LDR | | 02070nmm uu200397 4500 |
001 | | 000000332002 |
005 | | 20240805165821 |
008 | | 181129s2018 |||||||||||||||||c||eng d |
020 | |
▼a 9780438169531 |
035 | |
▼a (MiAaPQ)AAI10826761 |
035 | |
▼a (MiAaPQ)umn:19307 |
040 | |
▼a MiAaPQ
▼c MiAaPQ
▼d 248032 |
082 | 0 |
▼a 530 |
100 | 1 |
▼a Meyers, Patrick Michael. |
245 | 10 |
▼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. |
502 | 1 |
▼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 |
710 | 20 |
▼a University of Minnesota.
▼b Physics. |
773 | 0 |
▼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 |
856 | 40 |
▼u http://www.riss.kr/pdu/ddodLink.do?id=T14998934
▼n KERIS |
980 | |
▼a 201812
▼f 2019 |
990 | |
▼a 관리자 |