Neutrino astroparticle physics studies neutrinos as cosmic messengers, fundamental particles, and probes of astrophysical environments, cosmology, dark matter, and physics beyond the Standard Model.
Introduction to astroparticle physics
Neutrinos as cosmic messenger particles
Historical development of neutrino astronomy
Standard Model description of neutrinos
Neutrino flavor states
Neutrino mass eigenstates
Dirac versus Majorana neutrinos
Neutrino helicity and chirality
Active and sterile neutrinos
Neutrino mixing matrix
Pontecorvo–Maki–Nakagawa–Sakata matrix
Neutrino mass ordering
Absolute neutrino-mass scale
Neutrino magnetic and electromagnetic properties
Weak interactions of astrophysical neutrinos
Thermal neutrino production
Nuclear beta processes
Electron and positron capture
Proton–proton interactions
Proton–photon interactions
Charged-pion decay
Charged-kaon decay
Muon decay
Neutron decay
Photodisintegration processes
Pair-annihilation neutrinos
Plasma-process neutrinos
Bremsstrahlung neutrinos
Hadronuclear neutrino production
Photohadronic neutrino production
Cosmogenic neutrino production
Proton–proton-chain neutrinos
CNO-cycle neutrinos
Solar-neutrino energy spectrum
Solar-neutrino problem
Matter-enhanced solar-neutrino oscillations
Solar metallicity problem
Solar-core temperature measurements
Day–night asymmetry of solar neutrinos
Seasonal solar-neutrino variations
Solar-flare neutrinos
High-energy solar atmospheric neutrinos
Solar neutrinos as probes of new physics
Neutrinos from main-sequence stars
Red-giant neutrinos
White-dwarf neutrinos
Neutrinos from stellar nucleosynthesis
Thermal neutrino cooling of stars
Pre-supernova neutrinos
Neutrino emission during silicon burning
Neutrino constraints on stellar evolution
Neutrino magnetic moments in stars
Exotic-particle cooling constraints
Neutrinos from compact binary systems
Neutrino emission from stellar mergers
Core-collapse supernova neutrinos
Neutrino-driven supernova explosions
Neutronization-burst neutrinos
Accretion-phase neutrinos
Proto-neutron-star cooling
Supernova-neutrino energy spectra
Neutrino transport in dense matter
Neutrino opacity in supernova cores
Neutrino heating behind the shock
Collective neutrino oscillations
Fast flavor conversions
Matter-neutrino resonance
Supernova mass-ordering sensitivity
Supernova early-warning systems
Supernova-neutrino triangulation
Failed-supernova neutrinos
Black-hole formation signatures
Hypernova neutrinos
Diffuse supernova neutrino background
Supernova relic neutrinos
Neutrino cooling of neutron stars
Direct and modified Urca processes
Neutrino emission from neutron-star crusts
Neutron-star merger neutrinos
Post-merger neutrino emission
Neutrino transport in merger remnants
Neutrino-driven winds
Neutrino nucleosynthesis in compact-object mergers
Magnetar neutrinos
Pulsar-associated neutrinos
Neutrino emission from accreting neutron stars
Quark-matter effects on neutrino emission
Neutrinos from phase transitions in dense matter
TeV–PeV astrophysical neutrinos
Ultra-high-energy neutrinos
Exa-electronvolt neutrinos
Diffuse astrophysical neutrino flux
Point-source neutrino searches
Extended-source neutrino searches
Transient neutrino sources
Steady neutrino sources
Astrophysical-neutrino energy spectrum
Flavor composition at Earth
Neutrino–antineutrino composition
Spectral cutoffs and breaks
Source opacity to cosmic rays
Hidden cosmic-ray accelerators
Neutrino source population studies
Anisotropy of the cosmic-neutrino sky
Active galactic nuclei
Blazars
Radio galaxies
Seyfert galaxies
Quasars
Tidal disruption events
Gamma-ray bursts
Low-luminosity gamma-ray bursts
Choked-jet supernovae
Starburst galaxies
Galaxy clusters
Galaxy groups
Galactic Center
Galactic plane
Supernova remnants
Pulsar-wind nebulae
Microquasars
X-ray binaries
Binary neutron-star mergers
Neutron-star–black-hole mergers
Magnetar giant flares
Novae
Hypernovae
Fast radio bursts
Young stellar objects
Solar atmosphere
Interstellar-medium interactions
Cosmic-ray air showers
Conventional atmospheric neutrinos
Prompt atmospheric neutrinos
Pion- and kaon-decay neutrinos
Charm-decay neutrinos
Atmospheric-neutrino flux calculations
Zenith-angle distributions
Seasonal atmospheric-neutrino variations
Geomagnetic effects
Atmospheric-neutrino oscillations
Tau-neutrino appearance
Atmospheric-neutrino mass-ordering studies
Atmospheric-neutrino backgrounds
Atmospheric-muon rejection
High-energy atmospheric-neutrino uncertainties
Greisen–Zatsepin–Kuzmin neutrinos
Ultra-high-energy cosmic-ray interactions
Cosmic-ray interactions with the cosmic microwave background
Cosmic-ray interactions with extragalactic background light
Cosmogenic-neutrino flux models
Proton versus heavy-nucleus cosmic rays
Ultra-high-energy source evolution
Neutrino horizon at extreme energies
Earth absorption of ultra-high-energy neutrinos
Earth-skimming tau neutrinos
Mountain-skimming tau neutrinos
Upward-going tau air showers
Horizontal air-shower neutrinos
Radio detection of ultra-high-energy neutrinos
Askaryan emission from neutrino-induced cascades
Geomagnetic radio emission from tau air showers
Vacuum neutrino oscillations
Matter-enhanced neutrino oscillations
Mikheyev–Smirnov–Wolfenstein effect
Oscillations through Earth
Parametric neutrino resonances
Oscillations in stellar matter
Oscillations in supernova envelopes
Collective neutrino effects
Neutrino self-interactions
Flavor decoherence
Wave-packet separation
Astrophysical neutrino flavor ratios
Source flavor composition
Muon-damped neutrino sources
Neutron-beam neutrino sources
Tau-neutrino regeneration
Neutrino absorption in Earth
Neutrino attenuation in cosmic backgrounds
Neutrino lensing
Gravitational effects on neutrino propagation
Neutrino–nucleon scattering
Neutrino–electron scattering
Charged-current interactions
Neutral-current interactions
Deep-inelastic neutrino scattering
Quasi-elastic scattering
Resonant pion production
Coherent elastic neutrino–nucleus scattering
Glashow-resonance events
Tau-neutrino interactions
Tau-lepton emergence and decay
Neutrino cross-sections at extreme energies
Small-(x) parton distributions
Nuclear shadowing effects
Beyond-Standard-Model interaction signatures
Neutrino interactions with cosmic backgrounds
Cosmic neutrino background
Relic neutrino decoupling
Effective number of relativistic species
Neutrino contribution to radiation density
Neutrino masses from cosmology
Neutrino free-streaming
Effects on cosmic structure formation
Effects on the cosmic microwave background
Big Bang nucleosynthesis constraints
Lepton asymmetry of the Universe
Neutrino chemical potentials
Sterile neutrinos in cosmology
Neutrino isocurvature perturbations
Neutrino clustering
Detection of relic neutrinos
Cosmological neutrino tomography
Neutrinos from dark-matter annihilation
Neutrinos from dark-matter decay
Dark matter captured in the Sun
Dark matter captured in Earth
Galactic-halo neutrino signals
Galactic-Center dark-matter searches
Extragalactic dark-matter neutrino flux
Heavy dark-matter decay
Super-heavy dark matter
Secluded dark-matter models
Neutrino-portal dark matter
Sterile-neutrino dark matter
Neutrino–dark-matter scattering
Dark-matter effects on neutrino propagation
Dark-matter substructure searches
Dark-sector mediators
Sterile-neutrino searches
Nonstandard neutrino interactions
Secret neutrino interactions
Neutrino decay
Invisible neutrino decay
Pseudo-Dirac neutrinos
Lorentz-invariance violation
CPT violation
Equivalence-principle tests
Quantum-gravity effects
Neutrino magnetic moments
Neutrino millicharge
Axion–neutrino interactions
Majoron-neutrino interactions
Extra-dimensional models
Neutrino decoherence
Leptoquarks in neutrino interactions
Heavy neutral leptons
New resonances in cosmic-neutrino spectra
New long-range forces
Neutrino–gamma-ray correlations
Neutrino–cosmic-ray correlations
Neutrino–gravitational-wave correlations
Neutrino–X-ray correlations
Neutrino–radio correlations
Neutrino–optical transient correlations
Neutrino–fast-radio-burst correlations
Multimessenger observations of blazars
Multimessenger observations of supernovae
Multimessenger observations of compact mergers
Real-time neutrino alerts
Target-of-opportunity observations
Coincidence-search methods
Source localization
Temporal correlation analysis
Population-level multimessenger studies
Water-Cherenkov detection
Ice-Cherenkov detection
Liquid-scintillator detection
Liquid-argon time-projection chambers
Water-based liquid scintillators
Radio detection in ice
Radio detection in salt
Radio detection in lunar regolith
Radio detection in deserts
Acoustic neutrino detection
Air-shower fluorescence detection
Surface-particle detection
Imaging atmospheric Cherenkov detection
Mountain-based tau-neutrino detection
Balloon-borne neutrino detection
Satellite-based neutrino detection
Lunar neutrino detection
Coherent-scattering detectors
Neutrino-direction reconstruction
Neutrino-energy reconstruction
IceCube Neutrino Observatory
IceCube-Gen2
KM3NeT-ARCA
KM3NeT-ORCA
Baikal-GVD
ANTARES
Super-Kamiokande
Hyper-Kamiokande
JUNO
DUNE
SNO+
Borexino
Pierre Auger Observatory
ANITA
PUEO
RNO-G
ARA
ARIANNA
GRAND
Trinity
BEACON
TAMBO
POEMMA
EUSO-SPB
RET-N
NνDEx and coherent-neutrino experiments
PTOLEMY and relic-neutrino detection
Bay of Bengal neutrino-telescope concepts
Himalayan tau-neutrino observatory concepts
Photomultiplier tubes
Silicon photomultipliers
Digital optical modules
Multi-PMT optical modules
Radio antennas
Phased-array radio receivers
Acoustic sensors
Water-Cherenkov detector arrays
Scintillator arrays
Timing and synchronization systems
Underwater data transmission
Deep-sea detector deployment
Ice drilling and detector deployment
Detector calibration
Optical properties of water and ice
Radio attenuation lengths
Bioluminescence backgrounds
Environmental detector backgrounds
Trigger systems
Real-time data acquisition
Muon-track events
Electromagnetic-cascade events
Hadronic-cascade events
Double-bang tau-neutrino events
Lollipop events
Double-pulse events
Starting-track events
Through-going muon events
Upward-going events
Glashow-resonance events
Earth-skimming tau events
Radio-pulse reconstruction
Air-shower reconstruction
Neutrino angular resolution
Neutrino energy resolution
Flavor identification
Neutrino–antineutrino discrimination
Event topology classification
Background rejection
Source-direction reconstruction
Atmospheric-muon backgrounds
Atmospheric-neutrino backgrounds
Prompt-neutrino uncertainties
Cosmic-ray composition uncertainties
Detector-noise backgrounds
Optical scattering and absorption
Radio-frequency interference
Anthropogenic radio backgrounds
Bioluminescence and marine backgrounds
Ice and water property uncertainties
Neutrino cross-section uncertainties
Hadronic-interaction model uncertainties
Astrophysical-flux uncertainties
Calibration uncertainties
Detector-acceptance uncertainties
False multimessenger coincidences
Monte Carlo neutrino simulations
Cosmic-ray air-shower simulation
Neutrino event generators
Neutrino transport simulations
Tau-lepton propagation simulations
Detector-response simulation
Likelihood analysis
Bayesian neutrino inference
Unfolding neutrino spectra
Point-source search algorithms
Time-dependent source searches
Stacking analyses
Population analyses
Machine-learning event classification
Deep-learning track reconstruction
Graph neural networks for neutrino detectors
Anomaly detection
Real-time alert pipelines
Open neutrino-data analysis
High-performance computing
Hadronic source models
Leptohadronic source models
Cosmic-ray acceleration mechanisms
Fermi acceleration
Magnetic reconnection
Shock acceleration
Maximum particle energy
Particle escape from sources
Source magnetic fields
Radiation-field modeling
Gamma-ray opacity
Neutrino spectral modeling
Neutrino luminosity functions
Source population synthesis
Redshift evolution of neutrino sources
Diffuse-flux calculations
What produces the diffuse high-energy neutrino flux?
Which sources accelerate cosmic rays to ultra-high energies?
Are blazars dominant cosmic-neutrino sources?
Do hidden particle accelerators produce most cosmic neutrinos?
What is the astrophysical tau-neutrino flux?
What is the maximum energy of cosmic neutrinos?
Can neutrinos reveal the cosmic-ray mass composition?
Can neutrinos determine the mass ordering?
Do astrophysical neutrinos decay during propagation?
Are sterile neutrinos present in cosmic fluxes?
Can neutrinos identify dark matter?
Can relic neutrinos be detected directly?
How do neutrinos affect supernova explosions?
What causes fast flavor conversion in supernovae?
Can neutrinos probe neutron-star interiors?
Can neutrino observations test quantum gravity?
Can Earth-skimming tau neutrinos open the EeV sky?
What is the origin of the Glashow-resonance event population?
Is the cosmic-neutrino sky isotropic?
Can multimessenger observations identify individual neutrino accelerators?
Global neutrino-observatory networks
Real-time multimessenger neutrino astronomy
Neutrino tomography of Earth
Neutrino tomography of the Sun
Neutrino tomography of astrophysical sources
Ocean-based modular neutrino telescopes
Mountain-valley tau-neutrino arrays
Space-based tau-neutrino observatories
Lunar Askaryan neutrino detection
Radar detection of neutrino-induced cascades
Distributed radio-neutrino arrays
Quantum sensors for neutrino detection
Artificial-intelligence-controlled observatories
Autonomous underwater neutrino stations
Hybrid optical–radio–acoustic detection
Global ultra-high-energy neutrino maps
South Asian neutrino-astroparticle observatories
Bay of Bengal neutrino astronomy
Himalayan Earth-skimming neutrino detection
Next-generation PeV–EeV neutrino astronomy
These topics can be organized into five principal branches: cosmic-neutrino sources, neutrino propagation, particle interactions, detection technologies, and multimessenger/cosmological applications.