Characterisation of optical materials for next generation gravitational wave detectors
Lead Research Organisation:
University of Glasgow
Department Name: School of Physics and Astronomy
Abstract
Characterisation of optical materials for next generation gravitational wave detectors
People |
ORCID iD |
Iain Martin (Primary Supervisor) | |
Simon Tait (Student) |
Publications
Abbott R
(2021)
All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run
in Physical Review D
Abbott R
(2022)
Search for Subsolar-Mass Binaries in the First Half of Advanced LIGO's and Advanced Virgo's Third Observing Run.
in Physical review letters
Abbott R
(2022)
All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 data
in Physical Review D
Abbott R
(2022)
Model-based Cross-correlation Search for Gravitational Waves from the Low-mass X-Ray Binary Scorpius X-1 in LIGO O3 Data
in The Astrophysical Journal Letters
Abbott R
(2022)
Search for continuous gravitational wave emission from the Milky Way center in O3 LIGO-Virgo data
in Physical Review D
Abbott R
(2022)
Search for gravitational waves from Scorpius X-1 with a hidden Markov model in O3 LIGO data
in Physical Review D
Abbott R
(2022)
All-sky, all-frequency directional search for persistent gravitational waves from Advanced LIGO's and Advanced Virgo's first three observing runs
in Physical Review D
Abbott R
(2021)
All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems
in Physical Review D
Abbott R
(2021)
Tests of general relativity with binary black holes from the second LIGO-Virgo gravitational-wave transient catalog
in Physical Review D
Abbott R
(2020)
GW190814: Gravitational Waves from the Coalescence of a 23 Solar Mass Black Hole with a 2.6 Solar Mass Compact Object
in The Astrophysical Journal Letters
Abbott R
(2021)
Searches for Continuous Gravitational Waves from Young Supernova Remnants in the Early Third Observing Run of Advanced LIGO and Virgo
in The Astrophysical Journal
Abbott R
(2020)
Gravitational-wave Constraints on the Equatorial Ellipticity of Millisecond Pulsars
in The Astrophysical Journal Letters
Abbott R
(2021)
Search for Lensing Signatures in the Gravitational-Wave Observations from the First Half of LIGO-Virgo's Third Observing Run
in The Astrophysical Journal
Abbott R
(2021)
Diving below the Spin-down Limit: Constraints on Gravitational Waves from the Energetic Young Pulsar PSR J0537-6910
in The Astrophysical Journal Letters
Abbott R
(2022)
Search of the early O3 LIGO data for continuous gravitational waves from the Cassiopeia A and Vela Jr. supernova remnants
in Physical Review D
Abbott R
(2021)
Constraints on Cosmic Strings Using Data from the Third Advanced LIGO-Virgo Observing Run
in Physical Review Letters
Abbott R
(2021)
All-sky search for continuous gravitational waves from isolated neutron stars in the early O3 LIGO data
in Physical Review D
Abbott R
(2021)
Observation of Gravitational Waves from Two Neutron Star-Black Hole Coalescences
in The Astrophysical Journal Letters
Abbott R
(2022)
Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift during the LIGO-Virgo Run O3b
in The Astrophysical Journal
Abbott R
(2022)
Narrowband Searches for Continuous and Long-duration Transient Gravitational Waves from Known Pulsars in the LIGO-Virgo Third Observing Run
in The Astrophysical Journal
Abbott R
(2021)
Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO and Advanced Virgo's first three observing runs
in Physical Review D
Abbott R
(2020)
Properties and Astrophysical Implications of the 150 M ? Binary Black Hole Merger GW190521
in The Astrophysical Journal
Abbott R
(2021)
Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog
in The Astrophysical Journal Letters
Abbott R
(2022)
All-sky search for gravitational wave emission from scalar boson clouds around spinning black holes in LIGO O3 data
in Physical Review D
Abbott R
(2020)
GW190521: A Binary Black Hole Merger with a Total Mass of 150 M_{?}.
in Physical review letters
Abbott R
(2022)
Search for intermediate-mass black hole binaries in the third observing run of Advanced LIGO and Advanced Virgo
in Astronomy & Astrophysics
Abbott R
(2021)
All-sky search for long-duration gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run
in Physical Review D
Abbott R
(2020)
GW190412: Observation of a binary-black-hole coalescence with asymmetric masses
in Physical Review D
Abbott R
(2021)
GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo during the First Half of the Third Observing Run
in Physical Review X
Abbott R
(2021)
Upper limits on the isotropic gravitational-wave background from Advanced LIGO and Advanced Virgo's third observing run
in Physical Review D
Abbott R
(2021)
Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift during the LIGO-Virgo Run O3a
in The Astrophysical Journal
Abbott R
(2022)
Constraints on dark photon dark matter using data from LIGO's and Virgo's third observing run
in Physical Review D
Abernathy M
(2021)
Exploration of co-sputtered Ta 2 O 5 -ZrO 2 thin films for gravitational-wave detectors
in Classical and Quantum Gravity
Adhikari R
(2020)
A cryogenic silicon interferometer for gravitational-wave detection
in Classical and Quantum Gravity
Albert A
(2019)
Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube
in The Astrophysical Journal
Albert A
(2017)
Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory
in The Astrophysical Journal
Birney R
(2018)
Amorphous Silicon with Extremely Low Absorption: Beating Thermal Noise in Gravitational Astronomy
in Physical Review Letters
Burns E
(2019)
A Fermi Gamma-Ray Burst Monitor Search for Electromagnetic Signals Coincident with Gravitational-wave Candidates in Advanced LIGO's First Observing Run
in The Astrophysical Journal
Fletcher M
(2018)
Effect of Stress and Temperature on the Optical Properties of Silicon Nitride Membranes at 1,550 nm
in Frontiers in Materials
Hamburg R
(2020)
A Joint Fermi-GBM and LIGO/Virgo Analysis of Compact Binary Mergers from the First and Second Gravitational-wave Observing Runs
in The Astrophysical Journal
Kiessling F
(2022)
Quasi-monocrystalline silicon for low-noise end mirrors in cryogenic gravitational-wave detectors
in Physical Review Research
LIGO Scientific Collaboration And The Virgo Collaboration
(2017)
A gravitational-wave standard siren measurement of the Hubble constant.
in Nature
Rich Abbott
(2021)
Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo
in SoftwareX
Soares-Santos M
(2019)
First Measurement of the Hubble Constant from a Dark Standard Siren using the Dark Energy Survey Galaxies and the LIGO/Virgo Binary-Black-hole Merger GW170814
in The Astrophysical Journal
Tait S
(2020)
Demonstration of the Multimaterial Coating Concept to Reduce Thermal Noise in Gravitational-Wave Detectors
in Physical Review Letters
Studentship Projects
Project Reference | Relationship | Related To | Start | End | Student Name |
---|---|---|---|---|---|
ST/N504075/1 | 30/09/2015 | 30/03/2021 | |||
1802888 | Studentship | ST/N504075/1 | 30/09/2016 | 30/09/2019 | Simon Tait |
Description | The research presented in this thesis has been dedicated to the development of measurement techniques that can characterise a coating material's key material properties, which can affect the level of thermal noise and optical absorption produced by the coating material. As the next generation of gravitational wave detectors has a wide range of desired operation temperatures, wavelengths and laser cavity powers. Coating materials that complement each set of conditions are required. The main focus of this thesis was the experimental verification of a novel multi-material coating design. This coating stack, known as the `Full Stack' takes advantage of the low absorption of some silica and tantala layers to reduce the transmission of laser light to lower layers consisting of silica and amorphous silicon. The novel coating design requires less coating layers to produce the required 99.9999% optical reflectivity, which meets the requirements in reflectivity for gravitational wave detectors test mass optics. Measurements of the coatings optical absorption at a laser wavelength of 2000nm were carried out in conjunction with measurements of its mechanical loss. It was shown that by heat-treating the coatings to 500C for 3 hours that the optical and mechanical properties of the coating stack could be significantly improved. The properties of the Full Stack material were also measured using a custom cryogenic mechanical loss apparatus developed by the author, allowing its mechanical loss to be measured between 80K - 293K, providing crucial information for future, 3rd generation gravitational wave detectors which plan to operate at these ( or lower ) temperatures. |
Exploitation Route | The findings in this research will be of significant interest to the gravitational wave coatings community. The materials, and apparatus developed by the author will be replicated by other institutions allowing the same insight to be gained. |
Sectors | Other |
URL | https://link.aps.org/doi/10.1103/PhysRevLett.125.011102 |
Title | Measurement System for categorisation for Cryogenic mechanical loss of thin disk substrates |
Description | As the thermoelastic loss at room temperature dominates (phi) of silicon, this requires that the sample is cooled below the temperatures in which this dominates (< 200K). This would require that the sample and apparatus are placed inside a cryostat chamber where it can be evacuated to pressures 1x10-5,mbar and cooled. As the automatic suspension of silica disks was proven a viable method for balancing samples without external intervention, the same apparatus could, in theory, be adapted for this purpose. A system to measure the mechanical loss of thin cSi disks using the nodal support method was designed and built by myself and Mr R.Jones ( University of Glasgow ). This method allows for coating loss categorisation for materials which can reduce the total thermal noise in future cryogenic gravitational wave detectors. |
Type Of Material | Improvements to research infrastructure |
Year Produced | 2020 |
Provided To Others? | No |
Impact | This apparatus is a novel methodology which allows for measurements of coating loss in the cryogenic regime. Coating loss directly attributes to the limiting source of noise in gravitational wave detectors, and thus any method which aids for the categorisation of new materials to support this process is of the utmost importance for the gravitational wave detector community. |
Description | LIGO Scientific Collaboration |
Organisation | LIGO |
Country | United States |
Sector | Academic/University |
PI Contribution | Research focus for has been to provide measurements of optical absorption and mechanical loss of thin film coatings for future gravitational wave detector upgrades |
Collaborator Contribution | Research focus for has been to provide measurements of optical absorption and mechanical loss of thin film coatings for future gravitational wave detector upgrades |
Impact | optical absorption and mechanical loss of thin film coatings for future gravitational wave detector upgrades have been provided. The development of absorption monitoring of ETMs on site using mechanical eigenfrequencies was also implemented on site through this work |
Start Year | 2016 |
Description | Highschool masterclass for science outreach: Royal Society of Edinburgh |
Form Of Engagement Activity | A formal working group, expert panel or dialogue |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Schools |
Results and Impact | The Royal Society of Edinburgh (RSE) runs masterclasses for high school students to raise engagement in STEM subjects. These classes which I have lead involve a 1 hour talk, and team building exercises involving scientific themes such as aerodynamics, astronomy and structural engineering. |
Year(s) Of Engagement Activity | 2018,2019,2020 |
Description | Outreach Festival of Physics |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Public/other audiences |
Results and Impact | Outreach Physics Festival was a held at the Glasgow science centre with the aims of educating the general public on the outcomes of research produced by multiple universities in the area |
Year(s) Of Engagement Activity | 2018 |
Description | Physics&Astronomy Masterclass |
Form Of Engagement Activity | A formal working group, expert panel or dialogue |
Part Of Official Scheme? | No |
Geographic Reach | Local |
Primary Audience | Schools |
Results and Impact | Local school students with ages between 10 and 15 were invited to the unverisity for fun classes aimed to educated and open their minds to science. Looking at topics such as aerodynamics, rocketry and astrophysics |
Year(s) Of Engagement Activity | 2015,2016,2017,2018,2019 |
Description | Science Centre Open Day |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Geographic Reach | Local |
Primary Audience | Public/other audiences |
Results and Impact | Glasgow science centre open day was held with the aims of educating the general public on the outcomes of research produced by multiple universities in the area |
Year(s) Of Engagement Activity | 2018 |