Gravitational Waves from Core-Collapse Supernovae: Dependence on the Progenitor Star, Rotation Rate and Nuclear Equation of State
astro-ph.HE
Submitted: 2026-09-28
Updated: 2026-09-28
Terminology
Sources
- Gravitational Waves from Core-Collapse Supernovae
- deci-Hz Gravitational Wave Observations on the Moon and Beyond
- 2D and 3D Core-Collapse Supernovae Simulation Results Obtained with the CHIMERA Code
- Convection signatures in early-time gravitational waves from core-collapse supernovae
- Black Hole Supernovae Outcomes Across a Wide Progenitor Range
- Analytic insight into the physics of SASI II. Spiral instability of the prograde mode in a rotating stellar core
- Core-Collapse Supernova detections from Einstein Telescope within the Milky Way
- Gravitational-Wave Lunar Observatory for Cosmology
- All-sky search for short gravitational-wave bursts in the first part of the fourth LIGO-Virgo-KAGRA observing run
- Gravitational Waves from Neutrino-Driven Core Collapse Supernovae: Predictions, Detection, and Parameter Estimation
- Supernova Simulations
- Composable Effects for Flexible and Accelerated Probabilistic Programming in NumPyro
- Impact of the nuclear equation of state on the explodability of massive stars
- Gravitational waves from magnetorotational core-collapse supernovae using 3D GRMHD simulations: effect of rotation and magnetic fields
- Universal relations between the quasinormal modes of neutron star and tidal deformability
- GWTC-5.0: An Introduction to Version 5.0 of the Gravitational-Wave Transient Catalog
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