:: Library Catalog

Imagen de Portada

Guardado en:

Detalles Bibliográficos
Autores principales:	Liu, Tonghua, Shao, Chenggang, Liao, Kai
Formato:	Preprint
Publicado:	2026
Materias:	High Energy Astrophysical Phenomena
Acceso en línea:	https://arxiv.org/abs/2605.16425
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Is GW231123 a hierarchical merger?
por: Passenger, Lachlan, et al.
Publicado: (2025)

Searching for Electromagnetic Counterpart Candidates to GW231123
por: He, Lei, et al.
Publicado: (2025)

Superradiance Constraints from GW231123
por: Caputo, Andrea, et al.
Publicado: (2025)

On the Formation of GW231123 in Population III Star Clusters
por: Liu, Shuai, et al.
Publicado: (2025)

GW231123: extreme spins or microglitches?
por: Ray, Anarya, et al.
Publicado: (2025)

GW231123 Formation from Population III Stars: Isolated Binary Evolution
por: Tanikawa, Ataru, et al.
Publicado: (2025)

Testing the wormhole echo hypothesis for GW231123
por: Lai, Qi, et al.
Publicado: (2026)

The Hierarchical Merger Scenario for GW231123
por: Li, Guo-Peng, et al.
Publicado: (2025)

GW231123: Overlapping Gravitational Wave Signals?
por: Hu, Qian, et al.
Publicado: (2025)

Assembling GW231123 in star clusters through the combination of stellar binary evolution and hierarchical mergers
por: Paiella, Lavinia, et al.
Publicado: (2025)

Prospects for the formation of GW231123 from the AGN channel
por: Delfavero, V., et al.
Publicado: (2025)

GW231123 ringdown: interpretation as multimodal Kerr signal
por: Siegel, Harrison, et al.
Publicado: (2025)

Spinning into the Gap: Direct-Horizon Collapse as the Origin of GW231123 from End-to-End GRMHD Simulations
por: Gottlieb, Ore, et al.
Publicado: (2025)

Detection of a Higher Harmonic Quasi-normal Mode in the Ringdown Signal of GW231123
por: Wang, Hai-Tian, et al.
Publicado: (2025)

Accretion is All You Need: Black Hole Spin Alignment in Merger GW231123 Indicates Accretion Pathway
por: Bartos, Imre, et al.
Publicado: (2025)

Can GW231123 have a stellar origin?
por: Croon, Djuna, et al.
Publicado: (2025)

GW231123 Mass Gap Event and the Primordial Black Hole Scenario
por: Yuan, Chen, et al.
Publicado: (2025)

GW231123: A Possible Primordial Black Hole Origin
por: De Luca, Valerio, et al.
Publicado: (2025)

Gravitational-wave parameter estimation to the Moon and back: massive binaries and the case of GW231123
por: Iacovelli, Francesco, et al.
Publicado: (2025)

Machine Learning Confirms GW231123 is a "Lite" Intermediate Mass Black Hole Merger
por: Chatterjee, Chayan, et al.
Publicado: (2025)

GW231123: a Binary Black Hole Merger with Total Mass 190-265 $M_{\odot}$
por: The LIGO Scientific Collaboration, et al.
Publicado: (2025)

GW231123: Likely a product of successive mergers from $\sim 10 $ stellar-mass black holes
por: Li, Yin-Jie, et al.
Publicado: (2025)

Hierarchical Black Hole Mergers in Nuclear Star Clusters: A Combined Dynamical-Secular Channel for GW231123-like Events
por: Liu, Bin, et al.
Publicado: (2025)

Pulsed, Polarized X-ray Emission from Neutron Star Surfaces: the Effects of Vacuum Birefringence in the Magnetosphere
por: Thi, Hoa Dinh, et al.
Publicado: (2025)

Systematic Search for Electromagnetic Counterparts to the Binary Neutron Star Merger Candidate GW231109_235456
por: Li, Zhirui, et al.
Publicado: (2025)

Very Massive, Rapidly Spinning Binary Black Hole Progenitors through Chemically Homogeneous Evolution -- The Case of GW231123
por: Popa, Silvia A., et al.
Publicado: (2025)

The First Model-Independent Upper Bound on Micro-lensing Signature of the Highest Mass Binary Black Hole Event GW231123
por: Chakraborty, Aniruddha, et al.
Publicado: (2025)

The long-term evolution of the GW170817 remnant
por: Liu, Menquan, et al.
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)

Formation of GW230529 from Isolated Binary Evolution
por: Zhu, Jin-Ping, et al.
Publicado: (2024)

Simulation Study on Constraining GW Propagation Speed by GW and GRB Joint Observation on Binary Neutron Star Mergers
por: Rao, Jin-Hui, et al.
Publicado: (2024)

The Late-time Afterglow of GW170817 and Implications for Jet Dynamics
por: Katira, Aman, et al.
Publicado: (2025)

Quarkyonic Neutron Stars as Candidates for the GW230529 Mass-Gap Object
por: Pattnaik, Jeet Amrit, et al.
Publicado: (2025)

Multi-Energy and Multi-Sample Searches for Neutrinos from GW Events
por: V., Aswathi Balagopal, et al.
Publicado: (2025)

Lucky Strikes: On the Origins of GW190814 Through Isolated Binary Evolution
por: Hernandez, Ignacio Magaña, et al.
Publicado: (2025)

Assessing the imprint of eccentricity in GW signatures using two independent waveform models
por: Malagon, Natalie, et al.
Publicado: (2026)

The Very Late Time Afterglow of GW170817 Favors a Wobbling Jet
por: Wang, Hao, et al.
Publicado: (2026)

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars?
por: Saha, Asim Kumar, et al.
Publicado: (2025)

A model for the emission of SGRBs-GW from binary mergers
por: Ali, Shad
Publicado: (2026)

Multimessenger Constraints on Radiatively Decaying Axions from GW170817
por: Diamond, Melissa, et al.
Publicado: (2023)