The giant radio array for neutrino detection (GRAND): science and design
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 …
Radio detection of cosmic-ray air showers and high-energy neutrinos
FG Schröder - Progress in Particle and Nuclear Physics, 2017 - Elsevier
In the last fifteen years radio detection made it back to the list of promising techniques for
extensive air showers, firstly, due to the installation and successful operation of digital radio …
extensive air showers, firstly, due to the installation and successful operation of digital radio …
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 …
Ultra high energy cosmic rays The intersection of the Cosmic and Energy Frontiers
The present white paper is submitted as part of the “Snowmass” process to help inform the
long-term plans of the United States Department of Energy and the National Science …
long-term plans of the United States Department of Energy and the National Science …
Radio detection of cosmic ray air showers in the digital era
T Huege - Physics Reports, 2016 - Elsevier
In 1965 it was discovered that cosmic ray air showers emit impulsive radio signals at
frequencies below 100 MHz. After a period of intense research in the 1960s and 1970s …
frequencies below 100 MHz. After a period of intense research in the 1960s and 1970s …
Inferences on mass composition and tests of hadronic interactions from 0.3 to 100 EeV using the water-Cherenkov detectors of the Pierre Auger Observatory
A Aab, P Abreu, M Aglietta, I Al Samarai… - Physical Review D, 2017 - APS
We present a new method for probing the hadronic interaction models at ultrahigh energy
and extracting details about mass composition. This is done using the time profiles of the …
and extracting details about mass composition. This is done using the time profiles of the …
Measurement of the radiation energy in the radio signal of extensive air showers as a universal estimator of cosmic-ray energy
A Aab, P Abreu, M Aglietta, EJ Ahn, I Al Samarai… - Physical Review Letters, 2016 - APS
We measure the energy emitted by extensive air showers in the form of radio emission in the
frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger …
frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger …
[BOOK][B] Introduction to ultrahigh energy cosmic ray physics
P Sokolsky, G Thomson - 2020 - taylorfrancis.com
This revised edition provides an up-to-date summary of the field of ultra-high energy cosmic
rays, dealing with their origin, propagation, and composition,. The authors reflect the …
rays, dealing with their origin, propagation, and composition,. The authors reflect the …
COVID-19. Pandemic surgery guidance
Based on high quality surgery and scientific data, scientists and surgeons are committed to
protecting patients as well as healthcare staff and hereby provide this Guidance to address …
protecting patients as well as healthcare staff and hereby provide this Guidance to address …
Radio detection of air showers with the ARIANNA experiment on the Ross Ice Shelf
The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to
detect cosmogenic neutrinos of energies above 10 16 eV. The most neutrino-like …
detect cosmogenic neutrinos of energies above 10 16 eV. The most neutrino-like …