super-Kamiokande Collaborations, : +311

Preceding a core-collapse supernova, various processes produce an increasing amount of neutrinos of all flavors characterized by mounting energies from the interior of massive star…

Search for proton decay via p→e+I¨0I¨0 and p→I^¼+I¨0I¨0 in 0.401 megaton-years exposure of Super-Kamiokande I-V

Development of a data overflow protection system for Super-Kamiokande to maximize data from nearby supernovae

Combined Pre-Supernova Alert System with Kamland and Super-Kamiokande

Search for proton decay via $p \to e^{+} I ¨ ^{0} I ¨ ^{0}$ and $p \to I^¼^{+} I ¨ ^{0} I ¨ ^{0}$ in 0.401 megaton-years exposure of Super-Kamiokande I-V