Techniques for improving the readout sensitivity of gravitational wave antennae

Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2012.

Bibliographic Details
Main Author: Smith-Lefebvre, Nicolás de Mateo
Other Authors: Nergis Mavalvala and Peter Fritschel.
Format: Thesis
Language:eng
Published: Massachusetts Institute of Technology 2013
Subjects:
Online Access:http://hdl.handle.net/1721.1/77253
_version_ 1826205467042381824
author Smith-Lefebvre, Nicolás de Mateo
author2 Nergis Mavalvala and Peter Fritschel.
author_facet Nergis Mavalvala and Peter Fritschel.
Smith-Lefebvre, Nicolás de Mateo
author_sort Smith-Lefebvre, Nicolás de Mateo
collection MIT
description Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2012.
first_indexed 2024-09-23T13:13:18Z
format Thesis
id mit-1721.1/77253
institution Massachusetts Institute of Technology
language eng
last_indexed 2024-09-23T13:13:18Z
publishDate 2013
publisher Massachusetts Institute of Technology
record_format dspace
spelling mit-1721.1/772532019-04-12T21:41:39Z Techniques for improving the readout sensitivity of gravitational wave antennae Smith-Lefebvre, Nicolás de Mateo Nergis Mavalvala and Peter Fritschel. Massachusetts Institute of Technology. Dept. of Physics. Massachusetts Institute of Technology. Dept. of Physics. Physics. Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2012. This electronic version was submitted by the student author. The certified thesis is available in the Institute Archives and Special Collections. Cataloged from student-submitted PDF version of thesis. Includes bibliographical references (p. 135-143). The detection of gravitational waves (GWs) from astrophysical sources shows promise as a new method to probe extremely energetic phenomena and test the strong field limit of the general theory of relativity. The era of the first generation of broadband interferometric GW antennae is now drawing to a close, and the construction of the second generation has begun. The Laser Interferometer Gravitational-wave Observatory (LIGO) in the United States is one component of a worldwide array of sites designed to collectively record and analyze these GW signals. In preparation for the next major phase of operation, named Advanced LIGO, an incremental upgrade and prototyping project known as Enhanced LIGO introduced several upgrades to the initial LIGO detectors. The addition of the output mode cleaner (OMC), a critically coupled optical cavity designed to filter undesired light from the output of the interferometer before the GW signal is sensed on a photodetector, was one of these upgrades. This work describes several lessons learned as a result of the installation and commissioning of the OMC in Enhanced LIGO. The techniques described in this thesis include the development of a novel OMC alignment system designed to maximally transmit the GW signal in the presence of contamination that would confound a typical automatic alignment system, a design for a remotely controllable automatic mode matching system for the OMC, and prescriptions for reducing the presence of beam jitter noise associated with the OMC. The designs of each of the future GW detectors include the use of an OMC, thus the techniques described in this thesis will be directly applicable to achieving the maximum sensitivity of these detectors. by Nicolás de Mateo Smith-Lefebvre. Ph.D. 2013-03-01T14:33:32Z 2013-03-01T14:33:32Z 2012 2012 Thesis http://hdl.handle.net/1721.1/77253 827334806 eng M.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission. http://dspace.mit.edu/handle/1721.1/7582 143 p. application/pdf Massachusetts Institute of Technology
spellingShingle Physics.
Smith-Lefebvre, Nicolás de Mateo
Techniques for improving the readout sensitivity of gravitational wave antennae
title Techniques for improving the readout sensitivity of gravitational wave antennae
title_full Techniques for improving the readout sensitivity of gravitational wave antennae
title_fullStr Techniques for improving the readout sensitivity of gravitational wave antennae
title_full_unstemmed Techniques for improving the readout sensitivity of gravitational wave antennae
title_short Techniques for improving the readout sensitivity of gravitational wave antennae
title_sort techniques for improving the readout sensitivity of gravitational wave antennae
topic Physics.
url http://hdl.handle.net/1721.1/77253
work_keys_str_mv AT smithlefebvrenicolasdemateo techniquesforimprovingthereadoutsensitivityofgravitationalwaveantennae