“Any external influence on a pulsar, such as the gravitational pull of a massive object, would introduce anomalies in this steady arrival of pulses, which can be measured and modeled,” said Slavko Bogdanov, a research scientist at the Columbia Astrophysics Laboratory who was a co-author on the study. “In addition, when the pulses travel near a very massive object, they may be deflected and experience time delays due to the warping of space-time, as predicted by Einstein's General Theory of Relativity.”
Since Sagittarius A*, the central black hole in our Galaxy, has a mass about 4 million times the mass of our Sun, it exerts a strong influence on its surroundings.
Given the potential implications of this discovery, analysis of extensive follow-up observations is underway.
To maximize community impact, Breakthrough Listen is releasing the observations publicly, allowing researchers worldwide to pursue independent analyses and complementary science cases.
“We’re looking forward to what follow-up observations might reveal about this pulsar candidate,” Perez said. If confirmed, it could help us better understand both our own Galaxy, and General Relativity as a whole.”
Read more on Breakthrough Initiative’s website.