COALESCENCE RATE OF SUPERMASSIVE BLACK HOLE BINARIES DERIVED FROM COSMOLOGICAL SIMULATIONS: DETECTION RATES FOR LISA AND ET

DOI10.1142/S0218271811020433zbMath1266.83186arXiv1108.2638MaRDI QIDQ4917485

F. Durier, J. A. de Freitas Pacheco, Ch. Filloux, José Carlos N. de Araujo

Publication date: 30 April 2013

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1108.2638

zbMATH Keywords

gravitational wavescosmological simulationssupermassive black holes

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Black holes (83C57) Galactic and stellar structure (85A15) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10) Gravitational waves (83C35) Computational methods for problems pertaining to astronomy and astrophysics (85-08) Astrophysical cosmology (85A40) Experimental work for problems pertaining to relativity and gravitational theory (83-05)

Cites Work

• EVOLUTION OF SUPERMASSIVE BLACK HOLES FROM COSMOLOGICAL SIMULATIONS
• Quasinormal modes of black holes and black branes
• The growth of supermassive black holes fed by accretion disks

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