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From the 1 of 483 papers with an AI index.

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19932026
most citedEvidence for oscillation of atmospheric neutrinos

5.1k citations

Showing 2013Show all

27 papers · 1 filter

hep-ex2013★ 98 cited

First Indication of Terrestrial Matter Effects on Solar Neutrino Oscillation

A. Renshaw, K. Abe, Y. Hayato +112

We report an indication that the elastic scattering rate of solar B neutrinos with electrons in the Super-Kamiokande detector is larger when the neutrinos pass through the Eart…

hep-ex2013★ 90 cited

Search for doubly charmed baryons and study of charmed strange baryons at Belle

Y. Kato, T. Iijima, I. Adachi +167

We report results of a study of doubly charmed baryons and charmed strange baryons. The analysis is performed using a 980 fb^-1 data sample collected with the Belle detector at the…

astro-ph.SR2013★ 44 cited

Observations of 6.7 GHz Methanol Masers with EAVN I: VLBI Images of the first Epoch of Observations

Kenta Fujisawa, Koichiro Sugiyama, Kazuhito Motogi +26

Very long baseline interferometry (VLBI) monitoring of the 6.7 GHz methanol maser allows us to measure the internal proper motions of the maser spots and therefore study the gas mo…

hep-ex2013★ 132 cited

Supernova Relic Neutrino Search with Neutron Tagging at Super-Kamiokande-IV

Kamiokande Collaboration

A search for Supernova Relic Neutrinos 's is first conducted via inverse-beta-decay by tagging neutron capture on hydrogen at Super-Kamiokande-IV. The neutron tagging effi…

nlin.AO2013★ 7 cited

Power-law exponent of the Bouchaud-Mézard model on regular random network

Takashi Ichinomiya

We study the Bouchaud-Mézard model on a regular random network. By assuming adiabaticity and independency, and utilizing the generalized central limit theorem and the Tauberian the…

hep-ex2013★ 35 cited

High-statistics study of K^0_S pair production in two-photon collisions

The Belle Collaboration, S. Uehara, Y. Watanabe +164

We report a high-statistics measurement of the differential cross section of the process gamma gamma --> K^0_S K^0_S in the range 1.05 GeV <= W <= 4.00 GeV, where W is the center-o…