Pulsar web could detect low-frequency gravitational waves

February 25, 2016 by Elizabeth Ferrara
Gravitational waves are ripples in space-time, represented by the green grid, produced by accelerating bodies such as interacting supermassive black holes. These waves affect the time it takes for radio signals from pulsars to arrive at Earth. Credit: David Champion

The recent detection of gravitational waves by the Laser Interferometer Gravitational-Wave Observatory (LIGO) came from two black holes, each about 30 times the mass of our sun, merging into one. Gravitational waves span a wide range of frequencies that require different technologies to detect. A new study from the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) has shown that low-frequency gravitational waves could soon be detectable by existing radio telescopes.

"Detecting this signal is possible if we are able to monitor a sufficiently large number of pulsars spread across the sky," said Stephen Taylor, lead author of the paper published this week in the Astrophysical Journal Letters. He is a postdoctoral researcher at NASA's Jet Propulsion Laboratory, Pasadena, California. "The smoking gun will be seeing the same pattern of deviations in all of them." Taylor and colleagues at JPL and the California Institute of Technology in Pasadena have been studying the best way to use pulsars to detect signals from low-frequency gravitational waves. Pulsars are highly magnetized neutron stars, the rapidly rotating cores of stars left behind when a massive star explodes as a supernova.

Einstein's general theory of relativity predicts that gravitational waves—ripples in spacetime—emanate from accelerating massive objects. Nanohertz gravitational waves are emitted from pairs of supermassive orbiting each other, each of which contain millions or a billion times more mass than those detected by LIGO. These black holes each originated at the center of separate galaxies that collided. They are slowly drawing closer together and will eventually merge to create a single super-sized black hole.

As they orbit each other, the black holes pull on the fabric of space and create a faint signal that travels outward in all directions, like a vibration in a spider's web. When this vibration passes Earth, it jostles our planet slightly, causing it to shift with respect to distant pulsars. Gravitational waves formed by binary supermassive black holes take months or years to pass Earth and require many years of observations to detect.

"Galaxy mergers are common, and we think there are many galaxies harboring binary supermassive black holes that we should be able to detect," said Joseph Lazio, one of Taylor's co-authors, also based at JPL. "Pulsars will allow us to see these massive objects as they slowly spiral closer together."

Once these gigantic black holes get very close to each other, the gravitational waves are too short to detect using pulsars. Space-based laser interferometers like eLISA, a mission being developed by the European Space Agency with NASA participation, would operate in the frequency band that can detect the signature of merging. The LISA Pathfinder mission, which includes a stabilizing thruster system managed by JPL, is currently testing technologies necessary for the future eLISA mission.

Finding evidence for supermassive black hole binaries has been a challenge for astronomers. The centers of galaxies contain many stars, and even monstrous black holes are quite small—comparable to the size of our solar system. Seeing visible signatures of these binaries amid the glare of the surrounding galaxy has been difficult for astronomers.

Radio astronomers search instead for the gravitational signals from these binaries. In 2007, NANOGrav began observing a set of the fastest-rotating pulsars to try to detect tiny shifts caused by gravitational waves.

Pulsars emit beams of radio waves, some of which sweep across Earth once every rotation. Astronomers detect this as a rapid pulse of radio emission. Most pulsars rotate several times a second. But some, called , rotate hundreds of times faster.

"Millisecond pulsars have extremely predictable arrival times, and our instruments are able to measure them to within a ten-millionth of a second," said Maura McLaughlin, a radio astronomer at West Virginia University in Morgantown and member of the NANOGrav team. "Because of that, we can use them to detect incredibly small shifts in Earth's position."

But astrophysicists at JPL and Caltech caution that detecting faint gravitational waves would likely require more than a few pulsars. "We're like a spider at the center of a web," said Michele Vallisneri, another member of the JPL/Caltech research group. "The more strands we have in our web of pulsars, the more likely we are to sense when a gravitational wave passes by."

Vallisneri said accomplishing this feat will require international collaboration. "NANOGrav is currently monitoring 54 pulsars, but we can only see some of the southern hemisphere. We will need to work closely with our colleagues in Europe and Australia in order to get the all-sky coverage this search requires."

The feasibility of this approach was recently called into question when a group of Australian pulsar researchers reported that they were unable to detect such signals when analyzing a set of pulsars with the most precise timing measurements. After studying this result, the NANOGrav team determined that the reported non-detection was not a surprise, and resulted from the combination of optimistic gravitational wave models and analysis of too few pulsars. Their one-page response was released recently via the arXiv electronic print service.

Despite the technical challenges, Taylor is confident their team is on the right track. "Gravitational waves are washing over Earth all the time," Taylor said. "Given the number of pulsars being observed by NANOGrav and other international teams, we expect to have clear and convincing evidence of low-frequency gravitational waves within the next decade."

NANOGrav is a collaboration of over 60 scientists at more than a dozen institutions in the United States and Canada. The group uses radio timing observations acquired at NRAO's Green Bank Telescope in West Virginia and at Arecibo Radio Observatory in Puerto Rico to search for ripples in the fabric of spacetime. In 2015, NANOGrav was awarded $14.5 million by the National Science Foundation to create and operate a Physics Frontiers Center.

"With the recent detection of by LIGO, the outstanding work of the NANOGrav collaboration is particularly relevant and timely," said Pedro Marronetti, National Science Foundation program director for gravitational wave research. "This NSF-funded Physics Frontier Center is poised to complement LIGO observations, extending the window of to very low frequencies."

Explore further: Black holes don't make a big splash

More information: "Are We There Yet? Time to Detection of Nanohertz Gravitational Waves Based on Pulsar-Timing Array Limits," S. R. Taylor et al., 2016 Mar. 1, Astrophysical Journal Letters. iopscience.iop.org/article/10.3847/2041-8205/819/1/L6, preprint: arxiv.org/abs/1511.05564

"Interpreting the Recent Upper Limit on the Gravitational Wave Background from the Parkes Pulsar Timing Array," The NANOGrav Collaboration, 2016. preprint: arxiv.org/abs/1602.06301

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6 comments

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Psilly_T
5 / 5 (2) Feb 25, 2016
Sounds like a really cool concept. WE probably need a BUTT LOAD of pulsars tracked tho to make this thing sensitive. I could see how a grav wave "might" hit one pulsar and none of the others at the time and it might be hard to confirm that one such pulsar is equating to a grav wave but i'm no astrophysicist COOLBEANs
Captain Stumpy
2 / 5 (4) Feb 25, 2016
luckily for everyone and the future of all physics and science, we have bschott, the experienced one, to help them with this
http://phys.org/n...ina.html

in other places (edited by me)
...I believe they [mainstream scientists-TCS] are not [correct-TCS]. The difference between us is that I apply actual physics to the topic we are debating...Because of my experience I know [topic specific point deleted- TCS] ...you don't.
of course, i suggest the following:
EITHER:
1- research scientists are all incompetent
2- research scientists are all in a conspiracy to deceive you
3- research scientists know something you don't
potholer54
https://www.youtu...dYvz0VwQ

Whydening Gyre
5 / 5 (3) Feb 25, 2016
Sounds like a really cool concept. WE probably need a BUTT LOAD of pulsars tracked tho to make this thing sensitive. I could see how a grav wave "might" hit one pulsar and none of the others at the time and it might be hard to confirm that one such pulsar is equating to a grav wave but i'm no astrophysicist COOLBEANs

I think they are saying the waves affect EARTH's position not the pulsars...
Regardless, it IS cool. We need don't need a HUGE butt-load, but - I cannot lie here - we do need a bigger butt sensing fingerprint (meaning - more in the southern hemi) included in the network.
Old_C_Code
3 / 5 (2) Feb 25, 2016
It's not even good science fiction.
Psilly_T
1 / 5 (1) Feb 25, 2016
I think they are saying the waves affect EARTH's position not the pulsars...
Regardless, it IS cool. We need don't need a HUGE butt-load, but - I cannot lie here - we do need a bigger butt sensing fingerprint (meaning - more in the southern hemi) included in the network.

I c
wduckss
1 / 5 (1) Feb 26, 2016
It is obvious that in the end there will be a "Theory of Zadar" (2004) and tie the waves of rotation of the body. First they were "two black holes" now only pulsar ...

"Rotation of these bodies which is supported from inside creates bodie electro-magnetic powers, that are adequate to size of body, the strong repulsive waves htat are well-defined when the rotation is greater."

http://www.svemir...dar.html page 5.

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