Skip to main navigation
Skip to search
Skip to main content
University of Copenhagen Research Portal Home
Help & FAQ
Dansk
English
Home
Profiles
Research output
Research units
Press/Media
Activities
Prizes
???studenttheses???
Datasets
Search by expertise, name or affiliation
Inferring the flavor of high-energy astrophysical neutrinos at their sources
Mauricio Bustamante
*
,
Markus Ahlers
*
Corresponding author for this work
Theoretical high energy, astroparticle and gravitational physics
13
Citations (Scopus)
Overview
Fingerprint
Fingerprint
Dive into the research topics of 'Inferring the flavor of high-energy astrophysical neutrinos at their sources'. Together they form a unique fingerprint.
Sort by
Weight
Alphabetically
Keyphrases
Flavor Composition
100%
Astrophysical Neutrinos
100%
High Energy
100%
Production Mechanism
50%
Pion
25%
Neutrino Flavor
25%
Bayesian Methods
25%
Compositional Parameters
25%
Source Mechanism
25%
Neutrino Production
25%
Neutrinos
25%
Neutron
25%
Mixing Parameters
25%
Flavor Mixing
25%
IceCube Neutrinos
25%
Neutrino Telescope
25%
Neutrino Sources
25%
Physical Condition
25%
Source-driven
25%
Physics
Neutrino Telescopes
100%