L. N. Machado

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.HE2026

Development of an early warning method incorporating pre-supernova neutrino light curves

Keita Saito, Minori Eizuka, Zhuojun Hu +9

Massive stars ( $M > 8 M_{⊙}$ ) emit neutrinos known as pre-supernova (pre-SN) neutrinos through thermal and nuclear interactions for cooling the stellar core during the fina…

hep-ex2025

Search for Neutrino Counterparts to Gravitational Wave Events in Super-Kamiokande during the LIGO/Virgo/KAGRA O4 Observing Run

L. N . Machado

In recent years, the Super-Kamiokande (SK) experiment has contributed to multi-messenger astronomy by searching for neutrino signals in coincidence with gravitational wave events.…

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 an early warning method incorporating pre-supernova neutrino light curves

Search for Neutrino Counterparts to Gravitational Wave Events in Super-Kamiokande during the LIGO/Virgo/KAGRA O4 Observing Run

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