[HTML][HTML] Open questions in cosmic-ray research at ultrahigh energies
R Alves Batista, J Biteau, M Bustamante… - Frontiers in Astronomy …, 2019 - frontiersin.org
We review open questions and prospects for progress in ultrahigh-energy cosmic ray
(UHECR) research, based on a series of discussions that took place during the “The High …
(UHECR) research, based on a series of discussions that took place during the “The High …
The giant radio array for neutrino detection (GRAND): science and design
J Alvarez-Muniz, R Alves Batista, A Balagopal V… - Science China Physics …, 2020 - Springer
Abstract The Giant Radio Array for Neutrino Detection (GRAND) is a planned large-scale
observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 10 8 GeV …
observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 10 8 GeV …
IceCube-Gen2: the window to the extreme Universe
MG Aartsen, R Abbasi, M Ackermann… - Journal of Physics G …, 2021 - iopscience.iop.org
The observation of electromagnetic radiation from radio to γ-ray wavelengths has provided a
wealth of information about the Universe. However, at PeV (10 15 eV) energies and above …
wealth of information about the Universe. However, at PeV (10 15 eV) energies and above …
[HTML][HTML] 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 …
Design and sensitivity of the Radio Neutrino Observatory in Greenland (RNO-G)
This article presents the design of the Radio Neutrino Observatory Greenland (RNO-G) and
discusses its scientific prospects. Using an array of radio sensors, RNO-G seeks to measure …
discusses its scientific prospects. Using an array of radio sensors, RNO-G seeks to measure …
The future of high-energy astrophysical neutrino flavor measurements
N Song, SW Li, CA Argüelles… - … of Cosmology and …, 2021 - iopscience.iop.org
We critically examine the ability of future neutrino telescopes, including Baikal-GVD,
KM3NeT, P-ONE, TAMBO, and IceCube-Gen2, to determine the flavor composition of high …
KM3NeT, P-ONE, TAMBO, and IceCube-Gen2, to determine the flavor composition of high …
Status of non-standard neutrino interactions
T Ohlsson - Reports on Progress in Physics, 2013 - iopscience.iop.org
The phenomenon of neutrino oscillations has been established as the leading mechanism
behind neutrino flavor transitions, providing solid experimental evidence that neutrinos are …
behind neutrino flavor transitions, providing solid experimental evidence that neutrinos are …
Astrophysical neutrino oscillations after pulsar timing array analyses
The pattern of neutrino flavor oscillations could be altered by the influence of noisy
perturbations such as those arising from a gravitational wave background (GWB). A …
perturbations such as those arising from a gravitational wave background (GWB). A …
Flavor ratio of astrophysical neutrinos above 35 TeV in IceCube
MG Aartsen, M Ackermann, J Adams, JA Aguilar… - Physical review …, 2015 - APS
A diffuse flux of astrophysical neutrinos above 100 TeV has been observed at the IceCube
Neutrino Observatory. Here we extend this analysis to probe the astrophysical flux down to …
Neutrino Observatory. Here we extend this analysis to probe the astrophysical flux down to …
Theoretically palatable flavor combinations of astrophysical neutrinos
The flavor composition of high-energy astrophysical neutrinos can reveal the physics
governing their production, propagation, and interaction. The IceCube Collaboration has …
governing their production, propagation, and interaction. The IceCube Collaboration has …