Bumper crop of black holes in new gravitational wave paper

The international research team responsible for detecting gravitational waves has announced 39 new gravitational wave events, bringing the total number of confirmed detections to 50.

gravitational waves

Only a few years ago, scientists the world over celebrated as the first-ever gravitational waves were detected – confirming a long-held scientific theory and opening up an entirely new field of research.

Today, the Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo collaborations, which include many researchers from the UK, have published a series of papers that record events including the mergers of binary black holes, binary neutron stars and, possibly, neutron star-black holes.

These events were recorded during the first six months of the LIGO and Virgo detectors’ third observing run, between 1 April and 1 October 2019.

Journey across the universe

Professor Alberto Vecchio, director of the Institute for Gravitational Wave Astronomy at the University of Birmingham, says: "I remember when, over 20 years ago I started to devote most of my time to gravitational wave science, many of my former PhD colleagues thought I was mad. I would spend my scientific career just staring at terabytes of noise.

"I am so glad I was foolish enough not to pay much attention to their remarks. Now it’s surprise after surprise in an exhilarating journey across the universe, and this is just the very beginning."

UK scientists have designed and built instrumentation for the LIGO detectors, which are based in the United States, and have contributed to the analysis and interpretation of the data collected throughout the three observing runs.

The UK’s contribution to the collaborations is funded by the Science and Technology Facilities Council.

With this new, expanded catalogue of detections, scientists are provided with a wealth of black hole data to rigorously test Einstein’s General Theory of Relativity and give new insight into how black holes and neutron stars come into being.

Dr Andrew Williamson from the University of Portsmouth’s Institute of Cosmology and Gravitation, said: "This new catalogue of discoveries includes 39 new gravitational wave events observed between 1 April and 1 October 2019. That’s more than one discovery per week.

"Most of these were produced by merging pairs of black holes, but it also includes the second ever discovery of a colliding pair of neutron stars, and possibly the first discovery of a black hole and neutron star pair merging.

"Neutron stars are the extremely dense remains of dead stars, weighing more than our Sun but crushed into something the size of a city, less than 15 miles across.

"Combined with 11 discoveries made before 2019, we have now discovered 50 gravitational wave events, with many more surely to come. We now have enough events that we can really begin to answer questions like: ‘just how common are merging pairs of black holes?’ and ‘what does the population of black holes look like?’"

The future of black hole science

The new observations include binary black holes ranging from approximately five times the mass of the Sun at one end of the scale, all the way up to 85 times the mass of the Sun. At the top of this scale, the biggest black holes are much more massive than previously thought to exist.

In another observation, a black hole was seen to merge with an object 2.6 times the mass of the Sun. If that object was a black hole, it would have been lighter than thought possible. Alternatively, it may have been the biggest neutron star ever observed.

Now, astrophysicists will look to find out how and where in the Universe the systems found by LIGO and Virgo were formed.

Professor Sheila Rowan, director of the University of Glasgow’s Institute for Gravitational Research, said: "It’s amazing to think that, five years on from the first detection of gravitational waves, we’re now in a position where we can publish details of 39 new detections at once.

"That first detection was the culmination of decades of hard work by a remarkable international collaboration. All the detections we’ve made since then are the result of even more hard work to upgrade the detectors, improve their sensitivity, and keep them working for longer during each observing run."

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