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Insights into binary black hole formation from gravtitational waves

Stevenson, Simon Paul (2017)
Ph.D. thesis, University of Birmingham.

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Gravitational-waves provide a unique probe of the stellar remnants---black holes and neutron stars---left behind at the end of massive stars lives. On the 14th September 2015 the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) made the first direct detection of gravitational waves from a merging stellar mass binary black hole, GW150914, during its first observation run (O1). In this thesis we present Compact Object Mergers: Population Astrophysics and Statistics (COMPAS). COMPAS is a platform incorporating astrophysical modelling tools and statistical analysis tools to extract information from the population of merging binary black holes we observe. We demonstrate that the masses, spins and observed rate of binary black holes can offer new insights into their formation.

Type of Work:Ph.D. thesis.
Supervisor(s):Mandel, Ilya and Farr, Will
School/Faculty:Colleges (2008 onwards) > College of Engineering & Physical Sciences
Department:School of Physics & Astronomy
Subjects:QB Astronomy
Institution:University of Birmingham
ID Code:7667
This unpublished thesis/dissertation is copyright of the author and/or third parties. The intellectual property rights of the author or third parties in respect of this work are as defined by The Copyright Designs and Patents Act 1988 or as modified by any successor legislation. Any use made of information contained in this thesis/dissertation must be in accordance with that legislation and must be properly acknowledged. Further distribution or reproduction in any format is prohibited without the permission of the copyright holder.
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