Roles of fast neutrino-flavor conversion on the neutrino-heating mechanism of core-collapse supernova
arXiv:2301.10785 · doi:10.1103/PhysRevLett.130.211401
Abstract
One of the greatest uncertainties in any modeling of inner engine of core-collapse supernova (CCSN) is neutrino flavor conversions driven by neutrino self-interactions. We carry out large-scale numerical simulations of multi-energy, multi-angle, three-flavor framework, and general relativistic quantum kinetic neutrino transport in spherical symmetry with an essential set of neutrino-matter interactions under a realistic fluid profile of CCSN. Our result suggests that the neutrino heating in the gain region is reduced by due to fast neutrino-flavor conversion (FFC). We also find that the total luminosity of neutrinos is enhanced by , for which the substantial increase of heavy-leptonic neutrinos by FFCs are mainly responsible. This study provides evidence that FFC has a significant impact on the delayed neutrino-heating mechanism.
Accepted to PRL
References in corpus (22)
- Core-Collapse Supernova Explosion Theory
- New Developments in Flavor Evolution of a Dense Neutrino Gas
- Fast-pairwise collective neutrino oscillations associated with asymmetric neutrino emissions in core-collapse supernova
- A systematic study of proto-neutron star convection in three-dimensional core-collapse supernova simulations
- On the characteristics of fast neutrino flavor instabilities in three-dimensional core-collapse supernova models
- Fast flavor oscillations in dense neutrino media with collisions
- The Neutrino Fast Flavor Instability in Three Dimensions
- Time-dependent and quasi-steady features of fast neutrino-flavor conversion
- A change of direction in pairwise neutrino conversion physics: The effect of collisions
- Neutrino Flavor Conversions in High-Density Astrophysical and Cosmological Environments
- A new equation of state for core-collapse supernovae based on realistic nuclear forces and including a full nuclear ensemble
- Evolution of collisional neutrino flavor instabilities in spherically symmetric supernova models
- Simulations of Fast Neutrino Flavor Conversions with Interactions in Inhomogeneous Media
- The Fast Flavor Instability in Hypermassive Neutron Star Disk Outflows
- Prospects of fast flavor neutrino conversion in rotating core-collapse supernovae
- Comparing treatments of weak reactions with nuclei in simulations of core-collapse supernovae
- Dynamics of fast neutrino flavor conversions with scattering effects: a detailed analysis
- Neutrino Flavor Conversion, Advection, and Collisions: Towards the Full Solution
- Connecting small-scale to large-scale structures of fast neutrino-flavor conversion
- General-Relativistic Quantum-Kinetics Neutrino Transport
- Effects of energy-dependent scatterings on fast neutrino flavor conversions
- Fast Neutrino Conversion in Hydrodynamic Simulations of Neutrino-Cooled Accretion Disks
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- Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions
- Evaluating approximate asymptotic distributions for fast neutrino flavor conversions in a periodic 1D box
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- Flavor solitons in dense neutrino gases
- Collisional and Fast Neutrino Flavor Instabilities in Two-dimensional Core-collapse Supernova Simulation with Boltzmann Neutrino Transport
- Neutrino Oscillations in Core-Collapse Supernovae and Neutron Star Mergers
- Universality of the Neutrino Collisional Flavor Instability in Core Collapse Supernovae
- Neutrino fast flavor oscillations with moments: linear stability analysis and application to neutron star mergers
- Fast neutrino flavor conversions in a supernova: Emergence, evolution, and effects
- Fast flavor conversions at the edge of instability in a two-beam model
- Two-Moment Neutrino Flavor Transformation with applications to the Fast Flavor Instability in Neutron Star Mergers
- Perturbing Fast Neutrino Flavor Conversion
- Robust integration of fast flavor conversions in classical neutrino transport
- Asymptotic states of fast neutrino-flavor conversions in the three-flavor framework
- Flavor conversions with energy-dependent neutrino emission and absorption
- Neutrinos from explosive transients at the dawn of multi-messenger astronomy
- Evolution and the quasistationary state of collective fast neutrino flavor conversion in three dimensions without axisymmetry
- Fast neutrino-flavor swap in high-energy astrophysical environments
- Quasi-steady evolution of fast neutrino-flavor conversions
- Spectral diversity in collisional neutrino-flavor conversion: flavor equipartition or swap
- Thermodynamics of oscillating neutrinos
- Flavor Equilibration of Supernova Neutrinos: Exploring the Dynamics of Slow Modes
- Neutrino-driven massive stellar explosions in 3D fostered by magnetic fields via turbulent -effect
- Muon-induced collisional flavor instability in core-collapse supernova
- Comparative Testing of Subgrid Models for Fast Neutrino Flavor Conversions in Core-collapse Supernova Simulations
- Quantum Closures for Neutrino Moment Transport
- Neutrino quantum kinetics in two spatial dimensions
- Predicting the outcome of collisional neutrino flavor conversion
- Diagnosing electron-neutrino lepton number crossings in core-collapse supernovae: A comparison of methods
- Advection Algorithms for Quantum Neutrino Moment Transport
- Gravitational-Wave Signatures of Nonstandard Neutrino Properties in Collapsing Stellar Cores
- Flavor composition of supernova neutrinos
- Steady state of fast-oscillating neutrinos in an inhomogeneous medium
- Systematic local simulations of fast neutrino flavor conversions with scattering effects
- Electron-neutrino lepton number crossings: Variations with the supernova core physics
- Approximate Energy-Integration Method for Identifying Collisional Neutrino Flavor Instabilities
- Neutrino quantum kinetics in three flavors
- Comprehensive neutrino light curves and spectra: from pre-supernova evolution to early supernova phase