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CAVE visualization of the IceCube neutrino detector
2014 IEEE Virtual Reality (VR), 2014Neutrinos are nearly massless, weakly interacting particles that come from a variety of sources including the sun, radioactive decay and cosmic rays. Neutrinos are unique cosmic messengers that provide new ways to explore the Universe as well as opportunities to better understand the basic building blocks of matter.
Ross Tredinnick +3 more
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Response of deep detectors to extraterrestrial neutrinos
Physical Review D, 1985We calculate the rate of upward muons induced by an arbitrary spectrum of ..nu../sub ..mu../ and nu-bar/sub ..mu../, including effects of the W propagator in the relevant charged-current cross sections. The results can be used to infer a parent-neutrino rate from an observed signal of upward muons.
, Gaisser, , Stanev
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AIP Conference Proceedings, 2005
The neutrino physics is one of the most important research field and there are several experiments made and under construction focused on it. This paper will present a review on some detectors used for Solar Neutrinos detection, Atmospheric Neutrinos detection and in Long Baseline Experiments.
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The neutrino physics is one of the most important research field and there are several experiments made and under construction focused on it. This paper will present a review on some detectors used for Solar Neutrinos detection, Atmospheric Neutrinos detection and in Long Baseline Experiments.
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The Homestake Neutrino Detector
Nuclear Physics B - Proceedings Supplements, 2012Abstract Neutrino mass ordering, mixing, and potential for CP violation are some of the most important questions facing particle physics today. To address them, a Long Baseline Neutrino Experiment (LBNE) is being planned using a 700 kw beam that would be directed from Fermilab to an underground site in Lead, South Dakota – a baseline of 1300 km.
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2001
Due to their weak interaction with matter and to the absence of their interaction with the electro-magnetic radiations, neutrinos can travel in the Universe without being absorbed. This is not the case for photons which interact with matter, with the infra-red (IR) radiation and with the cosmic microwave background (CMB).
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Due to their weak interaction with matter and to the absence of their interaction with the electro-magnetic radiations, neutrinos can travel in the Universe without being absorbed. This is not the case for photons which interact with matter, with the infra-red (IR) radiation and with the cosmic microwave background (CMB).
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A Detector for Neutrino Oscillations and Other Neutrino Interactions
AIP Conference Proceedings, 2002A multipurpose neutrino detector is described to measure neutrino oscillation with high sensitivity and other neutrino cross sections, of interest to astrophysics. This detector could use the high intensity, fast‐spill beam produced by the Spallation Neutron Source under construction at the Oak Ridge National Laboratory.
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Deep Underground Neutrino Experiment (DUNE) Near Detector Conceptual Design Report
Instruments, 2021G Adamov, T Alion, P Amedo
exaly