Studies of silicon test mass properties for future gravitational wave detectors

Vahid Jaberian Hamedan

doi:10.26182/f08j-tj04

Studies of silicon test mass properties for future gravitational wave detectors

Vahid Jaberian Hamedan

School of Physics, Mathematics and Computing

Research output: Thesis › Doctoral Thesis

225 Downloads (Pure)

Abstract

The sensitivity of current gravitational wave detectors is limited by a variety of noise sources. Further improvements require significant modifications in the interferometer structure and operation. Operating at cryogenic temperatures, increasing laser power, and changing the optics materials are some of the proposed modifications for future gravitational wave detectors. The excellent properties of silicon at cryogenic temperatures make it one of the most interesting materials for future test masses. However, using Si test masses has some challenges, such as birefringence. In this thesis, some of the main silicon properties for use in future gravitational wave detectors were discussed.

Original language	English
Qualification	Doctor of Philosophy
Awarding Institution	The University of Western Australia
Supervisors/Advisors	Zhao, Chunnong, Supervisor Ju, Li, Supervisor Blair, Carl, Supervisor
Award date	26 May 2023
DOIs	https://doi.org/10.26182/f08j-tj04
Publication status	Unpublished - 2023

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10.26182/f08j-tj04

THESIS - DOCTOR OF PHILOSOPHY - HAMEDAN Vahid Jaberian -2023
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3 Article

Precision mapping of a silicon test mass birefringence
Jaberian Hamedan, V., Adam, A., Blair, C., Ju, L. & Zhao, C., 6 Feb 2023, In: Applied Physics Letters. 122, 6, 064101.
Research output: Contribution to journal › Article › peer-review

Open Access
9 Link opens in a new tab Citations (Scopus)
High mechanical Q-factor measurement of Si using a 3D cantilever support
Hamedan, V. J., Winterflood, J., Blair, C., Ju, L. & Zhao, C., 1 Oct 2022, In: Review of Scientific Instruments. 93, 10, 6 p., 104501.
Research output: Contribution to journal › Article › peer-review

Open Access
File
149 Downloads (Pure)
Demonstration of dynamic thermal compensation for parametric instability suppression in Advanced LIGO
Hardwick, T., Jaberian Hamedan, V., Blair, C., Green, A. C. & Vander-Hyde, D., 22 Oct 2020, In: Classical and Quantum Gravity. 37, 20, ab8be9.
Research output: Contribution to journal › Article › peer-review

Open Access
9 Link opens in a new tab Citations (Web of Science)

Cite this

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title = "Studies of silicon test mass properties for future gravitational wave detectors",

abstract = "The sensitivity of current gravitational wave detectors is limited by a variety of noise sources. Further improvements require significant modifications in the interferometer structure and operation. Operating at cryogenic temperatures, increasing laser power, and changing the optics materials are some of the proposed modifications for future gravitational wave detectors. The excellent properties of silicon at cryogenic temperatures make it one of the most interesting materials for future test masses. However, using Si test masses has some challenges, such as birefringence. In this thesis, some of the main silicon properties for use in future gravitational wave detectors were discussed.",

keywords = "Gravitational waves, Silicon test mass, Birefringence, Thermal transient, Mechanical Q-factor, Mechanical stress, High laser power, Gravitational waves detector",

author = "\{Jaberian Hamedan\}, Vahid",

year = "2023",

doi = "10.26182/f08j-tj04",

language = "English",

school = "The University of Western Australia",

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TY - BOOK

T1 - Studies of silicon test mass properties for future gravitational wave detectors

AU - Jaberian Hamedan, Vahid

PY - 2023

Y1 - 2023

N2 - The sensitivity of current gravitational wave detectors is limited by a variety of noise sources. Further improvements require significant modifications in the interferometer structure and operation. Operating at cryogenic temperatures, increasing laser power, and changing the optics materials are some of the proposed modifications for future gravitational wave detectors. The excellent properties of silicon at cryogenic temperatures make it one of the most interesting materials for future test masses. However, using Si test masses has some challenges, such as birefringence. In this thesis, some of the main silicon properties for use in future gravitational wave detectors were discussed.

AB - The sensitivity of current gravitational wave detectors is limited by a variety of noise sources. Further improvements require significant modifications in the interferometer structure and operation. Operating at cryogenic temperatures, increasing laser power, and changing the optics materials are some of the proposed modifications for future gravitational wave detectors. The excellent properties of silicon at cryogenic temperatures make it one of the most interesting materials for future test masses. However, using Si test masses has some challenges, such as birefringence. In this thesis, some of the main silicon properties for use in future gravitational wave detectors were discussed.

KW - Gravitational waves

KW - Silicon test mass

KW - Birefringence

KW - Thermal transient

KW - Mechanical Q-factor

KW - Mechanical stress

KW - High laser power

KW - Gravitational waves detector

U2 - 10.26182/f08j-tj04

DO - 10.26182/f08j-tj04

M3 - Doctoral Thesis

ER -

Studies of silicon test mass properties for future gravitational wave detectors

Abstract

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Research output

Precision mapping of a silicon test mass birefringence

High mechanical Q-factor measurement of Si using a 3D cantilever support

Demonstration of dynamic thermal compensation for parametric instability suppression in Advanced LIGO

Cite this