Squeeze leads to stellar-mass black hole collision precision

Squeeze leads to stellar-mass black hole collision precision
Artist’s depiction of a black hole about to swallow a neutron star. Credit: Carl Knox, OzGrav ARC Centre of Excellence

Scientists at The Australian National University (ANU) have found a way to better detect all collisions of stellar-mass black holes in the universe.

Stellar-mass black holes are formed by the gravitational collapse of a star. Their collisions are some of the most violent events in the universe, creating or ripples in space-time.

These ripples are miniscule and detected using laser interferometers. Until now, many signals have been drowned out by so-called on the pushing the mirrors of the laser interferometer around—making the measurements fuzzy or imprecise.

The researchers' new method, called "squeezing," dampens quantum noise making measurements more precise, with the findings published in Nature Photonics.

The breakthrough will be critical for next-generation detectors, which are expected to come online within the next 20 years.

One of the researchers involved, Dr. Robert Ward, said further experiments were being prepared to confirm the team's proof of concept for a new device to dampen the effect of quantum noise.

"The detectors use particles of light called photons from a laser beam to sense the change in position of widely separate mirrors," said Dr. Ward, from the ANU Research School of Physics and the ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav).

"However, the detectors are so sensitive that just the random quantum variability in the number of photons can disturb the mirrors enough to mask the wave-induced motion."

The researchers have shown that squeezing reduces this variability, making detectors more sensitive.

The Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) detectors in the United States and the European Gravitational Observatory's in Italy called Virgo have detected the mergers of two black holes, the collision of two neutron stars and possibly also a black hole eating a neutron star.

ANU plays a lead role in Australia's partnership with LIGO. Other members of the quantum squeezer team include Professor David McClelland, Ph.D. scholar Min Jet Yap and Dr. Bram Slagmolen.

"The 'quantum squeezers' we designed at ANU along with other upgrades for the current LIGO detectors have greatly improved their sensing capabilities," Dr. Slagmolen said.

Mr Yap said the latest experiment proves that scientists can cancel out other quantum noise that can affect the sensing capabilities of detectors.

"The new-generation LIGO detectors will have the capability to detect every black-hole smash in the universe at any given moment," he said.

The LIGO team plans to design and build the upgraded quantum squeezers within the next few years. The new devices could be retrofitted to the current LIGO detectors, enabling scientists to detect many more violent events much further into the universe.


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More information: Min Jet Yap et al. Broadband reduction of quantum radiation pressure noise via squeezed light injection, Nature Photonics (2019). DOI: 10.1038/s41566-019-0527-y
Journal information: Nature Photonics

Citation: Squeeze leads to stellar-mass black hole collision precision (2019, October 31) retrieved 29 October 2020 from https://phys.org/news/2019-10-stellar-mass-black-hole-collision-precision.html
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