Citation
Patel, Pinkesh Kiritbhai (2011) Search for Gravitational Waves from a Nearby Neutron Star Using Barycentric Resampling. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/00AG-ZF69. https://resolver.caltech.edu/CaltechTHESIS:09142010-170958877
Abstract
Rapidly spinning neutron stars in our Galactic neighborhood are promising sources of quasi-monochromatic continuous gravitational waves observable by the current LIGO detectors. I describe a search done on the LIGO S5 data, looking for an isolated neutron star hypothesized to be at a distance of about 100 parsecs. This kind of search is computationally bound and is made possible by the implementation of barycentric resampling, which is described here as well. I also describe the work done at the Hanford LIGO site, while taking data for the Astrowatch program.
Item Type: | Thesis (Dissertation (Ph.D.)) | ||||
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Subject Keywords: | Gravitaional Waves, Resampling, Continuous Waves, Neutron Stars | ||||
Degree Grantor: | California Institute of Technology | ||||
Division: | Physics, Mathematics and Astronomy | ||||
Major Option: | Physics | ||||
Thesis Availability: | Public (worldwide access) | ||||
Research Advisor(s): |
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Group: | LIGO | ||||
Thesis Committee: |
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Defense Date: | 26 August 2010 | ||||
Non-Caltech Author Email: | ppatel23 (AT) gmail.com | ||||
Funders: |
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Record Number: | CaltechTHESIS:09142010-170958877 | ||||
Persistent URL: | https://resolver.caltech.edu/CaltechTHESIS:09142010-170958877 | ||||
DOI: | 10.7907/00AG-ZF69 | ||||
Default Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||
ID Code: | 6030 | ||||
Collection: | CaltechTHESIS | ||||
Deposited By: | Pinkesh Patel | ||||
Deposited On: | 01 Oct 2010 22:09 | ||||
Last Modified: | 26 Oct 2021 17:44 |
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