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Topics of LIGO physics: Quantum noi...

Chen, Yanbei.

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Topics of LIGO physics: Quantum noise in advanced interferometers and template banks for compact-binary inspirals.

Record Type:	Electronic resources : Monograph/item
Title/Author:	Topics of LIGO physics: Quantum noise in advanced interferometers and template banks for compact-binary inspirals./
Author:	Chen, Yanbei.
Description:	426 p.
Notes:	Source: Dissertation Abstracts International, Volume: 64-06, Section: B, page: 2714.
Contained By:	Dissertation Abstracts International64-06B.
Subject:	Physics, Astronomy and Astrophysics. -
Online resource:	http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=3093476
ISBN:	0496411799

Topics of LIGO physics: Quantum noise in advanced interferometers and template banks for compact-binary inspirals.
Chen, Yanbei.

Topics of LIGO physics: Quantum noise in advanced interferometers and template banks for compact-binary inspirals. - 426 p.

Source: Dissertation Abstracts International, Volume: 64-06, Section: B, page: 2714.

Thesis (Ph.D.)--California Institute of Technology, 2003.

This thesis deals with the planning for advanced interferometeric gravitational-wave detectors, as well as the detection of inspiral waves using first-generation interferometers.

ISBN: 0496411799Subjects--Topical Terms:

1019521
Physics, Astronomy and Astrophysics.

Topics of LIGO physics: Quantum noise in advanced interferometers and template banks for compact-binary inspirals.
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100 1 $a Chen, Yanbei. $3 1935693
245 1 0 $a Topics of LIGO physics: Quantum noise in advanced interferometers and template banks for compact-binary inspirals.
300 $a 426 p.
500 $a Source: Dissertation Abstracts International, Volume: 64-06, Section: B, page: 2714.
500 $a Adviser: Kip S. Thorne.
502 $a Thesis (Ph.D.)--California Institute of Technology, 2003.
520 $a This thesis deals with the planning for advanced interferometeric gravitational-wave detectors, as well as the detection of inspiral waves using first-generation interferometers.
520 $a In Chapters 2--4 (in collaboration with Alessandra Buonanno), the signal recycling interferometer proposed for LIGO-II is studied in the two-photon formalism. This study reveals the optical spring effect, which allows the interferometer to beat the standard quantum limit, while in the same time introduces a dynamical instability. A classical control system is designed to suppress this instability. In Chapter 5 (in collaboration with Alessandra Buonanno and Nergis Mavalvala), the quantum noise in heterodyne readout schemes for advanced interferometers is studied. In Chapter 6 (in collaboration with Patricia Purdue), a QND Speed-Meter interferometer with Michelson topology is proposed, analyzed and shown to be a promising candidate for third-generation interferometers (LIGO-III or EURO). This design requires adding a kilometer-scale cavity into the interferometer. In Chapter 7, Sagnac interferometers are analyzed and shown to exhibit a similar broadband QND performance without the need of additional cavity---as expected since these interferometers are sensitive only to time-dependent mirror displacement, and are automatic speed meters.
520 $a In Chapter 8 (in collaboration with Alessandra Buonanno and Michele Vallisneri), the Post-Newtonian (PN) breakdown at late-stage inspirals of non-spinning binary black holes (with 5 M&odot; < m1, m2 < 20 M&odot; ) is studied. We propose the use of Detection Template Families (DTFs)---extensions of ordinary PN templates that can mimic all different PN waveforms and hence are plausible to catch the real waveform, yet do not provide straightforward parameter estimation.
520 $a In Chapter 9 (in collaboration with Alessandra Buonanno and Michele Vallisneri), binaries carrying spins are studied using an adiabatic PN model. Based on features of the precession dynamics, we construct a DTF, using a modified Apostolatos' ansatz, that can mimic the modulated waveforms reasonably well, while keeping a small number of parameters to be searched over one by one, with the rest searched over automatically. We also propose a (computationally) plausible way of searching over the entire physical parameter space of neutron-star-black-hole binaries.
590 $a School code: 0037.
650 4 $a Physics, Astronomy and Astrophysics. $3 1019521
650 4 $a Physics, Optics. $3 1018756
690 $a 0606
690 $a 0752
710 2 0 $a California Institute of Technology. $3 726902
773 0 $t Dissertation Abstracts International $g 64-06B.
790 1 0 $a Thorne, Kip S., $e advisor
790 $a 0037
791 $a Ph.D.
792 $a 2003
856 4 0 $u http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=3093476