Lightest Known Blackhole, Or Largest Known Neutron Star?

I tell ya, after years and years of searching for gravitational waves, and then finally discovering it several years ago, the LIGO-Virgo gravitational waves detector has become an amazing astronomical/astrophysical observatory, making one amazing discovery after another. The existence of such gravitational waves are no longer in doubt that they are now being used as a means to detect other astronomical events.

This is one such case where it appears that a 2.6 solar-mass unknown object collided with a 23 solar-mass blackhole.[1] If this 2.6 solar-mass object is a blackhole, it will be the lightest known blackhole. If it is a neutron star, it will be the heaviest known neutron star. Both scenario will require a reworking of current theories, because a blackhole that light, or a neutron star that heavy, was thought to be unlikely.

Neutron stars and stellar black holes are the final stages of evolution for large stars – with black holes being more massive than neutron stars. In theory, the maximum mass of a neutron star is about 2.1 solar masses. However, there is some indirect evidence that more massive neutron stars could exist. There is little evidence for the existence of black holes smaller than about 5 solar masses, leading to a mass gap in our observations of these compact objects.

What is intriguing about the August 2019 merger – dubbed GW190814 – is the mass of the smaller object, which appears to fall within this gap. “Whether any objects exist in the mass gap has been an ongoing mystery in astrophysics for decades,” says Charlie Hoy of the UK’s Cardiff University, who played a key role in analysing data from the detection and writing the paper that describes the observation, which has been published in The Astrophysical Journal Letters. “What we still don’t know is whether this object is the heaviest known neutron star or the lightest known black hole, but we do know that either way it breaks a record.”

The actual paper is available to be read for free here since it is an open access article.

Like I had said to the students in my astronomy classes, this is going to go down as the golden age of astronomy. Since the beginning of human history, we only had light as our only detector of the heavens. Now, we have not only neutrinos and high-energy cosmic rays, but also gravitational waves as our means to look at the heavens. We have three different and separate ways to look at our sky!

Zz.

[1] R. Abbott et al., The Astrophysical Journal Letters,896:L44(20pp), 2020.