Prospects of High Precision Fiber for Gravitational Wave Detection
Abstract/Contents
- Abstract
- All current gravitational wave (GW) detectors, such as those of the Laser Interferometer Gravitational-wave Observatory (LIGO) and Virgo, are precision optical interferometers with sub-attometer displacement sensitivity. Free space propagation of the optical beams of LIGO requires large (meter diameter and kilometers of length) evacuated stainless steel beam tubes that come with sizable manufacturing and operational costs. A fiber-based detector – with the free space beams of present schemes replaced by concentrated fiber spools – could mitigate these costs while simultaneously offering a more compact experimental setup. This thesis proposes a design for and carries out the strain calculations for a hypothetical Michaelson Morley fiber interferometer over a wide frequency range. Limits on thermoconductive, thermomechanical, and shot noise sources are established and compounded to arrive at an estimate of the overall noise floor. Considering an interferometer arm length comparable to that used in the current generation of detectors, we estimate the strain sensitivity at 1 kHz to be around 10^(−16)√Hz. Advanced cooling strategies, the novel fiber technologies mentioned above, and parameter tuning in the thermal noise are all potential options for improving on this baseline sensitivity. The thesis concludes by summarizing the major developments in each area, and the long-term outlook of using such detectors for detecting gravitational waves.
Description
Type of resource | text |
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Date created | May 2021 |
Creators/Contributors
Author | Shadmany, Danial |
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Degree granting institution | Stanford University, Department of Physics |
Primary advisor | Mavalvala, Nergis |
Advisor | Graham, Peter |
Subjects
Subject | gravitational wave detection |
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Subject | optical fiber |
Subject | optical fiber technology |
Genre | Thesis |
Bibliographic information
Access conditions
- Use and reproduction
- User agrees that, where applicable, content will not be used to identify or to otherwise infringe the privacy or confidentiality rights of individuals. Content distributed via the Stanford Digital Repository may be subject to additional license and use restrictions applied by the depositor.
- License
- This work is licensed under a Creative Commons Attribution Non Commercial 3.0 Unported license (CC BY-NC).
Preferred citation
- Preferred Citation
- Shadmany, Danial. (2021). Prospects of High Precision Fiber for Gravitational Wave Detection. Stanford Digital Repository. Available at: https://purl.stanford.edu/pr899zh2360
Collection
Undergraduate Theses, Department of Physics
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- Contact
- shadmany@stanford.edu
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