Results 101 to 110 of about 107,166 (236)
Reconstructing WIMP properties with neutrino detectors
Physics Letters B, 2008 If the dark matter of the Universe is constituted by weakly interacting massive particles (WIMP), they would accumulate in the core of astrophysical objects as the Sun and annihilate into particles of the Standard Model. High-energy neutrinos would be produced in the annihilations, both directly and via the subsequent decay of leptons, quarks and ...
Mena O, Palomares-Ruiz S, Pascoli S
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The KM3NeT neutrino telescopes in the Mediterranean Sea: Current status and prospects focusing on KM3NeT/ORCA [PDF]
EPJ Web of ConferencesThe KM3NeT research infrastructure is building second-generation neutrino telescopes in the depths of the Mediterranean Sea. The KM3NeT/ARCA detector at a depth of about 3500 m off the coast of Sicily, Italy, focuses on the detection of high energy (E ...
Tzamariudaki Ekaterini
doaj +1 more source
The numerical computer experiment for the neutrino events with the SK neutrino oscillation parameters occurring outside the Superkamiokande detector [PDF]
arXiv, 2008 Adopting neutrino oscillation parameters obtained by Super-Kamiokande, a numerical computer experiment for neutrino events occurring outside the detector, is carried out in the same SK live days, 1645.9 live days, constructing the virtual Super-Kamiokande detector in the computer.
arxiv
Recent Developments in Halide Perovskite Nanocrystals for Indirect X‐ray Detection
Advanced Materials Technologies, Volume 9, Issue 20, October 21, 2024.Perovskite nanocrystals act as scintillators under X‐ray illumination with different conversion yield, stability, or decay times and outperform commercial materials, depending on their composition, host matrix, and luminescence process. Besides the lead halide perovskites, there are lead‐free alternatives providing self‐trapped exciton emission ...
Olexiy Balitskii +2 more
wiley +1 more source
ICARUS T600: physics results and future activities
EPJ Web of Conferences, 2016 The ICARUS T600 detector has proven the effectiveness of Liquid Argon TPC technology with a successful three-year long run at the INFN Gran Sasso National Laboratories (LNGS).
Zani Andrea
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Early Neutrino Data in the NO$ν$A Near Detector Prototype [PDF]
arXiv, 2011 NOvA is a long-baseline neutrino experiment using an off-axis neutrino beam produced by the NuMI neutrino beam at Fermilab. The NOvA experiment will study neutrino $\nu_{\mu}\rightarrow\nu_{e}$ oscillations. A short term goal for the NOvA experiment is to develop a good understanding of the response of the detector.
arxiv
Probing Nonstandard Neutrino Physics at T2KK [PDF]
arXiv, 2008 Having a far detector in Korea for the J-PARC neutrino beam in addition to one at Kamioka has been shown to be a powerful way to lift neutrino parameter ($\Delta m^2$ and mixing angles) degeneracies. In this talk, I report the sensitivity of the same experimental setup to nonstandard neutrino physics, such as quantum decoherence, violation of Lorentz ...
arxiv
The ANTARES neutrino telescope
EPJ Web of Conferences, 2013 The ANTARES neutrino telescope is the largest operating undersea neutrino telescope. It is located in the Northern hemisphere, 40 km far from Toulon, in the Mediterranean Sea.
Margiotta Annarita
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Measurement of Neutrino-Electron Elastic Scattering at NOvA Near Detector [PDF]
arXiv, 2017 NOvA is a long-baseline accelerator-based neutrino oscillation experiment that is optimized for electron-neutrino appearance measurements. It uses the upgraded NuMI beam from Fermilab and consists of a Far Detector in Ash River, Minnesota and a Near Detector at Fermilab.
arxiv
Neutrino Tridents at Near Detectors [PDF]
, 2018 Presentation from PONDD 2018 session Neutrino Trident ...
Zahra Tabrizi +5 more
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