S. T. Dye

Determination of neutrino mass hierarchy and {theta}{sub 13} with a remote detector of reactor antineutrinos

We describe a method for determining the hierarchy of the neutrino mass spectrum and

Geophysical and geochemical constraints on geoneutrino fluxes from Earth's mantle

{\ensuremath{\theta}}_{13}

Limits on the flux of energetic neutrinos from the sun

through remote detection of electron antineutrinos from a nuclear reactor. This method utilizing a single, 10-kiloton scintillating liquid detector at a distance of 49\char21{}63 kilometers from the reactor complex measures mass-squared differences involving

IMB-3: a large water Cherenkov detector for nucleon decay and neutrino interactions

{\ensuremath{\nu}}_{3}

A serach for moderate- and high-energy neturino emission correlated with gamma-ray bursts

with a one(ten)-year exposure provided

Estimating terrestrial uranium and thorium by antineutrino flux measurements

{sin}^{2}(2{\ensuremath{\theta}}_{13})g0.05(0.02)

AGM2015: Antineutrino Global Map 2015

. Our technique applies the Fourier transform to the event rate as a function of neutrino flight distance over neutrino energy. Sweeping a relevant range of

Neutrino mixing discriminates geo-reactor models

\ensuremath{\delta}{m}^{2}

The many uses of electron antineutrinos

resolves separate spectral peaks for

Corrigendum: AGM2015: Antineutrino Global Map 2015

\ensuremath{\delta}m^{2}{}_{31}