Triple star recipe for supersized stellar-mass black holes

Now envision a typical triple system, where an inner pair of binary stars is orbited by a third star farther out. Once all three of these stars become black holes — provided they are massive enough — you have triple black hole system.

Over time, the two inner black holes merge together, giving birth to a black hole whose mass can easily exceed the lower limit of the mass gap. After another long wait, the combined central black hole will go on to merge with the third black hole farther out in the system, forming an even more massive final product.

But if astronomers only pick up gravitational waves from this second merger, they will remain oblivious to the system’s turbulent, more complicated history. Therefore, the triple-star merging sequence neatly explains why recent LIGO/Virgo detection have picked up collisions between black holes that seem too massive to have formed from individual stars.

Double down on triple star research

Triple stars are still a young field of study. Despite tremendous progress in the last decade, scientists haven’t yet figured out all aspects of their behavior.
How stars and their orbits evolve is heavily dependent their initial masses and orbital arrangement. The number of possible configurations is overwhelming — and it doesn’t help that detailed observations of triples are still sparse.

“We wanted to understand if we can get triples without a strong dynamical interaction that could form black holes in the mass gap,” says Alejandro Vigna-Gómez, an astrophysicist with the Niels Bohr Institute at the University of Copenhagen and lead author of the study. And working under the assumption of a simple interaction, the team identified several scenarios that could realistically lead to a supersized stellar-mass black that’s later involved in another merger.

These scenarios aren’t just untestable hypotheticals, either; they predict characteristic features that astronomers can look for in merger data. “We are searching for LIGO/Virgo mergers with particular mass ratios of the merging black holes and high values of their effective spin,” says Vigna-Gómez.

Indeed, the triple star merger scenario seems to be a favorable model for the merger dubbed GW170729, whose pre-merger black holes weighed in at approximately 51 and 36 solar masses. (However, their model can’t explain the properties of GW190521, the most extreme merger detected so far. This event was spawned by the collision of two black holes weighing roughly 85 and 66 solar masses.)

The proposed triple star model may not be the only — nor the dominant — mechanism for producing high-mass stellar black holes. However, the study does prove the model is a feasible alternative to other possible scenarios, such as a binary system snagging a passing black hole that gets too close. So, the researchers argue, the role triple stars may play in forming extra-large black holes should be taken seriously.

“There is still so much more to explore. We started with simple approximations, and now is the time to add more,” says Toonen.