Physicists Quiet the Quantum Whisper to Improve Gravitational Wave Detector Sensitivity

Gravitational Waves Concept

Using a miniature mirror the size of a human hair, researchers successfully reduced quantum backaction in a simplified system, confirming theoretical predictions.

By quieting the quantum whisper, we can now listen to the more subtle notes of the cosmic symphony.

Gravitational wave detectors have opened a new window to the universe by measuring the ripples in spacetime produced by colliding black holes and neutron stars, but they are ultimately limited by quantum fluctuations induced by light reflecting off of mirrors. LSU Ph.D. physics alumnus Jonathan Cripe, postdoctorsl fellow, NIST, and his team of LSU researchers have conducted a new experiment with scientists from Caltech and Thorlabs to explore a way to cancel this quantum backaction and improve detector sensitivity.

In a new paper in Physical Review X, the investigators present a method for removing quantum backaction in a simplified system using a mirror the size of a human hair and show the motion of the mirror is reduced in agreement with theoretical predictions. The research was supported by the National Science Foundation.

Jonathan Cripe

Louisiana State University Ph.D. physics alumnus Jonathan Cripe has conducted a new experiment with scientists from Caltech and Thorlabs to explore a way to improve gravitational wave detectors’ sensitivity. Credit: LSU

Despite using 40-kilogram mirrors for detecting passing gravitational waves, quantum fluctuations of light disturb the position of the mirrors when the light is reflected. As gravitational wave detectors continue to grow more sensitive with incremental upgrades, this quantum backaction will become a fundamental limit to the detectors’ sensitivity, hampering their ability to extract astrophysical information from gravitational waves.

Thomas Corbitt

LSU Associate Professor Thomas Corbitt. Credit: Elsa Hahne / LSU ORED

“We present an experimental testbed for studying and eliminating quantum backaction,” Cripe said. “We perform two measurements of the position of a macroscopic object whose motion is dominated by quantum backaction and show that by making a simple change in the measurement scheme, we can remove the quantum effects from the displacement measurement. By exploiting correlations between the phase and intensity of an optical field, quantum backaction is eliminated.”

Torrey Cullen

LSU Graduate Student Torrey Cullen. Credit: Paige Whittington / LSU Physics & Astronomy

Garrett Cole, technology manager at Thorlabs Crystalline Solutions (Crystalline Mirror Solutions was acquired by Thorlabs Inc. last year), and his team constructed the micromechanical mirrors from an epitaxial multilayer consisting of alternating GaAs and AlGaAs. An outside foundry, IQE North Carolina, grew the crystal structure while Cole and his team, including process engineers Paula Heu and David Follman, manufactured the devices at the University of California Santa Barbara nanofabrication facility. “By performing this measurement on a mirror visible to the naked eye—at room temperature and at frequencies audible to the human ear—we bring the subtle effects of quantum mechanics closer to the realm of human experience,” LSU Ph.D. candidate Torrey Cullen said. By quieting the quantum whisper, we can now listen to the more subtle notes of the cosmic symphony.”

“This research is especially timely because the Laser Interferometer Gravitational-wave Observatory, or LIGO, just announced last month in Nature that they have seen the effects of quantum radiation pressure noise at the LIGO Livingston observatory,” Thomas Corbitt, associate professor in the LSU Department of Physics & Astronomy, said.

The effort behind that paper, “Quantum correlations between light and the kilogram-mass mirrors of LIGO,” has been led by Nergis Mavalvala, dean of the MIT School of Science, as well as postdoctoral scholar Haocun Yu and research scientist Lee McCuller, both at the MIT Kavli Institute for Astrophysics and Space Research.

“Quantum radiation pressure noise is already poking out of the noise floor in Advanced LIGO, and before long, it will be a limiting noise source in GW detectors,” Mavalvala said. “Deeper astrophysical observations will only be possible if we can reduce it, and this beautiful result from the Corbitt group at LSU demonstrates a technique for doing just that.”

Reference: “Quantum Backaction Cancellation in the Audio Band” by Jonathan Cripe, Torrey Cullen, Yanbei Chen, Paula Heu, David Follman, Garrett D. Cole and Thomas Corbitt, 23 September 2020, Physical Review X.
DOI: 10.1103/PhysRevX.10.031065

4 Comments on "Physicists Quiet the Quantum Whisper to Improve Gravitational Wave Detector Sensitivity"

  1. Brilliant work by the LSU student. A game changer for astrophysics research. It has the potential to change our understanding of the universe.

  2. Exciting results! Nergis Mavalvala (quoted in the article) will be giving a public lecture on detecting gravitational waves on Thursday Oct. 1st at 6:30pm EDT. Anyone can join the livestream for free to learn more (link below).

  3. Livestream link for a talk by Nergis Mavalvala:

  4. Anyone considering what happens when gravitational waves interfere with each other?

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