Final spin and radiated energy in numerical simulations of binary black holes with equal masses and equal, aligned or antialigned spins

Final spin and radiated energy in numerical simulations of binary black holes with equal masses and equal, aligned or antialigned spins

The behavior of merging black holes (including the emitted gravitational waves and the properties of the remnant) can currently be computed only by numerical simulations. This paper introduces ten numerical relativity simulations of binary black holes with equal masses and equal spins aligned or ant...

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Veröffentlicht in:Physical review. D, Particles, fields, gravitation, and cosmology Particles, fields, gravitation, and cosmology, 2013-09, Vol.88 (6), Article 064014
Hauptverfasser: Hemberger, Daniel A., Lovelace, Geoffrey, Loredo, Thomas J., Kidder, Lawrence E., Scheel, Mark A., Szilágyi, Béla, Taylor, Nicholas W., Teukolsky, Saul A.
Format: Artikel
Sprache:eng
Schlagworte:
Alignment
Asymptotic properties
Black holes (astronomy)
Computer simulation
Fittings
Gravitational waves
Mathematical analysis
Mathematical models
Searching
Waveforms
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Zusammenfassung:The behavior of merging black holes (including the emitted gravitational waves and the properties of the remnant) can currently be computed only by numerical simulations. This paper introduces ten numerical relativity simulations of binary black holes with equal masses and equal spins aligned or antialigned with the orbital angular momentum. The initial spin magnitudes have chi sub(i) [
ISSN:1550-7998
1550-2368
DOI:10.1103/PhysRevD.88.064014