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dc.contributor.advisorChairperson, Graduate Committee: Ronald W. Hellings.en
dc.contributor.authorPlowman, Joseph Eugene.en
dc.date.accessioned2013-06-25T18:39:45Z
dc.date.available2013-06-25T18:39:45Z
dc.date.issued2010en
dc.identifier.urihttps://scholarworks.montana.edu/xmlui/handle/1/2063
dc.description.abstractA number of scenarios have been proposed for the origin of the supermassive black holes (SMBHs) that are found in the centres of most galaxies. Many such scenarios predict a high-redshift population of massive black holes (MBHs), with masses in the range 10 ² to 10 5 times that of the Sun. When the Laser Interferometer Space Antenna (LISA) is finally operational, it is likely that it will detect on the order of 100 of these MBH binaries as they merge. The differences between proposed population models produce appreciable effects in the portion of the population which is detectable by LISA, so it is likely that the LISA observations will allow us to place constraints on them. However, gravitational wave detectors such as LISA will not be able to detect all such mergers nor assign precise black hole parameters to the merger, due to weak gravitational wave signal strengths. This dissertation explores LISA's ability to distinguish between several MBH population models. In this way, we go beyond predicting a LISA observed population and consider the extent to which LISA observations could inform astrophysical modelers. The errors in LISA parameter estimation are applied in two ways, with an 'Error Kernel' that is marginalized over astrophysically uninteresting 'sample' parameters, and with a more direct method which generates random sample parameters for each source in a population realization. We consider how the distinguishability varies depending on the choice of source parameters (1 or 2 parameters chosen from masses, redshift or spins) used to characterize the model distributions, with confidence levels determined by 1 or 2-dimensional tests based on the Kolmogorov-Smirnov test.en
dc.language.isoengen
dc.publisherMontana State University - Bozeman, College of Letters & Scienceen
dc.subject.lcshBlack holes (Astronomy).en
dc.subject.lcshGravitational waves.en
dc.titleConstraining massive black hole population models with gravitational wave observations
dc.typeDissertation
dc.rights.holderCopyright Joseph Eugene Plowman 2010en
thesis.catalog.ckey1522507en
thesis.degree.committeemembersMembers, Graduate Committee: Sachiko Tsuruta; Neil J. Cornish; Dana W. Loncope; Charles Kankelborgen
thesis.degree.departmentPhysics.en
thesis.degree.genreDissertationen
thesis.degree.namePhDen
thesis.format.extentfirstpage1en
thesis.format.extentlastpage113en
mus.identifier.categoryPhysics & Mathematics
mus.relation.departmentPhysics.en_US
mus.relation.universityMontana State University - Bozemanen_US


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