Cosmic Pac-Man: Astronomers have picked up the first unmistakable gravitational wave signals from the collision of a neutron star with a black hole. LIGO and Virgo detected two such events in January 2020. The smaller neutron star may have been swallowed by the black hole whole and without an accompanying burst of radiation. Evidence for such mixed collisions opens the opportunity to learn more about the origin, evolution and end of these unequal pairs.
Since the first detection of gravitational waves in 2016, astronomers have recorded more than 50 cosmic collisions with detectors LIGO and Virgo. Usually two stellar black holes are merging, and in a few cases there are two neutron stars. Two partner mergers with highly unequal audiences are also included.
But what was missing so far was clear evidence of a mixed binary – a neutron star colliding with a black hole. Although there was a potential candidate in April 2019, the data situation was too poor to obtain clear evidence. Another event in June 2020 is puzzling because the second partner was very easy for a black hole, but a little heavy for a neutron star.
Mixed collisions in a row
Now, for the first time, astronomers have detected clear signals of a neutron star colliding with a black hole. In January 2020, LIGO detectors in the US and Virgo detectors in Italy recorded gravitational waves from this mixed duo twice in a row. “Gravity waves alone do not tell us the structure of the lightest object, but we can determine its maximum mass,” explains Bhooshan Gadre of the Max Planck Institute for Gravitational Physics in Potsdam.
These analyzes show that the smaller partner in both collisions cannot be a black hole, but rather a neutron star due to its low mass. In the GW200105 event on January 5, 2020, a black hole of mass 8.9 solar masses and a neutron star of mass 1.9 solar masses collided. The energy of this collision released gravitational waves that reached Earth about 900 million years later.
The second event was recorded on January 15th. GW200115 comes from a black hole of 5.7 solar masses and a neutron star of mass 1.5 solar masses, which collided about a billion light-years away.
Is there any associated radiation?
Since the gravitational waves of this second collision reached both the LIGO and Virgo detectors with good quality, the astronomers were at least able to roughly determine the likely location of the event. Using triangulation, they narrowed its position to an area of ​​sky corresponding to the size of about 3,000 full moons.
This approximate location determination allowed other teams to use telescopes to look for the electromagnetic effects of the collision. These radiation outbursts are usually absent when two black holes collide, but were discovered after neutron stars merge. However, it is unclear whether they will also be released in a mixed collision. At least with GW200115 astronomers haven’t found anything.
Swallow whole – like Pac-Man
Possible cause: The black hole may have swallowed the neutron star as a whole – leaving no radioactive debris behind. “These weren’t events where black holes nibbled neutron stars first and dumped their remnants like a cookie monster,” explains LIGO spokesman Patrick Brady of the University of Wisconsin-Milwaukee. This ejection would have generated radiation, but we don’t think that happened in those cases.
“In these collisions, two dense, dense objects just don’t come together and merge. It’s more like Pac-Man: the black hole completely devours its partner neutron star,” adds co-author Susan Scott of the Australian National University. These are really amazing events and we’ve been waiting a long time to witness them.”
Many unanswered questions
Events GW200105 and GW200115 clearly show that these asymmetric collisions exist in the universe – and that they can be detected by gravitational waves. At the same time, these collisions open up new opportunities for astronomers to investigate the origin, evolution, and end of these mixed pairs in more detail. “There’s a lot we don’t know about neutron stars and black holes – how small or large they can get, how fast they rotate, and how they pair up,” explains Maya Fischbach of Northwestern University in Evanston.
The LIGO and Virgo teams are currently working on improving their detectors in order to achieve higher sensitivity for the next round of observation in 2022. As a third member of the group, the Japanese KAGRA detector has also been in operation since 2020. (The Astrophysical Journal Letters, doi: 10.3847/2041-8213/c082e)
Cowell: University of Wisconsin-Milwaukee, Northwestern University, CNRS, Australian National University