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 …
The Muon Puzzle in cosmic-ray induced air showers and its connection to the Large Hadron Collider
High-energy cosmic rays are observed indirectly by detecting the extensive air showers
initiated in Earth's atmosphere. The interpretation of these observations relies on accurate …
initiated in Earth's atmosphere. The interpretation of these observations relies on accurate …
First observation of PeV-energy neutrinos with IceCube
We report on the observation of two neutrino-induced events which have an estimated
deposited energy in the IceCube detector of 1.04±0.16 and 1.14±0.17 PeV, respectively, the …
deposited energy in the IceCube detector of 1.04±0.16 and 1.14±0.17 PeV, respectively, the …
Phenomenology with massive neutrinos
MC Gonzalez-Garcia, M Maltoni - Physics Reports, 2008 - Elsevier
The current status and some perspectives of the phenomenology of massive neutrinos is
reviewed. We start with the phenomenology of neutrino oscillations in vacuum and in matter …
reviewed. We start with the phenomenology of neutrino oscillations in vacuum and in matter …
Ultrahigh-energy neutrino interactions
Cross sections for the interactions of ultrahigh-energy neutrinos with nucleons are evaluated
in the light of new information about nucleon structure functions. For 102 eV neutrinos, the …
in the light of new information about nucleon structure functions. For 102 eV neutrinos, the …
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 …
Evidence for astrophysical muon neutrinos from the northern sky with IceCube
MG Aartsen, K Abraham, M Ackermann, J Adams… - Physical review …, 2015 - APS
Results from the IceCube Neutrino Observatory have recently provided compelling evidence
for the existence of a high energy astrophysical neutrino flux utilizing a dominantly Southern …
for the existence of a high energy astrophysical neutrino flux utilizing a dominantly Southern …
Prompt neutrino fluxes from atmospheric charm
We calculate the prompt neutrino flux from atmospheric charm production by cosmic rays,
using the dipole picture in a perturbative QCD framework, which incorporates the parton …
using the dipole picture in a perturbative QCD framework, which incorporates the parton …
Flux of atmospheric neutrinos
TK Gaisser, M Honda - Annual Review of Nuclear and Particle …, 2002 - annualreviews.org
▪ Abstract Atmospheric neutrinos produced by cosmic-ray interactions in the atmosphere are
of interest for several reasons. As a beam for studies of neutrino oscillations, they cover a …
of interest for several reasons. As a beam for studies of neutrino oscillations, they cover a …
Atmospheric muon flux at sea level, underground, and underwater
EV Bugaev, A Misaki, VA Naumov, TS Sinegovskaya… - Physical Review D, 1998 - APS
The vertical sea-level muon spectrum at energies above 1 GeV and the muon intensities at
depths up to 18 km we in different rocks and in water are calculated. The results are …
depths up to 18 km we in different rocks and in water are calculated. The results are …