Imagen de Portada

Approximate Energy-Integration Method for Identifying Collisional Neutrino Flavor Instabilities

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Liu, Jiabao, Nagakura, Hiroki
Formato:	Preprint
Publicado:	2026
Materias:	High Energy Astrophysical Phenomena High Energy Physics - Phenomenology
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Dynamic Competition of Fast and Collisional Neutrino Flavor Instabilities with Collisional Damping in Spatially Inhomogeneous Systems
por: Takahashi, Shota, et al.
Publicado: (2026)

Detecting Fast Neutrino Flavor Conversions with Machine Learning
por: Abbar, Sajad, et al.
Publicado: (2023)

Fast Neutrino-Flavor Conversion with Attenuation and Global Lepton Gradient
por: Zaizen, Masamichi, et al.
Publicado: (2026)

Universality of the Neutrino Collisional Flavor Instability in Core Collapse Supernovae
por: Liu, Jiabao, et al.
Publicado: (2023)

Collisional and Fast Neutrino Flavor Instabilities in Two-dimensional Core-collapse Supernova Simulation with Boltzmann Neutrino Transport
por: Akaho, Ryuichiro, et al.
Publicado: (2023)

Collisional flavor swap with neutrino self-interactions
por: Kato, Chinami, et al.
Publicado: (2023)

Resolution requirements for numerical modeling of neutrino quantum kinetics
por: Nagakura, Hiroki, et al.
Publicado: (2025)

Detectability of Late-time Supernova Neutrinos with Fallback Accretion onto Protoneutron star
por: Akaho, Ryuichiro, et al.
Publicado: (2023)

Energy Dependence of Flavor Instabilities Stemming from Crossings in the Neutrino Flavor Lepton Number Angular Distribution
por: Neto, Pedro Dedin, et al.
Publicado: (2023)

Asymptotic states of fast neutrino-flavor conversions in the three-flavor framework
por: Liu, Jiabao, et al.
Publicado: (2025)

Two-Moment Neutrino Flavor Transformation with applications to the Fast Flavor Instability in Neutron Star Mergers
por: Grohs, Evan, et al.
Publicado: (2023)

Quasi-steady evolution of fast neutrino-flavor conversions
por: Liu, Jiabao, et al.
Publicado: (2024)

Fast neutrino-flavor swap in high-energy astrophysical environments
por: Zaizen, Masamichi, et al.
Publicado: (2023)

The Effect of the Collisional Flavor Instability on Core-Collapse Supernova Models
por: Wang, Tianshu, et al.
Publicado: (2025)

Muon-induced collisional flavor instability in core-collapse supernova
por: Liu, Jiabao, et al.
Publicado: (2024)

Neutrino-Mass-Driven Instabilities as the Earliest Flavor Conversion in Supernovae
por: Fiorillo, Damiano F. G., et al.
Publicado: (2025)

Machine Learning-Based Detection of Non-Axisymmetric Fast Neutrino Flavor Instabilities in Core-Collapse Supernovae
por: Abbar, Sajad, et al.
Publicado: (2024)

Fast Flavor Pendulum: Instability Condition
por: Fiorillo, Damiano F. G., et al.
Publicado: (2024)

Perturbing Fast Neutrino Flavor Conversion
por: Cornelius, Marie, et al.
Publicado: (2023)

Core-collapse supernova explosions hindered by eV-mass sterile neutrinos
por: Mori, Kanji, et al.
Publicado: (2025)

Flavor Matters, but Matter Flavors: Matter Effects on Flavor Composition of Astrophysical Neutrinos
por: Dev, P. S. Bhupal, et al.
Publicado: (2023)

Flavor Anisotropy in the High-Energy Astrophysical Neutrino Sky
por: Telalovic, Bernanda, et al.
Publicado: (2023)

Flavor Equilibration of Supernova Neutrinos: Exploring the Dynamics of Slow Modes
por: Padilla-Gay, Ian, et al.
Publicado: (2025)

Inspecting neutrino flavor instabilities during proto-neutron star cooling phase in supernova: I. Spherically symmetric model
por: Zaizen, Masamichi, et al.
Publicado: (2024)

Resonant Spin-Flavor Precession of Sterile Neutrinos
por: Wang, Edward
Publicado: (2023)

No Flavor Anisotropy in the High-Energy Neutrino Sky Upholds Lorentz Invariance
por: Telalovic, Bernanda, et al.
Publicado: (2025)

Characterization of the Three-Flavor Composition of Cosmic Neutrinos with IceCube
por: Abbasi, R., et al.
Publicado: (2025)

Do Neutrinos Become Flavor Unstable Due to Collisions with Matter in the Supernova Decoupling Region?
por: Shalgar, Shashank, et al.
Publicado: (2023)

Neutron star kick driven by asymmetric fast-neutrino flavor conversion
por: Nagakura, Hiroki, et al.
Publicado: (2024)

Pseudo-Dirac Neutrinos and Relic Neutrino Matter Effect on the High-energy Neutrino Flavor Composition
por: Dev, P. S. Bhupal, et al.
Publicado: (2024)

Comparative Testing of Subgrid Models for Fast Neutrino Flavor Conversions in Core-collapse Supernova Simulations
por: Akaho, Ryuichiro, et al.
Publicado: (2025)

Bifurcated Impact of Neutrino Fast Flavor Conversion on Core-collapse Supernovae Informed by Multi-angle Neutrino Radiation Hydrodynamics
por: Akaho, Ryuichiro, et al.
Publicado: (2026)

Oscillations of High-Energy Cosmic Neutrinos in the Copious MeV Neutrino Background
por: Abbar, Sajad, et al.
Publicado: (2022)

Particle Astrophysics with High and Ultrahigh Energy Neutrinos
por: Fang, Ke, et al.
Publicado: (2025)

Multimessenger Characterization of High-Energy Neutrino Emission from the Brightest Neutrino-Active Galactic Nuclei
por: Carpio, Jose Alonso, et al.
Publicado: (2026)

Neutrino Flavor Conversion Shapes the Rate of Failed Core-collapse Supernovae
por: Gogilashvili, Mariam, et al.
Publicado: (2026)

Dynamical equilibria of fast neutrino flavor conversion
por: Liu, Jiabao, et al.
Publicado: (2025)

Using Bayesian Inference to Distinguish Neutrino Flavor Conversion Scenarios via a Prospective Supernova Neutrino Signal
por: Abbar, Sajad, et al.
Publicado: (2024)

Low-Energy Supernova Constraints on Lepton Flavor Violating Axions
por: Huang, Zi-Miao, et al.
Publicado: (2025)

Cherenkov Telescope Arrays for High-Energy Neutrino Detection in Mountain Ranges
por: Bitam, Tariq, et al.
Publicado: (2024)