Imagen de Portada

Gravitational-Wave and Gravitational-Wave Memory Signatures of Core-Collapse Supernovae

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Choi, Lyla, Burrows, Adam, Vartanyan, David
Formato:	Preprint
Publicado:	2024
Materias:	High Energy Astrophysical Phenomena Solar and Stellar Astrophysics General Relativity and Quantum Cosmology
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Core-Collapse Supernovae and their Gravitational Wave Signals: The Status of Theory and Modeling
por: Müller, Bernhard
Publicado: (2026)

Predicted Neutrino Signal Features of Core-Collapse Supernovae
por: Choi, Lyla, et al.
Publicado: (2025)

Topology of the Superconducting Heart of Neutron Stars: Effects of Microphysics and Gravitational-Wave Signatures
por: Das, Mayusree, et al.
Publicado: (2025)

Gravitational Waves from Magnetars
por: Kouvaris, Chris
Publicado: (2024)

Population Synthesis of Gravitational Wave Sources
por: Breivik, Katelyn
Publicado: (2025)

Lightcurve Features of Magnetar-Powered Superluminous Supernovae with Gravitational-Wave Emission and High-Energy Leakage
por: Zhang, Jinghao, et al.
Publicado: (2025)

Exploring Temperature Influences on Gravitational Wave Production in Binary White Dwarfs
por: Nunes, Sílvia P., et al.
Publicado: (2025)

An Exploration of the Equation of State Dependence of Core-Collapse Supernova Explosion Outcomes and Signatures
por: Rusakov, Aleksandr, et al.
Publicado: (2026)

Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties
por: Li, Zhenwei, et al.
Publicado: (2024)

Deciphering Accretion-Driven Starquakes in Recycled Millisecond Pulsars using Gravitational Waves
por: Chatterjee, Sagnik, et al.
Publicado: (2024)

In LIGO's Sight? Vigorous Coherent Gravitational Waves from Cooled Collapsar Disks
por: Gottlieb, Ore, et al.
Publicado: (2024)

Astrophysical Parameter Inference on Accreting White Dwarf Binaries using Gravitational Waves
por: Yi, Sophia, et al.
Publicado: (2023)

Prospects for the Observation of Continuous Gravitational Waves from Deformed Fast-spinning White Dwarfs
por: Sousa, M. F., et al.
Publicado: (2024)

Gravitational Wave Emission by Accretion of Matter and Magnetic Deformation in Fast Rotating White Dwarfs
por: Sousa, Manoel F., et al.
Publicado: (2021)

Luminous Fast Blue Optical Transients as "Failed" Gravitational Wave Sources: Helium Core$-$Black Hole Mergers Following Delayed Dynamical Instability
por: Klencki, Jakub, et al.
Publicado: (2025)

Physical Correlations and Predictions Emerging from Modern Core-Collapse Supernova Theory
por: Burrows, Adam, et al.
Publicado: (2024)

The Nature of Gravitational Wave Events with Host Environment Escape Velocities
por: Li, Guo-Peng, et al.
Publicado: (2025)

Gravitational Wave emission in Binary Neutron Star early post-merger within a dark environment
por: Suárez-Fontanella, D., et al.
Publicado: (2024)

A Black-Hole Excision Scheme for General Relativistic Core-Collapse Supernova Simulations
por: Sykes, B., et al.
Publicado: (2022)

Detecting Gravitational Wave Memory in the Next Galactic Core-Collapse Supernova
por: Richardson, Colter J., et al.
Publicado: (2024)

Unraveling the Origin of Unequal Mass Gravitational Wave Events: Insights from a Galactic High Mass X-ray Binary
por: Shah, Neev, et al.
Publicado: (2026)

Collapsar Disk Outflows III: Detectable Neutrino and Gravitational Wave Signatures
por: Fernández, Rodrigo, et al.
Publicado: (2025)

Gravitational waves from neutron-star mountains
por: Gittins, Fabian
Publicado: (2024)

Resolving Black Hole Family Issues Among the Massive Ancestors of Very High-Spin Gravitational-Wave Events Like GW231123
por: Stegmann, Jakob, et al.
Publicado: (2025)

Fast Radio Bursts and Electromagnetic Transition Radiation on Gravitational Shockwaves
por: Fursaev, D. V., et al.
Publicado: (2025)

Distinguishing the Origin of Eccentric Black Hole Mergers with Gravitational-wave Spin Measurements
por: Stegmann, Jakob, et al.
Publicado: (2025)

Gravitational waves from r-mode oscillations of stochastically accreting neutron stars
por: Dong, Wenhao, et al.
Publicado: (2025)

Low-Frequency Gravitational Waves in Three-Dimensional Core-Collapse Supernova Models
por: Richardson, Colter J., et al.
Publicado: (2025)

Gravitational wave seismology of charged strange stars in the Cowling approximation: the fluid pulsation modes
por: Arbañil, José D. V., et al.
Publicado: (2024)

Slowly Rotating Relativistic Stars: VII. Gravitational Radiation from the Quasi-Radial Modes
por: Hartle, James B., et al.
Publicado: (2025)

Supernova Simulations
por: Müller, Bernhard
Publicado: (2024)

Model-Independent Determination of the Tidal Deformability of a 1.4 $M_{\odot}$ Neutron Star from Gravitational-Wave Measurements
por: Huang, Chun
Publicado: (2025)

Core Collapse Supernova Gravitational Wave Sourcing and Characterization based on Three-Dimensional Models
por: Murphy, R. Daniel, et al.
Publicado: (2025)

Waveform Reconstruction of Core-Collapse Supernovae Gravitational-Waves with Ensemble Empirical Mode Decomposition
por: Yuan, Yong, et al.
Publicado: (2023)

Assessing Matched Filtering for Core-Collapse Supernova Gravitational-Wave Detection
por: Andresen, Haakon, et al.
Publicado: (2024)

From Jets to Failed Supernovae: Morphologies and Gravitational-Wave Signatures in Two-Dimensional Magnetorotational Core-Collapse Supernovae
por: Pan, Kuo-Chuan, et al.
Publicado: (2026)

Gravitational wave signals from primordial black holes orbiting solar-type stars
por: De Lorenci, Vitorio A., et al.
Publicado: (2025)

Gravitational Waves from Neutrino-Driven Core Collapse Supernovae: Predictions, Detection, and Parameter Estimation
por: Mezzacappa, Anthony, et al.
Publicado: (2024)

The Impact of Solar-Terrestrial Plasma and Magnetic Field on the Detection of Space-borne Gravitational Wave Detections
por: Su, Wei
Publicado: (2025)

Long-Time 2D Simulations of Fallback Supernovae: A Systematic Investigation of Explosions Dynamics and Mass Ejections
por: Sykes, Bailey, et al.
Publicado: (2024)