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020 ▼a 9780438169531
035 ▼a (MiAaPQ)AAI10826761
035 ▼a (MiAaPQ)umn:19307
040 ▼a MiAaPQ ▼c MiAaPQ ▼d 247004
0820 ▼a 530
1001 ▼a Meyers, Patrick Michael.
24510 ▼a Cross-correlation Searches for Persistent Gravitational Waves with Advanced LIGO and Noise Studies for Current and Future Ground-based Gravitational-wave Detectors.
260 ▼a [S.l.]: ▼b University of Minnesota., ▼c 2018.
260 1 ▼a Ann Arbor: ▼b ProQuest Dissertations & Theses, ▼c 2018.
300 ▼a 242 p.
500 ▼a Source: Dissertation Abstracts International, Volume: 79-12(E), Section: B.
500 ▼a Adviser: Vuk Mandic.
5021 ▼a Thesis (Ph.D.)--University of Minnesota, 2018.
520 ▼a Over the last three years, the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) has detected signals from colliding black holes and a signal from colliding neutron stars. These detections ushered in a new era of gravitational-
520 ▼a In this dissertation, I present cross-correlation-based searches for a SGWB and other persistent sources of GWs. I introduce and use a new method for setting limits on the strain amplitude of a potential source of GWs in the directions of Scorpi
520 ▼a Improving sensitivity of current detectors and planning for future detectors is vital to the effort to measure and understand the SGWB. This will requires a better understanding of the noise sources that limit sensitivity, especially at lower fr
590 ▼a School code: 0130.
650 4 ▼a Physics.
690 ▼a 0605
71020 ▼a University of Minnesota. ▼b Physics.
7730 ▼t Dissertation Abstracts International ▼g 79-12B(E).
773 ▼t Dissertation Abstract International
790 ▼a 0130
791 ▼a Ph.D.
792 ▼a 2018
793 ▼a English
85640 ▼u http://www.riss.kr/pdu/ddodLink.do?id=T14998934 ▼n KERIS ▼z 이 자료의 원문은 한국교육학술정보원에서 제공합니다.
980 ▼a 201812 ▼f 2019
990 ▼a ***1012033