High-energy and ultra-high-energy neutrinos: A Snowmass white paper
M Ackermann, M Bustamante, L Lu, N Otte… - Journal of high energy …, 2022 - Elsevier
Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy
physics. With energies far beyond solar, supernovae, atmospheric, and accelerator …
physics. With energies far beyond solar, supernovae, atmospheric, and accelerator …
Detector requirements for model-independent measurements of ultrahigh energy neutrino cross sections
The ultrahigh energy range of neutrino physics (above∼ 10 7 GeV), as yet devoid of
detections, is an open landscape with challenges to be met and discoveries to be made …
detections, is an open landscape with challenges to be met and discoveries to be made …
Flavor composition of ultrahigh-energy cosmic neutrinos: Measurement forecasts for in-ice radio-based EeV neutrino telescopes
A Coleman, O Ericsson, C Glaser, M Bustamante - Physical Review D, 2024 - APS
In-ice radio detection is a promising technique to discover and characterize ultrahigh-energy
(UHE) neutrinos, with energies above 10 17 eV, adopted by present—ARA, ARIANNA, and …
(UHE) neutrinos, with energies above 10 17 eV, adopted by present—ARA, ARIANNA, and …
Radio detection of high energy neutrinos in ice
SW Barwick, C Glaser - The Encyclopedia of Cosmology: Set 2 …, 2024 - World Scientific
Radio-based detection of high-energy particles is growing in maturity. In this chapter, we
focus on the detection of neutrinos with energies in excess of 10 PeV that interact in the …
focus on the detection of neutrinos with energies in excess of 10 PeV that interact in the …
First-principle calculation of birefringence effects for in-ice radio detection of neutrinos
N Heyer, C Glaser - The European Physical Journal C, 2023 - Springer
The detection of high-energy neutrinos in the EeV range requires new detection techniques
to cope with the small expected flux. The radio detection method, utilizing Askaryan …
to cope with the small expected flux. The radio detection method, utilizing Askaryan …
Triboelectric backgrounds to radio-based polar ultra-high energy neutrino (UHEN) experiments
JA Aguilar, A Anker, P Allison, S Archambault… - Astroparticle …, 2023 - Elsevier
In the hopes of observing the highest-energy neutrinos (E> 1 EeV) populating the Universe,
both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar …
both past (RICE, AURA, ANITA) and current (RNO-G, ARIANNA, ARA and TAROGE-M) polar …
In-ice Askaryan Emission from Air Showers: Implications for Radio Neutrino Detectors
One of the most promising techniques for detecting ultra-high energy neutrinos involves the
use of radio antennas to observe the 10-1000 MHz radiation generated by the showers that …
use of radio antennas to observe the 10-1000 MHz radiation generated by the showers that …
A search for the ultra high energy neutrinos with the low threshold phased array trigger system of the Askaryan Radio Array
P Dasgupta - arXiv preprint arXiv:2409.19847, 2024 - arxiv.org
The Askaryan Radio Array (ARA) is an in-ice ultra high energy (UHE, $> 10$ PeV) neutrino
experiment at the South Pole that aims to detect UHE neutrino-induced radio emission in …
experiment at the South Pole that aims to detect UHE neutrino-induced radio emission in …
Simulation study for an in-situ calibration system for the measurement of the snow accumulation and the index-of-refraction profile for radio neutrino detectors
J Beise, C Glaser - Journal of Instrumentation, 2023 - iopscience.iop.org
Sensitivity to ultra-high-energy neutrinos (E> 17 eV) can be obtained cost-efficiently by
exploiting the Askaryan effect in ice, where a particle cascade induced by the neutrino …
exploiting the Askaryan effect in ice, where a particle cascade induced by the neutrino …
[PDF][PDF] Understanding Radar Echoes from High-Energy Particle Cascades
EH SANTIAGO - 2024 - researchportal.vub.be
To this day, no experiment has claimed to have detected a neutrino with an energy above 10
PeV, or 1016 eV. At those high energies, neutrinos are only known to be produced in the …
PeV, or 1016 eV. At those high energies, neutrinos are only known to be produced in the …