Particle astrophysics with high energy neutrinos
The topic of this review is the particle astrophysics of high energy neutrinos. High energy is
defined as Ev> 100 MeV. Main topics include:(i) atmospheric neutrinos and muons from π, K …
defined as Ev> 100 MeV. Main topics include:(i) atmospheric neutrinos and muons from π, K …
[HTML][HTML] Cosmic neutrino pevatrons: A brand new pathway to astronomy, astrophysics, and particle physics
The announcement by the IceCube Collaboration of the observation of 28 cosmic neutrino
candidates has been greeted with a great deal of justified excitement. The data reported so …
candidates has been greeted with a great deal of justified excitement. The data reported so …
Snowmass 2021 whitepaper: Proton structure at the precision frontier
An overwhelming number of theoretical predictions for hadron colliders require parton
distribution functions (PDFs), which are an important ingredient of theory infrastructure for …
distribution functions (PDFs), which are an important ingredient of theory infrastructure for …
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 …
Neutrino interactions at ultrahigh energies
We report new calculations of the cross sections for deeply inelastic neutrino-nucleon
scattering at neutrino energies between 10 9 eV and 10 21 eV. We compare with results in …
scattering at neutrino energies between 10 9 eV and 10 21 eV. We compare with results in …
Detecting ντ oscillations at PeV energies
It is suggested that a large deep underocean (or ice) neutrino detector, given the presence
of significant numbers of neutrinos in the PeV energy range as predicted by various models …
of significant numbers of neutrinos in the PeV energy range as predicted by various models …
Electromagnetic pulses from high-energy showers: Implications for neutrino detection
We review the properties of electromagnetic showers in dense media and calculate in detail
the associated electromagnetic pulses generated by shower electrons. We perform real-time …
the associated electromagnetic pulses generated by shower electrons. We perform real-time …
Astrophysical constraints on massive unstable neutral relic particles
J Ellis, GB Gelmini, JL Lopez, DV Nanopoulos… - Nuclear Physics B, 1992 - Elsevier
There has recently been renewed interest in massive neutral dark-matter particle candidates
with masses greater than∼ 1 TeV which may be unstable. We re-evaluate the constraints on …
with masses greater than∼ 1 TeV which may be unstable. We re-evaluate the constraints on …
Energy spectrum of ultra-high energy cosmic rays with extra-galactic origin
S Yoshida, M Teshima - Progress of theoretical physics, 1993 - academic.oup.com
We carried out a numerical calculation for the propagation of ultra-high energy cosmic ray
nucleons in the inergalactic space by a Monte-Carlo method. The resulting energy spectrum …
nucleons in the inergalactic space by a Monte-Carlo method. The resulting energy spectrum …
[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 …