Phenomenology with massive neutrinos
MC Gonzalez-Garcia, M Maltoni - Physics Reports, 2008 - Elsevier
The current status and some perspectives of the phenomenology of massive neutrinos is
reviewed. We start with the phenomenology of neutrino oscillations in vacuum and in matter …
reviewed. We start with the phenomenology of neutrino oscillations in vacuum and in matter …
Invited review article: IceCube: an instrument for neutrino astronomy
Neutrino astronomy beyond the Sun was first imagined in the late 1950s; by the 1970s, it
was realized that kilometer-scale neutrino detectors were required. The first such instrument …
was realized that kilometer-scale neutrino detectors were required. The first such instrument …
A convolutional neural network neutrino event classifier
A Aurisano, A Radovic, D Rocco… - Journal of …, 2016 - iopscience.iop.org
Convolutional neural networks (CNNs) have been widely applied in the computer vision
community to solve complex problems in image recognition and analysis. We describe an …
community to solve complex problems in image recognition and analysis. We describe an …
Testing the hadronuclear origin of PeV neutrinos observed with IceCube
We consider implications of the IceCube signal for hadronuclear (pp) scenarios of neutrino
sources such as galaxy clusters/groups and star-forming galaxies. Since the observed …
sources such as galaxy clusters/groups and star-forming galaxies. Since the observed …
First year performance of the IceCube neutrino telescope
A Achterberg, M Ackermann, J Adams, J Ahrens… - Astroparticle …, 2006 - Elsevier
The first sensors of the IceCube neutrino observatory were deployed at the South Pole
during the austral summer of 2004–2005 and have been producing data since February …
during the austral summer of 2004–2005 and have been producing data since February …
Calibration and characterization of the IceCube photomultiplier tube
Over 5000 PMTs are being deployed at the South Pole to compose the IceCube neutrino
observatory. Many are placed deep in the ice to detect Cherenkov light emitted by the …
observatory. Many are placed deep in the ice to detect Cherenkov light emitted by the …
TeV–PeV neutrinos from low-power gamma-ray burst jets inside stars
We study high-energy neutrino production in collimated jets inside progenitors of gamma-
ray bursts (GRBs) and supernovae, considering both collimation and internal shocks. We …
ray bursts (GRBs) and supernovae, considering both collimation and internal shocks. We …
Searches for sterile neutrinos with the IceCube detector
MG Aartsen, K Abraham, M Ackermann, J Adams… - Physical review …, 2016 - APS
The IceCube neutrino telescope at the South Pole has measured the atmospheric muon
neutrino spectrum as a function of zenith angle and energy in the approximate 320 GeV to …
neutrino spectrum as a function of zenith angle and energy in the approximate 320 GeV to …
Explosion mechanism, neutrino burst and gravitational wave in core-collapse supernovae
K Kotake, K Sato, K Takahashi - Reports on Progress in Physics, 2006 - iopscience.iop.org
Core-collapse supernovae are among the most energetic explosions in the universe
marking the catastrophic end of massive stars. In spite of rigorous studies for several …
marking the catastrophic end of massive stars. In spite of rigorous studies for several …
Muon track reconstruction and data selection techniques in AMANDA
The Antarctic Muon And Neutrino Detector Array (AMANDA) is a high-energy neutrino
telescope operating at the geographic South Pole. It is a lattice of photo-multiplier tubes …
telescope operating at the geographic South Pole. It is a lattice of photo-multiplier tubes …