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Quantum gravity phenomenology at the dawn of the multi-messenger era—A review
A Addazi, J Alvarez-Muniz, RA Batista… - Progress in Particle and …, 2022 - Elsevier
The exploration of the universe has recently entered a new era thanks to the multi-
messenger paradigm, characterized by a continuous increase in the quantity and quality of …
messenger paradigm, characterized by a continuous increase in the quantity and quality of …
The forward physics facility: Sites, experiments, and physics potential
Abstract The Forward Physics Facility (FPF) is a proposal to create a cavern with the space
and infrastructure to support a suite of far-forward experiments at the Large Hadron Collider …
and infrastructure to support a suite of far-forward experiments at the Large Hadron Collider …
Observation of high-energy neutrinos from the Galactic plane
IceCube Collaboration*†, R Abbasi, M Ackermann… - Science, 2023 - science.org
The origin of high-energy cosmic rays, atomic nuclei that continuously impact Earth's
atmosphere, is unknown. Because of deflection by interstellar magnetic fields, cosmic rays …
atmosphere, is unknown. Because of deflection by interstellar magnetic fields, cosmic rays …
[HTML][HTML] The forward physics facility at the high-luminosity LHC
High energy collisions at the High-Luminosity Large Hadron Collider (LHC) produce a large
number of particles along the beam collision axis, outside of the acceptance of existing LHC …
number of particles along the beam collision axis, outside of the acceptance of existing LHC …
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 …
Improved characterization of the astrophysical muon–neutrino flux with 9.5 years of IceCube data
R Abbasi, M Ackermann, J Adams… - The Astrophysical …, 2022 - iopscience.iop.org
We present a measurement of the high-energy astrophysical muon–neutrino flux with the
IceCube Neutrino Observatory. The measurement uses a high-purity selection of650k …
IceCube Neutrino Observatory. The measurement uses a high-purity selection of650k …
Detection of a particle shower at the Glashow resonance with IceCube
Nature, 2021 - nature.com
The Glashow resonance describes the resonant formation of a W− boson during the
interaction of a high-energy electron antineutrino with an electron, peaking at an …
interaction of a high-energy electron antineutrino with an electron, peaking at an …
High-energy and ultra-high-energy neutrinos: A Snowmass white paper
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 …
WIMP dark matter candidates and searches—current status and future prospects
L Roszkowski, EM Sessolo… - Reports on Progress in …, 2018 - iopscience.iop.org
We review several current aspects of dark matter theory and experiment. We overview the
present experimental status, which includes current bounds and recent claims and hints of a …
present experimental status, which includes current bounds and recent claims and hints of a …
Characteristics of the diffuse astrophysical electron and tau neutrino flux with six years of IceCube high energy cascade data
MG Aartsen, M Ackermann, J Adams, JA Aguilar… - Physical review …, 2020 - APS
We report on the first measurement of the astrophysical neutrino flux using particle showers
(cascades) in IceCube data from 2010–2015. Assuming standard oscillations, the …
(cascades) in IceCube data from 2010–2015. Assuming standard oscillations, the …