Neutrino Signals of Core-Collapse Supernovae in Underground Detectors

Abstract

For a suite of fourteen core-collapse models during the dynamical first second after bounce, we calculate the detailed neutrino "light" curves expected in the underground neutrino observatories Super-Kamiokande, DUNE, JUNO, and IceCube. These results are given as a function of neutrino-oscillation modality (normal or inverted hierarchy) and progenitor mass (specifically, post-bounce accretion history), and illuminate the differences between the light curves for 1D (spherical) models that don't explode with the corresponding 2D (axisymmetric) models that do. We are able to identify clear signatures of explosion (or non-explosion), the post-bounce accretion phase, and the accretion of the silicon/oxygen interface. In addition, we are able to estimate the supernova detection ranges for various physical diagnostics and the distances out to which various temporal features embedded in the light curves might be discerned. We find that the progenitor mass density profile and supernova dynamics during the dynamical explosion stage should be identifiable for a supernova throughout most of the galaxy in all the facilities studied and that detection by any one of them, but in particular more than one in concert, will speak volumes about the internal dynamics of supernovae.

arXiv commentAccepted to Monthly Notices of the Royal Astronomical Society

References in corpus (55)

• Neutrino Physics with JUNO
• Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions
• Black Hole Formation in Failing Core-Collapse Supernovae
• Core-collapse supernova equations of state based on neutron star observations
• Nucleosynthesis and Remnants in Massive Stars of Solar Metallicity
• Stability of Standing Accretion Shocks, With an Eye Toward Core Collapse Supernovae
• On the Nature of Core Collapse Supernova Explosions
• Identifying the neutrino mass spectrum from a supernova neutrino burst
• GADZOOKS! Antineutrino Spectroscopy with Large Water Cerenkov Detectors
• Perspectives on Core-Collapse Supernova Theory
• Hyper-Kamiokande Design Report
• Global constraints on absolute neutrino masses and their ordering
• Supernova Neutrino Detection
• Shock Breakout in Core-Collapse Supernovae and its Neutrino Signature
• Letter of Intent: The Hyper-Kamiokande Experiment --- Detector Design and Physics Potential ---
• Collective Neutrino Flavor Transformation In Supernovae
• Stellar evolution with rotation XII: Pre-supernova models
• Exploring the relativistic regime with Newtonian hydrodynamics: An improved effective gravitational potential for supernova simulations
• Neutrino Opacities in Nuclear Matter
• The neutrino signal from protoneutron star accretion and black hole formation
• The gravitational wave signal from core-collapse supernovae
• IceCube Sensitivity for Low-Energy Neutrinos from Nearby Supernovae
• The Progenitor Dependence of the Preexplosion Neutrino Emission in Core-Collapse Supernovae
• Neutrino emission characteristics and detection opportunities based on three-dimensional supernova simulations
• What can be learned from a future supernova neutrino detection?
• Multi-messenger signals of long-term core-collapse supernova simulations : synergetic observation strategies
• Electron-Capture and Low-Mass Iron-Core-Collapse Supernovae: New Neutrino-Radiation-Hydrodynamics Simulations
• Crucial Physical Dependencies of the Core-Collapse Supernova Mechanism
• Neutrino signature of supernova hydrodynamical instabilities in three dimensions
• An Investigation into the Character of Pre-Explosion Core-Collapse Supernova Shock Motion
• Neutrino signals from the formation of black hole: a probe of equation of state of dense matter
• 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
• Neutrino-nucleon scattering in supernova matter from the virial expansion
• Revival of the Fittest: Exploding Core-Collapse Supernovae from 12 to 25 M${}_{\odot }$
• The Role of Collective Neutrino Flavor Oscillations in Core-Collapse Supernova Shock Revival
• Real-Time Supernova Neutrino Burst Monitor at Super-Kamiokande
• 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
• Suppression of Self-Induced Flavor Conversion in the Supernova Accretion Phase
• Should One Use the Ray-by-Ray Approximation in Core-Collapse Supernova Simulations?
• Supernova Signatures of Neutrino Mass Ordering
• Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE) Conceptual Design Report, Volume 4 The DUNE Detectors at LBNF
• What can we learn on supernova neutrino spectra with water Cherenkov detectors?
• Gadolinium in water Cherenkov detectors improves detection of supernova ${\nu }_e$
• Neutrino emissions in all flavors up to the pre-bounce of massive stars and the possibility of their detections
• Neutrino Signals of Core-Collapse Supernovae in Underground Detectors
• Constraining Absolute Neutrino Masses via Detection of Galactic Supernova Neutrinos at JUNO
• Detecting the Supernova Breakout Burst in Terrestrial Neutrino Detectors
• Robust measurement of supernova ${\nu }_e$ spectra with future neutrino detectors
• Quantum Size Effects in the Atomistic Structure of Armchair-Nanoribbons
• Supernova Physics at DUNE
• Estimating the core compactness of massive stars with Galactic supernova neutrinos
• Neutrino oscillation and expected event rate of supernova neutrinos in adiabatic explosion model
• The Deep Underground Neutrino Experiment -- DUNE: the precision era of neutrino physics

Cited by in corpus (34)

• Core-Collapse Supernova Explosion Theory
• A Successful 3D Core-Collapse Supernova Explosion Model
• Is there a supernova bound on axions?
• Fornax: a Flexible Code for Multiphysics Astrophysical Simulations
• Temporal and Angular Variations of 3D Core-Collapse Supernova Emissions and their Physical Correlations
• Fast Flavor Depolarization of Supernova Neutrinos
• Fast-pairwise collective neutrino oscillations associated with asymmetric neutrino emissions in core-collapse supernova
• Supernova Model Discrimination with Hyper-Kamiokande
• Core-collapse supernova neutrino emission and detection informed by state-of-the-art three-dimensional numerical models
• Neutrino Emission as Diagnostics of Core-Collapse Supernovae
• 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
• Constraining properties of the next nearby core-collapse supernova with multi-messenger signals
• Towards an Understanding of the Resolution Dependence of Core-Collapse Supernova Simulations
• Developing the MeV potential of DUNE: Detailed considerations of muon-induced spallation and other backgrounds
• Supernova neutrino signals based on long-term axisymmetric simulations
• Neutrino Signals of Core-Collapse Supernovae in Underground Detectors
• Astrophysical constraints on non-standard coherent neutrino-nucleus scattering
• Retrieval of energy spectra for all flavor of neutrinos from core-collapse supernova with multiple detectors
• Black hole hyperaccretion in collapsars. I. MeV neutrinos
• Charged-current scattering off ${}^{16}$O nucleus as a detection channel for supernova neutrinos
• Enhanced low-energy supernova burst detection in large liquid argon time projection chambers enabled by Q-Pix
• Non-thermal neutrinos created by shock acceleration in successful and failed core-collapse supernova
• Anisotropic neutrinos and gravitational waves from black hole neutrino-dominated accretion flows in fallback core-collapse supernovae
• Quantum witness and invasiveness of cosmic neutrino measurements
• Neutrinos and gravitational waves from magnetized neutrino-dominated accretion discs with magnetic coupling
• Quantum Closures for Neutrino Moment Transport
• Theoretical X-ray light curves of young SNe II: the example of SN 2013ej
• Triangulating Black Hole Forming Stellar Collapses through Neutrinos
• Neutrino flavour as a test of the explosion mechanism of core-collapse supernovae
• A Brief History of the Co-evolution of Supernova Theory with Neutrino Physics
• Measuring the Low-Energy Weak Mixing Angle with Supernova Neutrinos
• Supernova $\nu$ flavour conversions in DUNE: the slow, the fast and the standard