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Precision mirrors poised to improve sensitivity of gravitational wave detectors:
Researchers have developed a new type of deformable mirror that could increase the sensitivity of ground-based gravitational wave detectors such as the Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO). Advanced LIGO measures faint ripples in space time called gravitational waves, which are caused by distant events such as collisions between black holes or neutron stars.
"In addition to improving today's gravitational wave detectors, these new mirrors will also be useful for increasing sensitivity in next generation detectors and allow detection of new sources of gravitational waves," said research team leader Huy Tuong Cao from the University of Adelaide node of the Australian Center of Excellence for Gravitational Waves Discovery (OzGrav).
Deformable mirrors, which are used to shape and control laser light, have a surface made of tiny mirrors that can each be moved, or actuated, to change the overall shape of the mirror. As detailed in The Optical Society's (OSA) journal Applied Optics, Cao and colleagues have, for the first time, made a deformable mirror based on the bimetallic effect in which a temperature change is used to achieve mechanical displacement.
"Our new mirror provides a large actuation range with great precision," said Cao. "The simplicity of the design means it can turn commercially available optics into a deformable mirror without any complicated or expensive equipment. This makes it useful for any system where precise control of beam shape is crucial."
[...] Most deformable mirrors use thin mirrors to induce large amount of actuation, but these thin mirrors can produce undesirable scattering because they are hard to polish. The researchers designed a new type of deformable mirror using the bimetallic effect by attaching a piece of metal to a glass mirror. When the two are heated together the metal expands more than the glass, causing the mirror to bend.
The new design not only creates a large amount of precise actuation but is also compact and requires minimum modifications to existing systems. Both the fused silica mirrors and aluminum plates used to create the deformable mirror are commercially available. To attach the two layers, the researchers carefully selected a bonding adhesive that would maximize actuation.
Journal Reference:
Huy Tuong Cao et al. High dynamic range thermally actuated bimorph mirror for gravitational wave detectors, Applied Optics (2020). (DOI: 10.1364/AO.376764)
(Score: 0) by Anonymous Coward on Thursday March 19 2020, @05:27PM (6 children)
Very cool. I bet a lot of telescope designers are kicking themselves about now, wishing they had come up with this idea.
(Score: 2) by Barenflimski on Thursday March 19 2020, @06:44PM (1 child)
I've been kicking myself for not coming up with the One-Click-Shopping patent for 20 years now.
(Score: 0) by Anonymous Coward on Thursday March 19 2020, @09:31PM
You can stop kicking yourself now--
> In the United States, under current patent law, the term of patent, provided that maintenance fees are paid on time, is 20 years from the filing date of the earliest U.S. or international (PCT) application to which priority is claimed (excluding provisional applications).
(Score: 3, Informative) by Anonymous Coward on Thursday March 19 2020, @07:30PM (3 children)
No, this is not useful for telescope designers. Adaptive optics are used there to correct the wavefront that has been disturbed by atmospheric effects. This is for very slow corrections. Because it depends upon thermal effects, its response time is on par with thermally induced changes. If you look in their paper, Figure 7 specifically, you'll see that it take over an hour to go from one steady state to another.
(Score: 0) by Anonymous Coward on Thursday March 19 2020, @09:29PM (2 children)
Spotted the person that read the link!
(Score: 0) by Anonymous Coward on Friday March 20 2020, @03:17PM
Not only that, but I read the paper behind the link!
(Score: 0) by Anonymous Coward on Friday March 20 2020, @03:18PM
Ha-ha! NERD!