The future of high-energy astrophysical neutrino flavor measurements
N Song, SW Li, CA Argüelles… - … of Cosmology and …, 2021 - iopscience.iop.org
We critically examine the ability of future neutrino telescopes, including Baikal-GVD,
KM3NeT, P-ONE, TAMBO, and IceCube-Gen2, to determine the flavor composition of high …
KM3NeT, P-ONE, TAMBO, and IceCube-Gen2, to determine the flavor composition of high …
Theoretically palatable flavor combinations of astrophysical neutrinos
The flavor composition of high-energy astrophysical neutrinos can reveal the physics
governing their production, propagation, and interaction. The IceCube Collaboration has …
governing their production, propagation, and interaction. The IceCube Collaboration has …
Effect of new physics in astrophysical neutrino flavor
Astrophysical neutrinos are powerful tools for investigating the fundamental properties of
particle physics through their flavor content. In this Letter, we perform the first general new …
particle physics through their flavor content. In this Letter, we perform the first general new …
Probing BSM neutrino physics with flavor and spectral distortions: Prospects for future high-energy neutrino telescopes
IM Shoemaker, K Murase - Physical Review D, 2016 - APS
The flavor of cosmic neutrinos may help unveil their sources and could reveal the presence
of new physics in the neutrino sector. We consider impacts of next-generation neutrino …
of new physics in the neutrino sector. We consider impacts of next-generation neutrino …
Spectral analysis of the high-energy IceCube neutrinos
S Palomares-Ruiz, AC Vincent, O Mena - Physical Review D, 2015 - APS
A full energy and flavor-dependent analysis of the three-year high-energy IceCube neutrino
events is presented. By means of multidimensional fits, we derive the current preferred …
events is presented. By means of multidimensional fits, we derive the current preferred …
Flavor composition of ultrahigh-energy cosmic neutrinos: Measurement forecasts for in-ice radio-based EeV neutrino telescopes
A Coleman, O Ericsson, C Glaser, M Bustamante - Physical Review D, 2024 - APS
In-ice radio detection is a promising technique to discover and characterize ultrahigh-energy
(UHE) neutrinos, with energies above 10 17 eV, adopted by present—ARA, ARIANNA, and …
(UHE) neutrinos, with energies above 10 17 eV, adopted by present—ARA, ARIANNA, and …
Multimessenger astronomy and new neutrino physics
KJ Kelly, PAN Machado - Journal of Cosmology and Astroparticle …, 2018 - iopscience.iop.org
We discuss how to constrain new physics in the neutrino sector using multimessenger
astronomical observations by the IceCube experiment. The information from time and …
astronomical observations by the IceCube experiment. The information from time and …
Searching for MeV-scale gauge bosons with IceCube
A DiFranzo, D Hooper - Physical Review D, 2015 - APS
Light gauge bosons can lead to resonant interactions between high-energy astrophysical
neutrinos and the cosmic neutrino background. We study this possibility in detail …
neutrinos and the cosmic neutrino background. We study this possibility in detail …
New limits on neutrino decay from high-energy astrophysical neutrinos
Since neutrinos have mass differences they could decay into one another, but their lifetimes
are likely long, even when shortened by new physics, so decay likely impacts neutrinos only …
are likely long, even when shortened by new physics, so decay likely impacts neutrinos only …
Analysis of the 4-year IceCube high-energy starting events
AC Vincent, S Palomares-Ruiz, O Mena - Physical Review D, 2016 - APS
After four years of data taking, the IceCube neutrino telescope has detected 54 high-energy
starting events (HESE, or contained-vertex events) with deposited energies above 20 TeV …
starting events (HESE, or contained-vertex events) with deposited energies above 20 TeV …