Gravitational waves from three-dimensional core-collapse supernova models: The impact of moderate progenitor rotation
arXiv:1810.07638 · doi:10.1093/mnras/stz990
Abstract
We present predictions for the gravitational-wave (GW) emission of three-dimensional supernova (SN) simulations performed for a 15 solar-mass progenitor with the Prometheus-Vertex code using energy-dependent, three-flavor neutrino transport. The progenitor adopted from stellar evolution calculations including magnetic fields had a fairly low specific angular momentum (j_Fe <~ 10^{15} cm^2/s) in the iron core (central angular velocity ~0.2 rad/s), which we compared to simulations without rotation and with artificially enhanced rotation (j_Fe <~ 2*10^{16} cm^2/s; central angular velocity ~0.5 rad/s). Our results confirm that the time-domain GW signals of SNe are stochastic, but possess deterministic components with characteristic patterns at low frequencies (<~200 Hz), caused by mass motions due to the standing accretion shock instability (SASI), and at high frequencies, associated with gravity-mode oscillations in the surface layer of the proto-neutron star (PNS). Non-radial mass motions in the post-shock layer as well as PNS convection are important triggers of GW emission, whose amplitude scales with the power of the hydrodynamic flows. There is no monotonic increase of the GW amplitude with rotation, but a clear correlation with the strength of SASI activity. Our slowly rotating model is a fainter GW emitter than the non-rotating model because of weaker SASI activity and damped convection in the post-shock layer and PNS. In contrast, the faster rotating model exhibits a powerful SASI spiral mode during its transition to explosion, producing the highest GW amplitudes with a distinctive drift of the low-frequency emission peak from ~80-100 Hz to ~40-50 Hz. This migration signifies shock expansion, whereas non-exploding models are discriminated by the opposite trend.
arXiv commentAdded new figure, figure 9. Updated figure 9, now figure 10. Modified the discussion of the proto-neutron star convection. Added a figure showing the average rotation rate as a function of radius. Added a section discussing where the low-frequency gravitational waves are generated, this information is visualized in figure 9. We also made some minor changes to the text and selected plots
References in corpus (71)
- Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
- Presupernova Evolution of Differentially Rotating Massive Stars Including Magnetic Fields
- Measuring gravitational waves from binary black hole coalescences: I. Signal to noise for inspiral, merger, and ringdown
- Fast core rotation in red-giant stars revealed by gravity-dominated mixed modes
- Spin down of the core rotation in red giants
- Two-dimensional hydrodynamic core-collapse supernova simulations with spectral neutrino transport. I. Numerical method and results for a 15 M_sun star
- Delayed neutrino-driven supernova explosions aided by the standing accretion-shock instability
- Radiation hydrodynamics with neutrinos: Variable Eddington factor method for core-collapse supernova simulations
- Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914
- Seismic constraints on the radial dependence of the internal rotation profiles of six Kepler subgiants and young red giants
- Pulsar Recoil and Gravitational Radiation due to Asymmetrical Stellar Collapse and Explosion
- Relativistic simulations of rotational core collapse. II. Collapse dynamics and gravitational radiation
- A New Multi-Dimensional General Relativistic Neutrino Hydrodynamics Code of Core-Collapse Supernovae III. Gravitational Wave Signals from Supernova Explosion Models
- Two-Dimensional Hydrodynamic Core-Collapse Supernova Simulations with Spectral Neutrino Transport II. Models for Different Progenitor Stars
- Angular momentum transport within evolved low-mass stars
- Exploring the relativistic regime with Newtonian hydrodynamics: An improved effective gravitational potential for supernova simulations
- Supernova Simulations from a 3D Progenitor Model -- Impact of Perturbations and Evolution of Explosion Properties
- Instability of a stalled accretion shock: evidence for the advective-acoustic cycle
- The gravitational wave burst signal from core collapse of rotating stars
- Neutrino-driven explosion of a 20 solar-mass star in three dimensions enabled by strange-quark contributions to neutrino-nucleon scattering
- A Model for Gravitational Wave Emission from Neutrino-Driven Core-Collapse Supernovae
- SASI Activity in Three-Dimensional Neutrino-Hydrodynamics Simulations of Supernova Cores
- Non-Radial Instabilities and Progenitor Asphericities in Core-Collapse Supernovae
- Is Strong SASI Activity the Key to Successful Neutrino-Driven Supernova Explosions?
- Towards Realistic Progenitors of Core-Collapse Supernovae
- Revival of The Stalled Core-Collapse Supernova Shock Triggered by Precollapse Asphericity in the Progenitor Star
- Multidimensional supernova simulations with approximative neutrino transport. II. Convection and the advective-acoustic cycle in the supernova core
- Multiple physical elements to determine the gravitational-wave signatures of core-collapse supernovae
- A Xylophone Configuration for a third Generation Gravitational Wave Detector
- The gravitational wave signal from core-collapse supernovae
- Gravitational Wave Signals from 3D Neutrino Hydrodynamics Simulations of Core-Collapse Supernovae
- 3D Collapse of Rotating Stellar Iron Cores in General Relativity including Deleptonization and a Nuclear Equation of State
- Self-sustained asymmetry of lepton-number emission: A new phenomenon during the supernova shock-accretion phase in three dimensions
- Neutrino emission characteristics and detection opportunities based on three-dimensional supernova simulations
- Observing Gravitational Waves from Core-Collapse Supernovae in the Advanced Detector Era
- Three-dimensional simulations of rapidly rotating core-collapse supernovae: finding a neutrino-powered explosion aided by non-axisymmetric flows
- Rotation-supported Neutrino-driven Supernova Explosions in Three Dimensions and the Critical Luminosity Condition
- A New Gravitational-Wave Signature from Standing Accretion Shock Instabilities in Supernovae
- Generic Gravitational Wave Signals from the Collapse of Rotating Stellar Cores
- Dynamics and Gravitational Wave Signature of Collapsar Formation
- Three-dimensional simulations of stellar core collapse in full general relativity: Nonaxisymmetric dynamical instabilities
- One-armed Spiral Instability in a Low T/|W| Postbounce Supernova Core
- Pulsar Spin-Velocity Alignment: Kinematic Ages, Birth Periods and Braking Indices
- The influence of model parameters on the prediction of gravitational wave signals from stellar core collapse
- Neutrino signature of supernova hydrodynamical instabilities in three dimensions
- Gravitational Wave Signatures from Low-mode Spiral Instabilities in Rapidly Rotating Supernova Cores
- Neutrino-driven Explosions
- Correlated Signatures of Gravitational-Wave and Neutrino Emission in Three-Dimensional General-Relativistic Core-Collapse Supernova Simulations
- Gravitational waves from axisymmetric rotating stellar core collapse to a neutron star in full general relativity
- Turbulent convection in stellar interiors. III. Mean-field analysis and stratification effects
- Gravitational wave signatures in black-hole-forming core collapse
- Correlated Gravitational Wave and Neutrino Signals from General-Relativistic Rapidly Rotating Iron Core Collapse
- Anisotropic emission of neutrino and gravitational-wave signals from rapidly rotating core-collapse supernovae
- A First Targeted Search for Gravitational-Wave Bursts from Core-Collapse Supernovae in Data of First-Generation Laser Interferometer Detectors
- Initial spin periods of neutron stars in supernova remnants
- A New Multi-Dimensional General Relativistic Neutrino Hydrodynamics Code for Core-Collapse Supernovae IV. The Neutrino Signal
- Pulsar Birthrate from Parkes Multi-beam Survey
- Gravitational Radiation from Axisymmetric Rotational Core Collapse
- Effect of Rotation on the Stability of a Stalled Cylindrical Shock and its Consequences for Core-Collapse Supernovae
- Neutrino-driven Turbulent Convection and Standing Accretion Shock Instability in Three-Dimensional Core-Collapse Supernovae
- Gravitational Waves from Stellar Collapse: Correlations to Explosion Asymmetries
- Are pulsars spun up or down by SASI spiral modes?
- Pushing towards the ET sensitivity using 'conventional' technology
- Effects of Rotation on Stochasticity of Gravitational Waves in Nonlinear Phase of Core-Collapse Supernovae
- Circular polarizations of gravitational waves from core-collapse supernovae: a clear indication of rapid rotation
- Inferring the core-collapse supernova explosion mechanism with three-dimensional gravitational-wave simulations
- Probing Rotation of Core-collapse Supernova with Concurrent Analysis of Gravitational Waves and Neutrinos
- Gravitational waves from supernova matter
- A simple toy model of the advective-acoustic instability. II. Numerical simulations
- Supernova Explosions and Neutron Star Formation
- Gravitational Waves from Core-Collapse Supernovae
Cited by in corpus (70)
- Properties and astrophysical implications of the 150 Msun binary black hole merger GW190521
- Characterizing the Gravitational Wave Signal from Core-Collapse Supernovae
- Enhancing Gravitational-Wave Science with Machine Learning
- Gravitational Wave Emission from 3D Explosion Models of Core-Collapse Supernovae with Low and Normal Explosion Energies
- Three-dimensional core-collapse supernova simulations of massive and rotating progenitors
- Temporal and Angular Variations of 3D Core-Collapse Supernova Emissions and their Physical Correlations
- Gravitational-wave signal of a core-collapse supernova explosion of a 15 Solar mass star
- The Science of the Einstein Telescope
- Particle-in-cell Simulation of the Neutrino Fast Flavor Instability
- Detection and Classification of Supernova Gravitational Waves Signals: A Deep Learning Approach
- 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
- Equation of State Dependence of Gravitational Waves in Core-Collapse Supernovae
- Core Collapse Supernova Gravitational Wave Emission for Progenitors of 9.6, 15, and 25 Solar Masses
- Gravitational Waves from Neutrino Asymmetries in Core-Collapse Supernovae
- Constraining properties of the next nearby core-collapse supernova with multi-messenger signals
- Stellar Mass Black Hole Formation and Multi-messenger Signals from Three Dimensional Rotating Core-Collapse Supernova Simulations
- Characteristic Time Variability of Gravitational-Wave and Neutrino Signals from Three-dimensional Simulations of Non-Rotating and Rapidly Rotating Stellar Core-Collapse
- Pulsational pair-instability supernovae: gravitational collapse, black-hole formation, and beyond
- The final core collapse of pulsational pair instability supernovae
- Three-dimensional simulation of a core-collapse supernova for a binary star progenitor of SN 1987A
- Three dimensional magnetorotational core-collapse supernova explosions of a 39 solar mass progenitor star
- Features of Accretion-phase Gravitational-wave Emission from Two-dimensional Rotating Core-collapse Supernovae
- The role of jets in exploding supernovae and in shaping their remnants
- Dimension dependence of numerical simulations on gravitational waves from protoneutron stars
- The Lunar Gravitational-wave Antenna: Mission Studies and Science Case
- Inferring Astrophysical Parameters of Core-Collapse Supernovae from their Gravitational-Wave Emission
- Improving the background of gravitational-wave searches for core collapse supernovae: A machine learning approach
- Magnetic support for neutrino-driven explosion of 3D non-rotating core-collapse supernova models
- Determination of properties of protoneutron stars toward black hole formation via gravitational wave observations
- Insights into non-axisymmetric instabilities in three-dimensional rotating supernova models with neutrino and gravitational-wave signatures
- Determining the Structure of Rotating Massive Stellar Cores with Gravitational Waves
- Gravitational-wave Signals From Three-dimensional Supernova Simulations With Different Neutrino-Transport Methods
- Multimessenger Asteroseismology of Core-Collapse Supernovae
- Supplying angular momentum to the jittering jets explosion mechanism using inner convection layers
- Search for gravitational-wave bursts in the third Advanced LIGO-Virgo run with coherent WaveBurst enhanced by Machine Learning
- Gravitational Wave Signals from Two-Dimensional Core-Collapse Supernova Models with Rotation and Magnetic Fields
- Modeling Core-Collapse Supernovae Gravitational-Wave Memory in Laser Interferometric Data
- A semi-supervised Machine Learning search for never-seen Gravitational-Wave sources
- Remnant masses of core collapse supernovae in the jittering jets explosion mechanism
- Classification of the core-collapse supernova explosion mechanism with learned dictionaries
- Characterizing a supernova's Standing Accretion Shock Instability with neutrinos and gravitational waves
- Stability of the protoneutron stars toward black hole formation
- Universality in supernova gravitational waves with proto-neutron star properties
- Effect of stellar rotation on the development of post-shock instabilities during core-collapse supernovae
- Exploring Supernova Gravitational Waves with Machine Learning
- Search for gravitational waves emitted from SN 2023ixf
- Gray Two-moment Neutrino Transport: Comprehensive Tests and Improvements for Supernova Simulations
- Non-thermal neutrinos created by shock acceleration in successful and failed core-collapse supernova
- The jittering jets explosion mechanism (JJEM) in electron capture supernovae
- Standing Accretion Shock Instability in the Collapse of a Rotating Stellar Core
- Accretion-Induced Collapse of Dark Matter Admixed White Dwarfs -- II: Rotation and Gravitational-wave Signals
- Modifications to the signal from a gravitational wave event due to a surrounding shell of matter
- Detecting and reconstructing gravitational waves from the next Galactic core-collapse supernova in the Advanced Detector Era
- Implications of post-kick jets in core collapse supernovae
- Gravitational Waves from Supernova Mass Loss and Natal Kicks in Close Binaries
- Effects of multidimensional treatment of gravity in simulations on supernova gravitational waves
- Estimate of the Detectability of the Circular Polarisation Signature of Supernova Gravitational Waves Using the Stokes Parameters
- Evolving massive stars to core collapse with GENEC: Extension of equation of state, opacities and effective nuclear network
- Waveform Reconstruction of Core-Collapse Supernova Gravitational Waves with Improved Multisynchrosqueezing Transform
- Gravitational Lensing of Core Collapse Supernova Gravitational Wave Signals
- Digital Discovery of interferometric Gravitational Wave Detectors
- A Parametric Study of the SASI Comparing General Relativistic and Nonrelativistic Treatments
- Unveiling gravitational waves from core-collapse supernovae with MUSE
- Constraining the Time of Gravitational Wave Emission from Core-Collapse Supernovae
- Residual neural networks to classify the high frequency emission in core-collapse supernova gravitational waves
- Constraining the gravitational-wave emission of core-collapse supernovae with ground-based detectors
- Gravitational wave interactions with a viscous fluid: Core collapse supernova, binary neutron star merger, and accretion around a black hole merger
- Trends in gravitational wave emission in axisymmetric simulations of rotating core-collapse supernovae
- Stochastic Gravitational-Wave Background from Stellar Core-Collapse Events