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ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes

Fuente: arXiv

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Detalles Bibliográficos
Autores principales:	Paul, Kaushik, Maurya, Akash, Henry, Quentin, Sharma, Kartikey, Satheesh, Pranav, Divyajyoti, Kumar, Prayush, Mishra, Chandra Kant
Formato:	Preprint
Publicado:	2024
Materias:	General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

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