Probing Rotation of Core-collapse Supernova with Concurrent Analysis of Gravitational Waves and Neutrinos

Abstract

The next time a core-collapse supernova (SN) explodes in our galaxy, vari- ous detectors will be ready and waiting to detect its emissions of gravitational waves (GWs) and neutrinos. Current numerical simulations have successfully introduced multi-dimensional effects to produce exploding SN models, but thus far the explosion mechanism is not well understood. In this paper, we focus on an investigation of progenitor core rotation via comparison of the start time of GW emission and that of the neutronization burst. The GW and neutrino de- tectors are assumed to be, respectively, the KAGRA detector and a co-located gadolinium-loaded water Cherenkov detector, either EGADS or GADZOOKS!. Our detection simulation studies show that for a nearby supernova (0.2 kpc) we can confirm the lack of core rotation close to 100% of the time, and the presence of core rotation about 90% of the time. Using this approach there is also po- tential to confirm rotation for considerably more distant Milky Way supernova explosions.

31pages, 15figures, submit to ApJ

References in corpus (20)

• LIGO: The Laser Interferometer Gravitational-Wave Observatory
• Delayed neutrino-driven supernova explosions aided by the standing accretion-shock instability
• The gravitational wave burst signal from core collapse of rotating stars
• Neutrino-driven supernova of a low-mass iron-core progenitor boosted by three-dimensional turbulent convection
• The isotropic diffusion source approximation for supernova neutrino transport
• The Dynamics of Neutrino-Driven Supernova Explosions after Shock Revival in 2D and 3D
• Generic Gravitational Wave Signals from the Collapse of Rotating Stellar Cores
• High-Resolution Three-Dimensional Simulations of Core-Collapse Supernovae in Multiple Progenitors
• Two-Dimensional Core-Collapse Supernova Models with Multi-Dimensional Transport
• Limits on Majoron-emitting double-beta decays of Xe-136 in the KamLAND-Zen experiment
• Calibration and sensitivity of the Virgo detector during its second science run
• Measuring the Angular Momentum Distribution in Core-Collapse Supernova Progenitors with Gravitational Waves
• Neutrinos from Supernovae as a Trigger for Gravitational Wave Search
• Comparison of Gravitational Wave Detector Network Sky Localization Approximations
• Reconstructing the supernova bounce time with neutrinos in IceCube
• Two-Dimensional Core-Collapse Supernova Simulations with the Isotropic Diffusion Source Approximation for Neutrino Transport
• Toward connecting core-collapse supernova theory with observations: I. Shock revival in a 15 Msun blue supergiant progenitor with SN 1987A energetics
• From supernovae to neutron stars
• Bayesian parameter estimation of core collapse supernovae using gravitational wave simulations
• Multivariate Regression Analysis of Gravitational Waves from Rotating Core Collapse

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• What can be learned from a future supernova neutrino detection?
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• Correlated Signatures of Gravitational-Wave and Neutrino Emission in Three-Dimensional General-Relativistic Core-Collapse Supernova Simulations
• The Science of the Einstein Telescope
• Anisotropic emission of neutrino and gravitational-wave signals from rapidly rotating core-collapse supernovae
• Gravitational wave asteroseismology with protoneutron stars
• Neutrino Emission as Diagnostics of Core-Collapse Supernovae
• Parameter Estimation and Model Selection of Gravitational Wave Signals Contaminated by Transient Detector Noise Glitches
• Observing Supernova Neutrino Light Curves with Super-Kamiokande: Expected Event Number over 10 s
• Coherent Network Analysis of Gravitational Waves from Three-Dimensional Core-Collapse Supernova Models
• Core-collapse supernovae in the hall of mirrors. A three-dimensional code-comparison project
• On the Neutrino Distributions in Phase Space for the Rotating Core-collapse Supernova Simulated with a Boltzmann-neutrino-radiation-hydrodynamics Code
• Dimension dependence of numerical simulations on gravitational waves from protoneutron stars
• Astrophysical science metrics for next-generation gravitational-wave detectors
• Determination of properties of protoneutron stars toward black hole formation via gravitational wave observations
• Improved Detection of Supernovae with the IceCube Observatory
• Stability of the protoneutron stars toward black hole formation
• Measuring the properties of $f-$mode oscillations of a protoneutron star by third generation gravitational-wave detectors
• Long-term gravitational wave asteroseismology of supernova: from core collapse to 20 seconds postbounce
• Exploring Supernova Gravitational Waves with Machine Learning
• Inferring physical properties of stellar collapse by third-generation gravitational-wave detectors
• The Yet-Unobserved Multi-Messenger Gravitational-Wave Universe
• Equation of state in neutron stars and supernovae
• Timing coincidence search for supernova neutrinos with optical transient surveys
• Prospects for detecting proto-neutron star rotation and spindown using supernova neutrinos