The black hole named Cygnus X-1 formed when a large star caved in. This black hole pulls matter from the blue star beside it.
Physicists have described how observations of gravitational waves limit the possible explanations for the formation of black holes outside of our galaxy; either they are spinning more slowly than black holes in our own galaxy or they spin rapidly but are ‘tumbled around’ with spins randomly oriented to their orbit.
In our own galaxy we have been able to electromagnetically observe black holes orbited by stars and map their behaviour — notably their rapid spinning.
Gravitational waves carry information about the dramatic origins of black that cannot otherwise be obtained. Physicists concluded that the first detected gravitational waves, in September 2015, were produced during the final fraction of a second of the merger of two black holes to produce a single, more massive spinning black hole. Collisions of two black holes had been predicted, but never observed.
As such, gravitational waves present the best and only way to get a deep look at the population of stellar-mass binary black holes beyond our galaxy. This paper states that the black holes seen via gravitational waves are different to those previously seen in our galaxy in one of two possible ways.
The first possibility is that the black holes are spinning slowly. If that is the case it suggests that something different is happening to the stars that form these black holes than those observed in our galaxy.
The second possibility is that the black holes are spinning rapidly, much like those in our galaxy, but have been ‘tumbled’ during formation and are therefore no longer aligned with orbit. If this is the case, it would mean that the black holes are living in a dense environment — most likely within star clusters. That would make for a considerably more dynamic formation.
There is, however, also the chance that both possibilities are true — that there are instances of black holes spinning slowly in the field and instances of black holes spinning rapidly in a dense environment.
Dr Will Farr, from the School of Physics and Astronomy at the University of Birmingham, explained, “By presenting these two explanations for the observed behaviour, and ruling out other scenarios, we are providing those who study and try to explain the formation of black holes a target to hit. In our field, knowing the question to ask is almost as important as getting the answer itself.”
Professor Ilya Mandel, also from the University of Birmingham, added “We will know which explanation is right within the next few years. This is something that has only been made possible by the LIGO detections of gravitational waves in the last couple of years. This field is in its infancy; I’m confident that in the near future we will look back on these first few detections and rudimentary models with nostalgia and a much better understanding of how these exotic binary systems form.”
The team was led by researchers from the University of Birmingham in the UK alongside the University of Maryland, University of Chicago and Kavli Institute for Theoretical Physics in the US.
Story Source:Materials provided by University of Birmingham Original written by Whitney Clavin.Note: Content may be edited for style and length.
Will M. Farr, Simon Stevenson, M. Coleman Miller, Ilya Mandel, Ben Farr, Alberto Vecchio. Distinguishing spin-aligned and isotropic black hole populations with gravitational waves. Nature, 2017; 548 (7667): 426 DOI: 10.1038/nature23453