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Gravitational Waves from Neutrino-Driven Core Collapse Supernovae: Predictions, Detection, and Parameter Estimation

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arxiv 2401.11635 v1 pith:BPYP3NZP submitted 2024-01-22 astro-ph.HE gr-qc

Anthony Mezzacappa , Michele Zanolin This is my paper · ORCID
classification astro-ph.HEgr-qc
keywords collapsecoregravitationalpredictionsdetectionemissionestimationmodeling
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Three-dimensional modeling has reached a level of maturity to provide detailed predictions of the gravitational wave emission in neutrino-driven core collapse supernovae. We review the status of these modeling efforts, current predictions for core collapse supernova gravitational wave emission, and the status of algorithms for the detection of core collapse supernova gravitational waves and the estimation of physical parameters associated with these events, which we hope to use to cull information about the central engine.

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Cited by 14 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. On the nature of oscillating modes of proto-neutron stars

    gr-qc 2026-08 conditional novelty 7.0 of 10

    A new energy-based classifier separates proto-neutron star oscillation modes into four families and identifies the dominant high-frequency gravitational-wave feature as the PNS fundamental mode.

  2. Parameter estimation of protoneutron stars from gravitational wave signals using the Hilbert-Huang transform

    gr-qc 2024-11 conditional novelty 6.0 of 10

    An HHT-based pipeline estimates protoneutron star mass/radius-squared from simulated core-collapse supernova gravitational waves with accuracy comparable to STFT-based methods.

  3. Reconstructing Core-Collapse Supernova Gravitational-Wave Signals with Transdimensional Bayesian Inference

    astro-ph.HE 2026-08 conditional novelty 5.0 of 10

    Transdimensional Bayesian inference with tBilby reconstructs core-collapse supernova gravitational-wave signals in simulated LIGO noise with overlaps up to 85%, and captures the dominant proto-neutron-star mode even a...

  4. Trends in gravitational wave emission in axisymmetric simulations of rotating core-collapse supernovae

    astro-ph.HE 2025-12 conditional novelty 5.0 of 10

    Rotating core-collapse supernova simulations produce gravitational waves up to ~3 kHz, whose frequency and amplitude fall with faster rotation, and no resonant amplification is found.

  5. Impact of rotation on the accretion of entropy perturbations in collapsing massive stars

    astro-ph.SR 2025-09 conditional novelty 5.0 of 10

    Rotation has little effect on entropy perturbations falling onto a supernova shock: the sound and vortex waves they create stay below about 1% of the local sound speed, and convective eddies dominate for the modes tha...

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    astro-ph.HE 2026-03 conditional novelty 4.5 of 10

    Using a linear SVM, EOS classification from bounce gravitational waves remains robust to real noise, progenitor diversity, and bounce-time uncertainty in the frequency domain, but collapses in the time domain under ti...

  7. Classifying the nuclear equation of state in LVK interferometric noise through core-collapse supernova gravitational-wave signatures using convolutional neural networks

    gr-qc 2026-07 conditional novelty 4.0 of 10

    A CNN can distinguish five supernova equations of state from reconstructed time-frequency images at 1 kpc in LVK O3b noise, but accuracy drops sharply by 5-10 kpc and the reported numbers are internally inconsistent.

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    astro-ph.HE 2025-07 conditional novelty 4.0 of 10

    An all-sky search of O4a LIGO data finds no new gravitational-wave bursts and improves burst sensitivity and rate limits by factors of 2 to 10 over the previous run.

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    A systematic set of equations of state and pasta-phase structures for cold dense stellar matter, tabulated for 13 relativistic mean-field models over a wide range of densities and proton fractions.

  10. Waveform Reconstruction of Core-Collapse Supernova Gravitational Waves with Improved Multisynchrosqueezing Transform

    astro-ph.HE 2024-12 reject novelty 4.0 of 10

    An improved multisynchrosqueezing transform is reported to reconstruct simulated supernova gravitational waves out to 317 kpc with the Einstein Telescope, versus 186 kpc for the short-time Fourier transform.

  11. Exploring Physics beyond the Standard Model from kHz-Gravitational-Wave Signals of Core-Collapse Supernovae

    astro-ph.HE 2026-07 unverdicted novelty 2.0 of 10

    A topical review arguing that kHz gravitational-wave signals from supernova collapse can probe dense matter and gravity beyond the standard model.

  12. Targeted searches for gravitational waves from SN 2023ixf and SGR 1935+2154

    gr-qc 2025-06 unverdicted novelty 1.0 of 10

    A proceedings summary reporting that targeted searches found no gravitational waves from SN 2023ixf or SGR 1935+2154 and produced improved energy upper limits.

  13. What shall we learn from a future supernova?

    astro-ph.SR 2024-12 unverdicted novelty 1.0 of 10

    A review of supernova neutrino and DSNB physics, with a reproduced Bayesian figure from the author's prior work, but no new analysis.

  14. Applications of machine learning in gravitational wave research with current interferometric detectors

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    A community review of machine learning in current gravitational-wave detectors, mapping where ML already works in production (noise subtraction, glitch classification, low-latency classification) and where traditional...

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