We show that the measurements of 10 GeV atmospheric neutrinos by an upcoming array of densely-packed phototubes buried deep inside the IceCube detector at the South Pole can be used to determine the neutrino mass hierarchy for values of sin sin(2)2 theta(13) close to the present bound, if the hierarchy is normal. These results are obtained for an exposure of 100 Mton years and systematic uncertainties up to 10%
This paper investigates the physics reach of the IceCube neutrino detector when it will have collect...
IceCube is currently being built deep in the glacial ice beneath the South Pole. In its second year ...
The story of neutrinos began in 1930 when Pauli proposed a hypothesized particle as a ``desperate ...
The main goal of the IceCube Deep Core array is to search for neutrinos of astrophysical origins. At...
We present a measurement of the atmospheric neutrino oscillation parameters using three years of dat...
We study the possibility to perform neutrino oscillation tomography and to determine the neutrino ma...
AbstractThe nature of the neutrino mass hierarchy is one of the most interesting open questions in p...
We present a measurement of the atmospheric neutrino oscillation parameters using three years of dat...
We present a measurement of the atmospheric neutrino oscillation parameters using three years of dat...
We present a measurement of the atmospheric neutrino oscillation parameters using three years of dat...
We explore the physics potential of multi-megaton scale ice or water Cherenkov detectors with low ($...
AbstractWith its low-energy extension DeepCore, the IceCube Neutrino Observatory at the Amundsen-Sco...
The issue of determining the neutrino mass hierarchy is one of the outstanding questions in neutrino...
With its low-energy extension DeepCore, the IceCube Neutrino Observatory at the Amundsen-Scott South...
IceCube, a gigaton-scale neutrino detector located at the South Pole, was primarily designed to sear...
This paper investigates the physics reach of the IceCube neutrino detector when it will have collect...
IceCube is currently being built deep in the glacial ice beneath the South Pole. In its second year ...
The story of neutrinos began in 1930 when Pauli proposed a hypothesized particle as a ``desperate ...
The main goal of the IceCube Deep Core array is to search for neutrinos of astrophysical origins. At...
We present a measurement of the atmospheric neutrino oscillation parameters using three years of dat...
We study the possibility to perform neutrino oscillation tomography and to determine the neutrino ma...
AbstractThe nature of the neutrino mass hierarchy is one of the most interesting open questions in p...
We present a measurement of the atmospheric neutrino oscillation parameters using three years of dat...
We present a measurement of the atmospheric neutrino oscillation parameters using three years of dat...
We present a measurement of the atmospheric neutrino oscillation parameters using three years of dat...
We explore the physics potential of multi-megaton scale ice or water Cherenkov detectors with low ($...
AbstractWith its low-energy extension DeepCore, the IceCube Neutrino Observatory at the Amundsen-Sco...
The issue of determining the neutrino mass hierarchy is one of the outstanding questions in neutrino...
With its low-energy extension DeepCore, the IceCube Neutrino Observatory at the Amundsen-Scott South...
IceCube, a gigaton-scale neutrino detector located at the South Pole, was primarily designed to sear...
This paper investigates the physics reach of the IceCube neutrino detector when it will have collect...
IceCube is currently being built deep in the glacial ice beneath the South Pole. In its second year ...
The story of neutrinos began in 1930 when Pauli proposed a hypothesized particle as a ``desperate ...