420 citations · 2.9k across the 65 of their papers we have counts for
7 papers · 2 filters
Inverting a Supernova: Neutrino Mixing, Temperatures and Binding Energy
V. Barger, D. Marfatia, B. P. Wood
We show that the temperatures of the emergent non-electron neutrinos and the binding energy released by a galactic Type II supernova are determinable, assuming the Large Mixing Ang…
E1 Working Group Summary: Neutrino Factories and Muon Colliders
D. Harris
We are in the middle of a time of exciting discovery, namely that neutrinos have mass and oscillate. In order to take the next steps to understand this potential window onto what w…
Neutrino Superbeam Scenarios at the Peak
V. Barger, D. Marfatia, K. Whisnant
We discuss options for U.S. long baseline neutrino experiments using upgraded conventional neutrino beams, assuming is chosen to be near the peak of the leading oscillation…
Testing radiative neutrino mass generation via R-parity violation at the Tevatron
V. Barger, T. Han, S. Hesselbach +1
An R-parity violating SUSY model with lepton-number violating couplings , i=2,3 can generate a neutrino mass spectrum that explains the recent results from neutrino oscil…
Unknowns after the SNO Charged-Current Measurement
V. Barger, D. Marfatia, K. Whisnant
We perform a model-independent analysis of solar neutrino flux rates including the recent charged-current measurement at the Sudbury Neutrino Observatory (SNO). We derive a univers…
Piecing the Solar Neutrino Puzzle Together at SNO
V. Barger, D. Marfatia, K. Whisnant
We perform an oscillation parameter-independent analysis of solar neutrino flux measurements from which we predict the charged-current rate at SNO relative to Standard Solar Model…
Earth Regeneration of Solar Neutrinos at SNO and Super-Kamiokande
V. Barger, D. Marfatia, K. Whisnant +1
We analyze the 1258-day Super-Kamiokande day and night solar neutrino energy spectra with various definitions. The best-fit lies in the LMA region at $(Δm^2, tan^2 θ)=(5.01\t…