Researchers are using pulsars to detect low-frequency gravitational waves from supermassive black hole mergers, and recent findings show promising timing variations, though more data is needed for confirmation.
Astronomers have been using gravitational waves to detect merging black holes for years now, but may have to rely on pulsars – rapidly spinning neutron stars – to observe the mergers of supermassive black holes.
When black holes merge, they release enormous amounts of energy in the form of ripples in the fabric of spacetime. These ripples are constantly washing over the Earth, and it’s only through the use of extremely – and I mean extremely – sensitive detectors that we can spot them.
Limitations of Current Gravitational Wave Detectors
Right now, our gravitational wave detectors are only sensitive to brief, intense pulses, signaling the mergers of relatively small black holes and neutron stars. When giant black holes merge, however, the process takes so long – and produces gravitational waves of such low frequency – that we can’t spot it in the data.
A recent study led by Dr. Boris Goncharov and Prof Ryan Shannon – both researchers from the ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav) in Australia – are trying a different tactic: instead of observing gravitational waves directly, they’re hoping that pulsars do the hard work for us.
Pulsars are a special kind of neutron star that rapidly rotates, sending a splash of radiation across the Earth at precisely timed intervals. Their work uses the Parkes Pulsar Timing Array to monitor as many pulsars as possible. As the gravitational waves from a supermassive black hole merger wiggle through the galaxy, they will cause variations in the timing of the pulses.
Early Findings from the Parkes Pulsar Timing Array
Recently, the team announced that they did indeed observe variations in the timings of pulsar flashes, and that the variations are consistent with expectations from gravitational waves. However, they haven’t observed enough pulsars yet to determine if it’s truly a global signal, or just an artifact of their observations.
According to Dr. Goncharov: “To find out if the observed ‘common’ drift has a gravitational wave origin, or if the gravitational-wave signal is deeper in the noise, we must continue working with new data from a growing number of pulsar timing arrays across the world.”
Adapted from an article originally published on Universe Today.
For more on this research, see Pulsar Timing Array Explores Mystery Gravitational Waves From Supermassive Black Holes.
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