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pro vyhledávání: '"Verpoest, Stef"'
Autor:
Verpoest, Stef
The next-generation neutrino telescope IceCube-Gen2 is planned to include a surface detector array consisting of scintillation detectors and radio antennas for the detection of cosmic-ray air showers. Prototype stations, each comprising 8 scintillato
Externí odkaz:
http://arxiv.org/abs/2409.00713
Publikováno v:
Astroparticle Physics 161 (2024) 102985
Seasonal variations of atmospheric muons are traditionally interpreted in terms of an effective temperature that relates the atmospheric temperature profile at a given time to the dependence of muon production on atmospheric depth. This paper aims to
Externí odkaz:
http://arxiv.org/abs/2405.08926
The IceCube Neutrino Observatory at the geographic South Pole is, with its surface and in-ice detectors, used for both neutrino and cosmic-ray physics. The surface array, named IceTop, consists of ice-Cherenkov tanks grouped in 81 pairs spanning a 1
Externí odkaz:
http://arxiv.org/abs/2307.15394
Autor:
Verpoest, Stef
We report on an analysis of the high-energy muon component in near-vertical extensive air showers detected by the surface array IceTop in coincidence with the in-ice array of the IceCube Neutrino Observatory. In the coincidence measurement, the predo
Externí odkaz:
http://arxiv.org/abs/2307.14689
Autor:
Verpoest, Stef
The IceCube Neutrino Observatory at the South Pole can provide unique tests of muon production models in extensive air showers by measuring both the low-energy (GeV) and high-energy (TeV) muon components. We present here a measurement of the TeV muon
Externí odkaz:
http://arxiv.org/abs/2211.16970
Autor:
Gaisser, Thomas, Verpoest, Stef
Competition between decay and re-interaction of charged pions and kaons depends on the temperature/density profile of the upper atmosphere. The amplitude and phase of the variations depend on the minimum muon energy required to reach the detector and
Externí odkaz:
http://arxiv.org/abs/2107.12913
Autor:
Verpoest, Stef, Gaisser, Thomas K.
Production of high-energy muons in cosmic-ray air showers, relevant for underground detectors, depends on the properties of the primary cosmic ray as well as the atmospheric temperature through the competition between decay and re-interaction of char
Externí odkaz:
http://arxiv.org/abs/2107.11068
Testing Hadronic Interaction Models with Cosmic Ray Measurements at the IceCube Neutrino Observatory
The IceCube Neutrino Observatory provides the opportunity to perform unique measurements of cosmic-ray air showers with its combination of a surface array and a deep detector. Electromagnetic particles and low-energy muons ($\sim$GeV) are detected by
Externí odkaz:
http://arxiv.org/abs/2107.09387
Autor:
Gaisser, Thomas K., Verpoest, Stef
Publikováno v:
Astroparticle Physics 133 (2021) 102630
The production spectrum of high-energy muons as a function of depth in the atmosphere is relevant for understanding properties of event rates in deep detectors. For a given atmospheric profile, cascades of heavy nuclei develop at higher altitude than
Externí odkaz:
http://arxiv.org/abs/2106.12247
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