Three-flavor collective neutrino conversions with multi-azimuthal-angle instability in an electron-capture supernova model
arXiv:2011.09635 · doi:10.1103/PhysRevD.103.063008
Abstract
We investigate the multi-azimuthal angle (MAA) effect on collective neutrino oscillation by considering the three-dimensional neutrino momentum distribution in a realistic electron-capture supernova model with an progenitor. We find that the MAA effect induces collective flavor conversions at epochs when it is completely suppressed under the axial-symmetric approximation. This novel activity is switched on/off by the growth of the MAA instability and imprints additional time evolution in the expected neutrino event rate. We validate our results by extending the linear stability analysis into the three-flavor scheme including mixing angles, and confirm that the onset of collective neutrino oscillation matches the steep growth of flavor instability. We discuss how the MAA effect alters neutrino detection at Super-Kamiokande and DUNE.
arXiv comment15 pages with 28 figures, Version accepted in Phys. Rev. D
References in corpus (62)
- The fate of hints: updated global analysis of three-flavor neutrino oscillations
- Collective Neutrino Oscillations
- Monte Carlo Study of Supernova Neutrino Spectra Formation
- Explosions of O-Ne-Mg Cores, the Crab Supernova, and Subluminous Type II-P Supernovae
- Nuclear weak-interaction processes in stars
- Simulation of Coherent Non-Linear Neutrino Flavor Transformation in the Supernova Environment I: Correlated Neutrino Trajectories
- Perspectives on Core-Collapse Supernova Theory
- Precise quasielastic neutrino/nucleon cross section
- Global constraints on absolute neutrino masses and their ordering
- Supernova Neutrino Detection
- The Physics of Core-Collapse Supernovae
- Explosion Mechanism, Neutrino Burst, and Gravitational Wave in Core-Collapse Supernovae
- Speed-up of neutrino transformations in a supernova environment
- Collective neutrino flavor transitions in supernovae and the role of trajectory averaging
- Multiple Spectral Splits of Supernova Neutrinos
- Fast Pairwise Conversion of Supernova Neutrinos: A Dispersion-Relation Approach
- Current unknowns in the three neutrino framework
- Collective neutrino flavor conversion: Recent developments
- The isotropic diffusion source approximation for supernova neutrino transport
- Neutrino Mass Ordering from Oscillations and Beyond: 2018 Status and Future Prospects
- High-resolution supernova neutrino spectra represented by a simple fit
- 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
- Linearized flavor-stability analysis of dense neutrino streams
- Global Comparison of Core-Collapse Supernova Simulations in Spherical Symmetry
- Three-dimensional simulations of rapidly rotating core-collapse supernovae: finding a neutrino-powered explosion aided by non-axisymmetric flows
- Self-induced neutrino flavor conversion without flavor mixing
- Decoherence in supernova neutrino transformations suppressed by deleptonization
- What can be learned from a future supernova neutrino detection?
- Collective three-flavor oscillations of supernova neutrinos
- Fast neutrino flavor conversions near the supernova core with realistic flavor-dependent angular distributions
- Axial symmetry breaking in self-induced flavor conversion of supernova neutrino fluxes
- On the occurrence of fast neutrino flavor conversions in multidimensional supernova models
- Fast Neutrino Flavor Instability in the Neutron-star Convection Layer of Three-dimensional Supernova Models
- Neutrino scattering and flavor transformation in supernovae
- Fast collective neutrino oscillations inside the neutrino sphere in core-collapse supernovae
- A new possibility of the fast neutrino-flavor conversion in the pre-shock region of core-collapse supernova
- Addendum to: Global constraints on absolute neutrino masses and their ordering
- Effects of neutrino oscillations on nucleosynthesis and neutrino signals for an 18 M supernova model
- Self-refraction of supernova neutrinos: mixed spectra and three-flavor instabilities
- Supernova Explosions of Super-Asymptotic Giant Branch Stars: Multicolor Light Curves of Electron-Capture Supernovae
- Neutrino mass hierarchy and three-flavor spectral splits of supernova neutrinos
- Temporal Instability Enables Neutrino Flavor Conversions Deep Inside Supernovae
- Halo Modification of a Supernova Neutronization Neutrino Burst
- Back to (Mass-)Square(d) One: The Neutrino Mass Ordering in Light of Recent Data
- Three flavor neutrino conversions in supernovae: Slow Fast instabilities
- Multi-azimuthal-angle effects in self-induced supernova neutrino flavor conversions without axial symmetry
- Damping the neutrino flavor pendulum by breaking homogeneity
- Self-induced flavor conversion of supernova neutrinos on small scales
- Long-term Simulations of Multi-Dimensional Core-collapse Supernovae: Implications for Neutron Star Kicks
- Possible effects of collective neutrino oscillations in the three flavor multi-angle simulations on supernova process
- Multi-azimuthal-angle instability for different supernova neutrino fluxes
- Multi-angle effects in self-induced oscillations for different supernova neutrino fluxes
- Multi-Angle Simulation of Flavor Evolution in the Neutrino Neutronization Burst From an O-Ne-Mg Core-Collapse Supernova
- Suppression of the multi-azimuthal-angle instability in dense neutrino gas during supernova accretion phase
- Neutrino halo effect on collective neutrino oscillation in iron core-collapse supernova model of a 9.6 star
- Neutrino Capture Reactions on Ar
- Self-induced temporal instability from a neutrino antenna
- Stability of three neutrino flavor conversion in supernovae
- Collective neutrino oscillations with the halo effect in single-angle approximation
- Detectability of Collective Neutrino Oscillation Signatures in the Supernova Explosion of a 8.8 star
- Collective neutrino oscillations and detectabilities in failed supernovae
Cited by in corpus (10)
- Simple method for determining asymptotic states of fast neutrino-flavor conversion
- Code Comparison for Fast Flavor Instability Simulation
- Three-dimensional simulation of a core-collapse supernova for a binary star progenitor of SN 1987A
- Dynamics of fast neutrino flavor conversions with scattering effects: a detailed analysis
- General-Relativistic Quantum-Kinetics Neutrino Transport
- Flavor Triangle of the Diffuse Supernova Neutrino Background
- Fast Flavor Transformations
- Neutrino-antineutrino oscillations induced by strong magnetic fields in dense matter
- Symmetry and bipolar motion in collective neutrino flavor oscillations
- Nonlinear evolution of fast neutrino flavor conversion in the preshock region of core-collapse supernovae