Neutrino signature of supernova hydrodynamical instabilities in three dimensions

Abstract

The first full-scale three-dimensional (3D) core-collapse supernova (SN) simulations with sophisticated neutrino transport show pronounced effects of the standing accretion shock instability (SASI) for two high-mass progenitors (20 and 27 M_sun). In a low-mass progenitor (11.2 M_sun), large-scale convection is the dominant nonradial hydrodynamic instability in the postshock accretion layer. The SASI-associated modulation of the neutrino signal (80 Hz in our two examples) will be clearly detectable in IceCube or the future Hyper-Kamiokande detector, depending on progenitor properties, distance, and observer location relative to the main SASI sloshing direction. The neutrino signal from the next galactic SN can therefore diagnose the nature of the hydrodynamic instability.

6 pages, including 4 figures. Results unchanged. Matches published version in PRL. Animated visualization available at: http://www.mpa-garching.mpg.de/ccsnarchive/data/Hanke2013_movie/index.html

References in corpus (15)

• Nucleosynthesis and Remnants in Massive Stars of Solar Metallicity
• Delayed neutrino-driven supernova explosions aided by the standing accretion-shock instability
• Pulsar spins from an instability in the accretion shock of supernovae
• Criteria for Core-Collapse Supernova Explosions by the Neutrino Mechanism
• Multidimensional supernova simulations with approximative neutrino transport. II. Convection and the advective-acoustic cycle in the supernova core
• Equation-of-State Dependent Features in Shock-Oscillation Modulated Neutrino and Gravitational-Wave Signals from Supernovae
• Role of dense matter in collective supernova neutrino transformations
• Axial symmetry breaking in self-induced flavor conversion of supernova neutrino fluxes
• Hydrodynamical Neutron Star Kicks in Three Dimensions
• Neutrino scattering and flavor transformation in supernovae
• Analysis of matter suppression in collective neutrino oscillations during the supernova accretion phase
• Effects of Rotation on Standing Accretion Shock Instability in Nonlinear Phase for Core-Collapse Supernovae
• Supernova neutrino halo and the suppression of self-induced flavor conversion
• Earth matter effects in supernova neutrinos: Optimal detector locations
• Neutrino flavor pendulum in both mass hierarchies

Cited by in corpus (77)

• Physics of Core-Collapse Supernovae in Three Dimensions: a Sneak Preview
• Neutrino-driven explosion of a 20 solar-mass star in three dimensions enabled by strange-quark contributions to neutrino-nucleon scattering
• Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae
• Characterizing the Gravitational Wave Signal from Core-Collapse Supernovae
• Hydrodynamics of core-collapse supernovae and their progenitors
• The Development of Explosions in Axisymmetric Ab Initio Core-Collapse Supernova Simulations of 12-25 $M_{\odot }$ Stars
• Neutrino Quantum Kinetics
• Gravitational Wave Signals from 3D Neutrino Hydrodynamics Simulations of Core-Collapse Supernovae
• Self-sustained asymmetry of lepton-number emission: A new phenomenon during the supernova shock-accretion phase in three dimensions
• Grand Unified Neutrino Spectrum at Earth: Sources and Spectral Components
• The explosion mechanism of core-collapse supernovae: progress in supernova theory and experiments
• Neutrino emission characteristics and detection opportunities based on three-dimensional supernova simulations
• What can be learned from a future supernova neutrino detection?
• A New Gravitational-Wave Signature from Standing Accretion Shock Instabilities in Supernovae
• Multi-messenger signals of long-term core-collapse supernova simulations : synergetic observation strategies
• Progenitor-dependent Explosion Dynamics in Self-consistent, Axisymmetric Simulations of Neutrino-driven Core-collapse Supernovae
• Gravitational waves from three-dimensional core-collapse supernova models: The impact of moderate progenitor rotation
• Supernova neutrino physics with xenon dark matter detectors: A timely perspective
• Magnetorotational Explosion of A Massive Star Supported by Neutrino Heating in General Relativistic Three Dimensional Simulations
• Temporal and Angular Variations of 3D Core-Collapse Supernova Emissions and their Physical Correlations
• Neutrino-driven Explosions
• Correlated Signatures of Gravitational-Wave and Neutrino Emission in Three-Dimensional General-Relativistic Core-Collapse Supernova Simulations
• Two-Dimensional Core-Collapse Supernova Models with Multi-Dimensional Transport
• Gravitational-wave signal of a core-collapse supernova explosion of a 15 Solar mass star
• The Science of the Einstein Telescope
• Anisotropic emission of neutrino and gravitational-wave signals from rapidly rotating core-collapse supernovae
• Neutrino Emission from Supernovae
• Supernova Model Discrimination with Hyper-Kamiokande
• Core-collapse supernova neutrino emission and detection informed by state-of-the-art three-dimensional numerical models
• Three-Dimensional Simulations of SASI- and Convection-Dominated Core-Collapse Supernovae
• Should One Use the Ray-by-Ray Approximation in Core-Collapse Supernova Simulations?
• Neutrino Emission as Diagnostics of Core-Collapse Supernovae
• Neutrino emission characteristics of black hole formation in three-dimensional simulations of stellar collapse
• Snowmass White Paper: Beyond the Standard Model effects on Neutrino Flavor
• An advanced leakage scheme for neutrino treatment in astrophysical simulations
• Gravitational Waves from Neutrino Asymmetries in Core-Collapse Supernovae
• Core-collapse supernova simulations and the formation of neutron stars, hybrid stars, and black holes
• Characteristic Time Variability of Gravitational-Wave and Neutrino Signals from Three-dimensional Simulations of Non-Rotating and Rapidly Rotating Stellar Core-Collapse
• Multi-azimuthal-angle effects in self-induced supernova neutrino flavor conversions without axial symmetry
• Self-induced flavor conversion of supernova neutrinos on small scales
• Supernova neutrino signals based on long-term axisymmetric simulations
• Observing Supernova Neutrino Light Curves with Super-Kamiokande: Expected Event Number over 10 s
• The KM3NeT potential for the next core-collapse supernova observation with neutrinos
• Gadolinium in water Cherenkov detectors improves detection of supernova ${\nu }_e$
• Neutrino Signals of Core-Collapse Supernovae in Underground Detectors
• Multi-azimuthal-angle instability for different supernova neutrino fluxes
• Three-dimensional core-collapse supernovae with complex magnetic structures: II. Rotational instabilities and multi-messenger signatures
• New method for detecting fast neutrino flavor conversions in core-collapse supernova models with two-moment neutrino transport
• The Boltzmann-radiation-hydrodynamics Simulations of Core-collapse Supernovae with Different Equations of State: the Role of Nuclear Composition and the Behavior of Neutrinos
• Effects of the standing accretion-shock instability and the lepton-emission self-sustained asymmetry in the neutrino emission of rotating supernovae
• Multimessenger Asteroseismology of Core-Collapse Supernovae
• Identifying rotation in SASI-dominated core-collapse supernovae with a neutrino gyroscope
• Circular polarization of gravitational waves from non-rotating supernova cores: a new probe into the pre-explosion hydrodynamics
• Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos
• Robust measurement of supernova ${\nu }_e$ spectra with future neutrino detectors
• The neutrino gravitational memory from a core collapse supernova: phenomenology and physics potential
• Detectability of SASI activity in supernova neutrino signals
• Effect of stellar rotation on the development of post-shock instabilities during core-collapse supernovae
• Nuclear pasta and supernova neutrinos at late times
• Application of the Hilbert-Huang transform for analyzing standing-accretion-shock-instability induced gravitational waves in a core-collapse supernova
• Neutrinos from explosive transients at the dawn of multi-messenger astronomy
• Late time supernova neutrino signal and proto-neutron star radius
• The non-linear onset of neutrino-driven convection in two and three-dimensional core-collapse supernovae
• Multi-messenger observations of core-collapse supernovae: Exploiting the standing accretion shock instability
• Standing Accretion Shock Instability in the Collapse of a Rotating Stellar Core
• Multipole expansion method for supernova neutrino oscillations
• Sensitivity of multi-PMT Optical Modules in Antarctic Ice to Supernova Neutrinos of MeV energy
• 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
• Characterization and Optimization of a Cryogenic Pure CsI Detector with Remarkable Light Yield and Unprecedented Energy Resolution for CLOVERS Experiment
• Timing coincidence search for supernova neutrinos with optical transient surveys
• Collapsar Disk Outflows III: Detectable Neutrino and Gravitational Wave Signatures
• Simulating fast time variations in the supernova neutrino flux in Hyper-Kamiokande
• Status and Perspectives of Neutrino Physics
• Matter- and magnetically-driven flavor conversion of neutrinos in magnetorotational collapses
• FRIB and the GW170817 Kilonova
• Joint Detection and Characterization of the Standing Accretion Shock Instability for Core-Collapse Supernovae with cWB XP