This article has been reviewed according to Science X's editorial process and policies. Editors have highlighted the following attributes while ensuring the content's credibility: Researchers have developed and tested a new locking method for gravitational wave detectors that will advance the discovery of distant black holes and neutron stars colliding. Researchers from ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav) nodes at The University of Western Australia, the Australian National University and the University of Adelaide co-authored the study published in Physical Review D.
Jian Liu, from UWA's School of Physics, Mathematics and Computing, said gravitational wave detectors, such as LIGO, detected ripples in space-time created by colliding black holes by measuring changes in distance 1,000 times smaller than the width of a proton. "To do this, the detector's 40-kilogram (88-pound) mirrors, which sit four kilometers (2.5 miles) apart, must be locked in exactly the right positions using laser light," Liu said. "Before the detector can start listening to the universe, the mirrors must be gently brought to rest and locked in place by a system called arm-length stabilization or the locking system.
"The next upgrade of LIGO will use new crystalline mirror coating technology to improve sensitivity, but the coating absorbs the green laser light the current locking system relies on." Researchers developed and tested a new locking scheme using infrared light (1596 nanometers), a color the new coatings do not absorb. Special crystals were used to convert the frequency of the light, changing the locking infrared light (1596 nm) and the detector's main (1064 nm) laser light into green light, which allowed control to be handed over smoothly from the locking laser to the main laser. "We demonstrated a stable handover from the locking laser to the main laser that took about 60 seconds, which is much faster than the current system, and repeated it successfully over several days," Liu said.
"Based on these results, we estimate the measurement error between the lasers to be incredibly small—about one-tenth the width of an atom even when measuring along a four-kilometer (2.5-mile) LIGO laser arm." The findings show a practical locking method exists for gravitational wave detectors that use the new low-noise crystalline mirror coatings. Jian Liu et al., Novel arm-length stabilization scheme for gravitational-wave detectors with AlGaAs/GaAs coated mirrors, Physical Review D (2026). On arXiv: arxiv.org/abs/2606.24149 Journal information: Physical Review D , arXiv Provided by University of Western Australia Swati Mestri holds a bachelor's degree in Electronics Engineering and has worked as a content editor since 2019.
She has experience editing research documents across technology, health care, and materials science, and has a particular interest in technology and space. Full profile → Bachelor's in mathematical biology, Master's in creative writing. Well-traveled with unique perspectives on science and language.
Extract — continue reading at the source.
