[HTML][HTML] Feebly-interacting particles: FIPs 2022 workshop report
C Antel, M Battaglieri, J Beacham, C Boehm… - The European Physical …, 2023 - Springer
Particle physics today faces the challenge of explaining the mystery of dark matter, the origin
of matter over anti-matter in the Universe, the origin of the neutrino masses, the apparent …
of matter over anti-matter in the Universe, the origin of the neutrino masses, the apparent …
Grand unified neutrino spectrum at Earth: Sources and spectral components
The dominant neutrino fluxes at Earth from different sources are reviewed and the grand
unified neutrino spectrum ranging from meV to PeV energies is presented. For each energy …
unified neutrino spectrum ranging from meV to PeV energies is presented. For each energy …
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 …
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 …
IceCube high-energy starting event sample: Description and flux characterization with 7.5 years of data
The IceCube Neutrino Observatory has established the existence of a high-energy all-sky
neutrino flux of astrophysical origin. This discovery was made using events interacting within …
neutrino flux of astrophysical origin. This discovery was made using events interacting within …
Multi-messenger observations of a binary neutron star merger
BP Abbott - 2017 - iopscience.iop.org
On 2017 August 17 a binary neutron star coalescence candidate (later designated
GW170817) with merger time 12: 41: 04 UTC was observed through gravitational waves by …
GW170817) with merger time 12: 41: 04 UTC was observed through gravitational waves by …
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 …
Letter of intent for KM3NeT 2.0
S Adrian-Martinez, M Ageron… - Journal of Physics G …, 2016 - iopscience.iop.org
The main objectives of the KM3NeT Collaboration are (i) the discovery and subsequent
observation of high-energy neutrino sources in the Universe and (ii) the determination of the …
observation of high-energy neutrino sources in the Universe and (ii) the determination of the …
Observation and Characterization of a Cosmic Muon Neutrino Flux from the Northern Hemisphere using six years of IceCube data
MG Aartsen, K Abraham, M Ackermann… - The Astrophysical …, 2016 - iopscience.iop.org
The detection of high-energy cosmic neutrinos as cosmic messengers has been an
important goal of astroparticle physics. Being stable, electrically neutral particles, high …
important goal of astroparticle physics. Being stable, electrically neutral particles, high …
A combined maximum-likelihood analysis of the high-energy astrophysical neutrino flux measured with IceCube
MG Aartsen, K Abraham, M Ackermann… - The Astrophysical …, 2015 - iopscience.iop.org
A COMBINED MAXIMUM-LIKELIHOOD ANALYSIS OF THE HIGH-ENERGY
ASTROPHYSICAL NEUTRINO FLUX MEASURED WITH ICECUBE - IOPscience Skip to …
ASTROPHYSICAL NEUTRINO FLUX MEASURED WITH ICECUBE - IOPscience Skip to …