New technology improves gravitational wave detectors by cutting quantum noise

An aerial view of the Laser Interferometer Gravitational-wave Observatory (LIGO) detector in Livingston, Louisiana. LIGO has two detectors: one in Livingston and the other in Hanaford, Washington. LIGO is funded by NSF; Caltech and MIT conceived, built and operate the laboratories. Credit: LIGO Laboratory

Physicists have successfully developed a new instrument that significantly reduces quantum-level noise that has thus far limited experiments' ability to spot gravitational waves. Collisions between massive black holes and stars are thought to generate these ripples in space-time that were first detected in 2015. In all, about 11 detections have been fully confirmed so far.

The device marks a major improvement to the Laser Interferometer Gravitational-Wave Observatory, or LIGO, increasing its detection range by 15%. Since the sky is a sphere, scientists expect to be able to detect about 50% more . They now predict that they will catch dozens of these rarely detected events during LIGO's ongoing experiment run through April 2020, which could transform their understanding of the phenomena. The collaboration published their findings today in the journal Physical Review Letters.

"This is really the turning point, because now we can really do statistics" with all these detections, said Lisa Barsotti, an MIT astrophysicist and one of the scientists leading the effort. "That's why it's becoming a new era in gravitational wave astronomy."

LIGO's detectors in Hanford, Washington and Livingston, Louisiana reveal an incoming gravitational wave using giant interferometers. These involve lasers bouncing off mirrors and traveling along two L-shaped arms 4 kilometers in length. A gravitational wave strains the arms so that the pair of beams become out of phase.

But physicists' ability to detect such a tiny signal is limited by seemingly insurmountable quantum noise, due to random fluctuations that slightly modulate the arrival time of photons, the smallest quantum bits of laser light. To remedy that, Barsotti and her colleagues use a quantum "squeezer," a crystal in the cavity of the arms of the interferometer that manipulates the interactions between the laser and the quantum vacuum and produces smaller fluctuations among the photons.

The achievement brought together expertise in and astrophysics and enables more sensitive detections of black holes and extremely dense neutron stars as they smash into each other. Other colliding objects, like supernova explosions and more typical stars, create gravitational waves that are still too tiny to pick out with current technologies.

Similar quantum squeezing devices are also being tested by LIGO's European counterparts in Advanced Virgo, using detectors built in northern Italy. Barsotti predicts that quantum squeezed light will become the standard for all next-generation detectors, like the proposed Cosmic Explorer, which would have arms stretching 40 kilometers on the ground, further increasing its sensitivity.

More information: M. Tse et al. Quantum-Enhanced Advanced LIGO Detectors in the Era of Gravitational-Wave Astronomy, Physical Review Letters (2019). DOI: 10.1103/PhysRevLett.123.231107

F. Acernese et al. Increasing the Astrophysical Reach of the Advanced Virgo Detector via the Application of Squeezed Vacuum States of Light, Physical Review Letters (2019). DOI: 10.1103/PhysRevLett.123.231108

Journal information: Physical Review Letters

This story is republished courtesy of Inside Science. Read the original story here. Used with permission. Inside Science is an editorially independent news service of the American Institute of Physics.

Citation: New technology improves gravitational wave detectors by cutting quantum noise (2019, December 12) retrieved 14 June 2024 from
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