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dc.contributor.advisorScott A. Hughes.en_US
dc.contributor.authorSen, Bidisha.en_US
dc.contributor.otherMassachusetts Institute of Technology. Department of Physics.en_US
dc.date.accessioned2020-01-08T19:40:51Z
dc.date.available2020-01-08T19:40:51Z
dc.date.copyright2019en_US
dc.date.issued2019en_US
dc.identifier.urihttps://hdl.handle.net/1721.1/123388
dc.descriptionThesis: S.B., Massachusetts Institute of Technology, Department of Physics, 2019en_US
dc.descriptionCataloged from PDF version of thesis.en_US
dc.descriptionIncludes bibliographical references (page 39).en_US
dc.description.abstractGravitational waves emitted from binary black hole systems carry energy away from the orbit, and cause the black holes to spiral towards one another and eventually merge. While all such detected systems are effectively circular at coalescence, these binaries may start out with non-negligible eccentricity. Due to certain astrophysical phenomena, it is expected that some binary systems may merge with some residual eccentricity, and so understanding how to measure the waveforms from these systems are of particular interest for future third generation detectors, such as LISA.en_US
dc.description.statementofresponsibilityby Bidisha Sen.en_US
dc.format.extent39 pagesen_US
dc.language.isoengen_US
dc.publisherMassachusetts Institute of Technologyen_US
dc.rightsMIT theses are protected by copyright. They may be viewed, downloaded, or printed from this source but further reproduction or distribution in any format is prohibited without written permission.en_US
dc.rights.urihttp://dspace.mit.edu/handle/1721.1/7582en_US
dc.subjectPhysics.en_US
dc.titleThe frequency spectrum of gravitational waves from eccentric orbitsen_US
dc.typeThesisen_US
dc.description.degreeS.B.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.identifier.oclc1132272772en_US
dc.description.collectionS.B. Massachusetts Institute of Technology, Department of Physicsen_US
dspace.imported2020-01-08T19:40:50Zen_US
mit.thesis.degreeBacheloren_US
mit.thesis.departmentPhysen_US


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