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On the distribution of stellar-sized black hole spins
- Source :
- Journal of Physics: Conference Series, Journal of Physics: Conference Series 716 (2016), Nr. 1
- Publication Year :
- 2016
- Publisher :
- arXiv, 2016.
-
Abstract
- Black hole spin will have a large impact on searches for gravitational waves with advanced detectors. While only a few stellar mass black hole spins have been measured using X-ray techniques, gravitational wave detectors have the capacity to greatly increase the statistics of black hole spin measurements. We show what we might learn from these measurements and how the black hole spin values are influenced by their formation channels.<br />Comment: 4 pages, 2 figures, pre-GW150914 detection, refereed and accepted contribution to proceedings of 11th Edoardo Amaldi Conference on Gravitational Waves, June 2015, Gwangju, Korea
- Subjects :
- History
Stellar mass
Astrophysics::High Energy Astrophysical Phenomena
FOS: Physical sciences
Astrophysics
General Relativity and Quantum Cosmology (gr-qc)
Gravity waves
01 natural sciences
General Relativity and Quantum Cosmology
Education
Advanced detector
Gravitational wave detectors
Gravitation
0103 physical sciences
ddc:530
010303 astronomy & astrophysics
Konferenzschrift
Dewey Decimal Classification::500 | Naturwissenschaften
Spin-½
Gravitationswelle
Physics
High Energy Astrophysical Phenomena (astro-ph.HE)
Spins
Black holes
010308 nuclear & particles physics
Gravitational wave
Gravitational effects
Stars
X-ray techniques
Computer Science Applications
Black hole
Distribution (mathematics)
Stellar-mass black holes
Condensed Matter::Strongly Correlated Electrons
ddc:500
Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik
Astrophysics - High Energy Astrophysical Phenomena
Subjects
Details
- Database :
- OpenAIRE
- Journal :
- Journal of Physics: Conference Series, Journal of Physics: Conference Series 716 (2016), Nr. 1
- Accession number :
- edsair.doi.dedup.....d47c2798b1c462e83dd9a57ef18731f2
- Full Text :
- https://doi.org/10.48550/arxiv.1604.00778