When IceCube, a neutrino detector $250m observatory, is finally completed in around 2010, it will use 1km cube of ice, more than 2km below the surface at the South Pole, to detect the messengers from some of the most violent events in the universe. The project ...
Infrared Spectrum of a Molecular Ice Cube: The S$_4$ and D$_{2d}$ Water Octamers in Benzene-(Water)$_8$ IceCube Collaboration First year performance of the IceCube neutrino telescope Search for dark matter annihilations in the sun with the 79-string IceCube detector ...
ARA Collaboration (2012) Design and initial performance of the Askaryan Radio Array prototype EeV neutrino detector at the South Pole. Astropart Phys 35(7):457–477 Google Scholar Ashmore DW, Hubbard B, Luckman A et al (2017) Ice and firn heterogeneity within Larsen C Ice Shelf from bore...
str0552 Neutrino Radar Detectors str0553 Radars are able to see the whole layout of the target location. str0554 Subspace Tunneling str0555 Teleporting is now possible to previously unvisited locations but can fail sometimes. str0556 Waste Matter Condenser str0557 You are able to produce ...
Ice Cube has reported the detection of a diffuse Te V-Pe V neutrino emission, for which the flat spectrum radio quasars(FSRQs) have been proposed to be the candidate sources. Here we assume that the neutrino flux from FSRQs is proportional to their gamma-ray ones, and obtain the gamma-...
Atmospheric neutrino oscillations with DeepCore; Supernova detection with\nIceCube and beyond; Study of South Pole ice transparency with IceCube flashers;\nSubmitted papers to the 32nd International Cosmic Ray Conference, Beijing 2011.IceCube Collaboration...
M. Spurio, "Constraints to a Galactic Component of the Ice Cube cosmic neu- trino flux from ANTARES," Phys. Rev. D 90 (2014) 10, 103004M. Spurio, "Constraints to a Galactic component of the Ice Cube cosmic neutrino flux from ANTARES," Phys. Rev. D, vol. 90, p. 103004, Nov. ...
John Matson
How to See the Universe Through Neutrino EyesClara Moskowitz