Neutrino Emission as Diagnostics of Core-Collapse Supernovae

Abstract

With myriads of detection events from a prospective Galactic core-collapse supernova, current and future neutrino detectors will be able to sample detailed, time-dependent neutrino fluxes and spectra. This offers enormous possibilities for inferring supernova physics from the various phases of the neutrino signal from the neutronization burst through the accretion and early explosion phase to the cooling phase. The signal will constrain the time evolution of bulk parameters of the young proto-neutron star like its mass and radius as well as the structure of the progenitor, probe multi-dimensional phenomena in the supernova core, and constrain thedynamics of the early explosion phase. Aside from further astrophysical implications, supernova neutrinos may also shed further light on the properties of matter at supranuclear densities and on open problems in particle physics.

arXiv comment26 pages, 5 figures. Accepted for publication in Annual Review of Nuclear and Particle Science, vol. 69. Non-copyedited version prepared by the author

References in corpus (147)

• A Massive Pulsar in a Compact Relativistic Binary
• Neutron Star Structure and the Equation of State
• Explosion Mechanisms of Core-Collapse Supernovae
• Neutrino Physics with JUNO
• Theory of Core-Collapse Supernovae
• Birth and Evolution of Isolated Radio Pulsars
• Stability of Standing Accretion Shocks, With an Eye Toward Core Collapse Supernovae
• On the Nature of Core Collapse Supernova Explosions
• Collective Neutrino Oscillations
• Inside the Supernova: A Powerful Convective Engine
• Evolution of Protoneutron Stars
• Monte Carlo Study of Supernova Neutrino Spectra Formation
• Explosions of O-Ne-Mg Cores, the Crab Supernova, and Subluminous Type II-P Supernovae
• Magnetorotationally driven Supernovae as the origin of early galaxy $r$-process elements?
• Neutron-star radius constraints from GW170817 and future detections
• Spin down of the core rotation in red giants
• Protoneutron star evolution and the neutrino driven wind in general relativistic neutrino radiation hydrodynamics simulations
• Physics of Core-Collapse Supernovae in Three Dimensions: a Sneak Preview
• Simulations of Magnetically-Driven Supernova and Hypernova Explosions in the Context of Rapid Rotation
• The Magnetorotational Instability in Core Collapse Supernova Explosions
• Perspectives on Core-Collapse Supernova Theory
• Two-dimensional hydrodynamic core-collapse supernova simulations with spectral neutrino transport. I. Numerical method and results for a 15 M_sun star
• Neutrino Signal of Electron-Capture Supernovae from Core Collapse to Cooling
• Delayed neutrino-driven supernova explosions aided by the standing accretion-shock instability
• A single low-energy, iron-poor supernova as the source of metals in the star SMSS J 031300.36-670839.3
• Supernova Neutrino Detection
• Supernova Simulations with Boltzmann Neutrino Transport: A Comparison of Methods
• The Supernova Channel of Super-AGB Stars
• A New Multi-Dimensional General Relativistic Neutrino Hydrodynamics Code of Core-Collapse Supernovae III. Gravitational Wave Signals from Supernova Explosion Models
• Two-Dimensional Hydrodynamic Core-Collapse Supernova Simulations with Spectral Neutrino Transport II. Models for Different Progenitor Stars
• A New Open-Source Code for Spherically-Symmetric Stellar Collapse to Neutron Stars and Black Holes
• Magnetorotational Core-Collapse Supernovae in Three Dimensions
• Electron capture rates on nuclei and implications for stellar core collapse
• Signals of the QCD phase transition in core-collapse supernovae
• Supernova Simulations from a 3D Progenitor Model -- Impact of Perturbations and Evolution of Explosion Properties
• Instability of a stalled accretion shock: evidence for the advective-acoustic cycle
• The gravitational wave burst signal from core collapse of rotating stars
• SN 2005cs in M51 II. Complete Evolution in the Optical and the Near-Infrared
• The Diffuse Supernova Neutrino Background
• Weak magnetism for antineutrinos in supernovae
• A New Multi-Dimensional General Relativistic Neutrino Hydrodynamics Code for Core-Collapse Supernovae II. Relativistic Explosion Models of Core-Collapse Supernovae
• A Simple Approach to the Supernova Progenitor-Explosion Connection
• Investigating stellar-mass black hole kicks
• The next-generation liquid-scintillator neutrino observatory LENA
• Effects of Strong and Electromagnetic Correlations on Neutrino Interactions in Dense Matter
• Supernova Neutrino Opacity from Nucleon-Nucleon Bremsstrahlung and Related Processes
• Three-Dimensional Simulations of Neutrino-Driven Core-Collapse Supernovae from Low-Mass Single and Binary Star Progenitors
• The Status of Multi-Dimensional Core-Collapse Supernova Models
• Charged-current weak interaction processes in hot and dense matter and its impact on the spectra of neutrinos emitted from proto-neutron star cooling
• 2D Multi-Angle, Multi-Group Neutrino Radiation-Hydrodynamic Simulations of Postbounce Supernova Cores
• Advanced burning stages and fate of 8-10 Mo stars
• Medium modification of the charged current neutrino opacity and its implications
• The neutrino signal from protoneutron star accretion and black hole formation
• A new multi-dimensional general relativistic neutrino hydrodynamics code for core-collapse supernovae. I. Method and code tests in spherical symmetry
• SN 2008S: an electron capture SN from a super-AGB progenitor?
• The Development of Explosions in Axisymmetric Ab Initio Core-Collapse Supernova Simulations of 12-25 $M_{\odot }$ Stars
• Muon Creation in Supernova Matter Facilitates Neutrino-driven Explosions
• Equation-of-State Dependent Features in Shock-Oscillation Modulated Neutrino and Gravitational-Wave Signals from Supernovae
• Self-sustained asymmetry of lepton-number emission: A new phenomenon during the supernova shock-accretion phase in three dimensions
• The Effects of Correlations on Neutrino Opacities in Nuclear Matter
• The multi-angle instability in dense neutrino systems
• IceCube Sensitivity for Low-Energy Neutrinos from Nearby Supernovae
• Super-AGB Stars and their role as Electron Capture Supernova progenitors
• Fornax: a Flexible Code for Multiphysics Astrophysical Simulations
• Evolution of Proto-Neutron Stars with Quarks
• Nucleon Spin Fluctuations and the Supernova Emission of Neutrinos and Axions
• Search for Supernova Neutrino Bursts at Super-Kamiokande
• High-resolution supernova neutrino spectra represented by a simple fit
• The Progenitor Dependence of the Preexplosion Neutrino Emission in Core-Collapse Supernovae
• Neutrino emission characteristics and detection opportunities based on three-dimensional supernova simulations
• A new multidimensional, energy-dependent two-moment transport code for neutrino-hydrodynamics
• Global Comparison of Core-Collapse Supernova Simulations in Spherical Symmetry
• Proto-Neutron Star Cooling with Convection: The Effect of the Symmetry Energy
• General Relativistic Three-Dimensional Multi-Group Neutrino Radiation-Hydrodynamics Simulations of Core-Collapse Supernovae
• The Dynamics of Neutrino-Driven Supernova Explosions after Shock Revival in 2D and 3D
• Flavor oscillations in the supernova hot bubble region: Nonlinear effects of neutrino background
• What can be learned from a future supernova neutrino detection?
• Quark deconfinement as supernova explosion engine for massive blue-supergiant stars
• New Supernova Limit on Large Extra Dimensions
• Dynamics and neutrino signal of black hole formation in non-rotating failed supernovae. I. EOS dependence
• A Fresh Look at Axions and SN 1987A
• Neutrino signatures of supernova shock and reverse shock propagation
• Evolution of Proto-Neutron stars with kaon condensates
• The Crab Nebula and the class of Type IIn-P supernovae caused by sub-energetic electron capture explosions
• Do electron-capture supernovae make neutron stars? First multidimensional hydrodynamic simulations of the oxygen deflagration
• Exploiting the neutronization burst of a galactic supernova
• Axial symmetry breaking in self-induced flavor conversion of supernova neutrino fluxes
• Probing axions with the neutrino signal from the next galactic supernova
• No collective neutrino flavor conversions during the supernova accretion phase
• Electron Neutrino Pair Annihilation: A New Source for Muon and Tau Neutrinos in Supernovae
• A New Multi-Energy Neutrino Radiation-Hydrodynamics Code in Full General Relativity and Its Application to Gravitational Collapse of Massive Stars
• Neutrino signature of supernova hydrodynamical instabilities in three dimensions
• Black hole formation and fallback during the supernova explosion of a $40{\mathrm{M}}_{\odot }$ star
• Interplay of Neutrino Opacities in Core-collapse Supernova Simulations
• Two Dimensional Core-Collapse Supernova Explosions Aided by General Relativity with Multidimensional Neutrino Transport
• A New Monte Carlo Method for Time-Dependent Neutrino Radiation Transport
• The millisecond pulsar mass distribution: Evidence for bimodality and constraints on the maximum neutron star mass
• Analysis of energy- and time-dependence of supernova shock effects on neutrino crossing probabilities
• Probing the neutrino mass hierarchy with the rise time of a supernova burst
• Many-Body Corrections to Charged-Current Neutrino Absorption Rates in Nuclear Matter
• Correlated Gravitational Wave and Neutrino Signals from General-Relativistic Rapidly Rotating Iron Core Collapse
• Flavor Evolution of the Neutronization Neutrino Burst from an O-Ne-Mg Core-Collapse Supernova
• Neutrino-nucleon scattering in supernova matter from the virial expansion
• Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE) Conceptual Design Report Volume 1: The LBNF and DUNE Projects
• Detection possibility of the pair-annihilation neutrinos from the neutrino-cooled pre-supernova star
• Measuring the Angular Momentum Distribution in Core-Collapse Supernova Progenitors with Gravitational Waves
• Three-Dimensional Core-Collapse Supernova Simulations with Multi-Dimensional Neutrino Transport Compared to the Ray-by-Ray-plus Approximation
• Diffuse neutrino flux from failed supernovae
• Core-collapse supernova simulations in one and two dimensions: comparison of codes and approximations
• Fast time variations of supernova neutrino fluxes and their detectability
• A New Multi-Dimensional General Relativistic Neutrino Hydrodynamics Code for Core-Collapse Supernovae IV. The Neutrino Signal
• Damping of supernova neutrino transitions in stochastic shock-wave density profiles
• Neutrino Emission from Supernovae
• Suppression of Self-Induced Flavor Conversion in the Supernova Accretion Phase
• Diffuse supernova neutrinos at underground laboratories
• Results From Core-Collapse Simulations with Multi-Dimensional, Multi-Angle Neutrino Transport
• On the Requirements for Realistic Modeling of Neutrino Transport in Simulations of Core-Collapse Supernovae
• Impact of Neutrino Opacities on Core-Collapse Supernova Simulations
• Should One Use the Ray-by-Ray Approximation in Core-Collapse Supernova Simulations?
• Probing non-standard neutrino interactions with supernova neutrinos
• Temporal Instability Enables Neutrino Flavor Conversions Deep Inside Supernovae
• Oscillation Effects and Time Variation of the Supernova Neutrino Signal
• Reconstructing the supernova bounce time with neutrinos in IceCube
• Self-induced flavor instabilities of a dense neutrino stream in a two-dimensional model
• Three-dimensional Boltzmann-Hydro code for core-collapse in massive stars II. The Implementation of moving-mesh for neutron star kicks
• Formation of the Black Hole in Nova Scorpii
• KamLAND Sensitivity to Neutrinos from Pre-Supernova Stars
• Turbulence effects on supernova neutrinos
• Multi-azimuthal-angle effects in self-induced supernova neutrino flavor conversions without axial symmetry
• Spurious instabilities in multiangle simulations of collective flavor conversion
• Reduced Neutrino Opacities and the SN 1987A Signal
• Detecting the QCD phase transition in the next Galactic supernova neutrino burst
• Fast time variations of supernova neutrino signals from 3-dimensional models
• Neutrino Signals of Core-Collapse Supernovae in Underground Detectors
• Presupernova neutrino events relating to the final evolution of massive stars
• Presupernova neutrinos: realistic emissivities from stellar evolution
• Neutrino oscillation signatures of oxygen-neon-magnesium supernovae
• Impact of sterile neutrinos on the early time flux from a galactic supernova
• The Impact of Different Neutrino Transport Methods on Multidimensional Core-collapse Supernova Simulations
• Impact of Nucleon-Nucleon Bremsstrahlung Rates Beyond One-Pion Exchange
• Probing Rotation of Core-collapse Supernova with Concurrent Analysis of Gravitational Waves and Neutrinos
• Linear stability analysis of collective neutrino oscillations without spurious modes
• Identifying rotation in SASI-dominated core-collapse supernovae with a neutrino gyroscope
• Supernova Neutrino Scattering Rates Reduced by Nucleon Spin Fluctuations: Perturbative Limit
• Estimating the core compactness of massive stars with Galactic supernova neutrinos
• Nuclear pasta and supernova neutrinos at late times
• Diagnosing the Structure of Massive Stars with Galactic Supernova Neutrinos

Cited by in corpus (47)

• Hydrodynamics of core-collapse supernovae and their progenitors
• Temporal and Angular Variations of 3D Core-Collapse Supernova Emissions and their Physical Correlations
• A new possibility of the fast neutrino-flavor conversion in the pre-shock region of core-collapse supernova
• The Science of the Einstein Telescope
• Fast Neutrino Flavor Conversion in Core-Collapse Supernovae: A Parametric Study in 1D Models
• Roles of fast neutrino-flavor conversion on the neutrino-heating mechanism of core-collapse supernova
• Core-collapse supernova neutrino emission and detection informed by state-of-the-art three-dimensional numerical models
• Neutrino emission characteristics of black hole formation in three-dimensional simulations of stellar collapse
• The Collapse and Three-Dimensional Explosion of Three-Dimensional, vis à vis One-Dimensional, Massive-star Supernova Progenitor Models
• Gravitational Waves from Neutrino Asymmetries in Core-Collapse Supernovae
• RES-NOVA: A new neutrino observatory based on archaeological lead
• Characteristic Time Variability of Gravitational-Wave and Neutrino Signals from Three-dimensional Simulations of Non-Rotating and Rapidly Rotating Stellar Core-Collapse
• The final core collapse of pulsational pair instability supernovae
• Revisiting the explodability of single massive star progenitors of stripped-envelope supernovae
• New method for detecting fast neutrino flavor conversions in core-collapse supernova models with two-moment neutrino transport
• Nuclear de-excitations in low-energy charged-current ${\nu }_e$ scattering on ${}^{40}$Ar
• Multimessenger Asteroseismology of Core-Collapse Supernovae
• Nucleosynthesis of an $11.8M_{\odot }$ Supernova with 3D Simulation of the Inner Ejecta: Overall Yields and Implications for Short-Lived Radionuclides in the Early Solar System
• Cosmic nucleosynthesis: a multi-messenger challenge
• A New Approach to Mass and Radius of Neutron Stars with Supernova Neutrinos
• Progenitor Dependence of Hadron-quark Phase Transition in Failing Core-collapse Supernovae
• Observing Supernova Neutrino Light Curves with Super-Kamiokande. II. Impact of the Nuclear Equation of State
• Post-explosion evolution of core-collapse supernovae
• Measuring the properties of $f-$mode oscillations of a protoneutron star by third generation gravitational-wave detectors
• The stochastic enrichment of Population II stars
• Neutrino transport with Monte Carlo method: I. Towards fully consistent implementation of nucleon recoils in core-collapse supernova simulations
• Analytic solutions for neutrino-light curves of core-collapse supernovae
• Non-thermal neutrinos created by shock acceleration in successful and failed core-collapse supernova
• Inferring physical properties of stellar collapse by third-generation gravitational-wave detectors
• Leptonic and semi-leptonic neutrino interactions with muons in the proto-neutron star cooling
• Standing Accretion Shock Instability in the Collapse of a Rotating Stellar Core
• Effects of nuclear matter and composition in core-collapse supernovae and long-term proto-neutron star cooling
• Inference of neutrino flavor evolution through data assimilation and neural differential equations
• Impact of Rotation on the Multimessenger Signatures of a Hadron-quark Phase Transition in Core-collapse Supernovae
• Light Curves of Type IIP Supernovae from Neutrino-driven Explosions of Red Supergiants Obtained by a Semi-analytic Approach
• Equation of state in neutron stars and supernovae
• Prospects for reconstructing the gravitational-wave signals from core-collapse supernovae with Advanced LIGO-Virgo and the BayesWave algorithm
• Triangulating Black Hole Forming Stellar Collapses through Neutrinos
• Evolving massive stars to core collapse with GENEC: Extension of equation of state, opacities and effective nuclear network
• Simple fits for the neutrino luminosities from protoneutron star cooling
• Observing Supernova Neutrino Light Curves with Super-Kamiokande. V. Distance Estimation with Neutrinos
• Sequency Hierarchy Truncation (SeqHT) for Adiabatic State Preparation and Time Evolution in Quantum Simulations
• Supernovae neutrino detection via coherent scattering off silicon nuclei
• Taking Neutrino Pictures via Electrons
• Collapsar Disk Outflows III: Detectable Neutrino and Gravitational Wave Signatures
• Neutrino transport with Monte Carlo method: II. Quantum Kinetic Equations
• Inference of bipolar neutrino flavor oscillations near a core-collapse supernova, based on multiple measurements at Earth