When you like giant objects Neutron Star and Black Hole Merge or when Supernova If it explodes in a far distance of space, it creates a final product smaller than an object that collides or erupts. The mass they lose is converted to energy according to Einstein’s famous equation E = MC2 Moves in the form of distortions in space. Scientists call these distortions Gravity wavesand they can indirectly detect them by studying how waves interfere with the observation of other distant objects, or directly interfere in facilities such as Laser interferometer gravitational wave astronomy Or ligo.

Scientists working on the Ligo project have discovered that most of the gravitational waves they detect come from the fusion of two black holes. However, these scientists don’t know how these pairs of black holes converge. So far, they have two broad theories about how this happens. The first is when a large star transforms into a black hole, drifting in close proximity due to the complexity of pushing and pulling other nearby objects. These duos are called It was formed dynamically Binary pair. The second is that two giant stars begin their lives in binary pairs before transitioning to a pair of black holes. These duos are called It is formed primitively Binary pair. Scientists cannot use LIGO data to distinguish between these two types of black holes. Can only be detected if integrated. Therefore, there are other ways to know how they merged.

A team of astrophysicists at Cardiff University used a series of computer simulations to test tests that the theory of black hole mergers is likely to reflect the real world. They use the astrophysical collision modeling code PETAR to group or cluster Stars, including black holes pioneers, have evolved over millions of years, and which scenarios have led to the merger of black holes.

The team created 35 model star clusters that vary by size, with a total mass of 1,000,000 times the total mass of the sun’s mass of all constituent stars, how close the stars are, and the percentage of the non-helium-helium-like elements of helium called hydrogen or helium. Metallic. They determined the size of a particular star within these clusters using statistical distributions ranging from 0.08 to 150 times the mass of the sun. Next, we divide the specific variations of cluster size, star density, and metallicity into two model versions. One had no primitive binary pairs, and the other had more than 20 times the sun’s binary companions.

Researchers looked for general trends in how the simulation progressed. They discovered four million years later that the first black hole formed from the largest star was a pair of binary black holes and black holes stars. Simulations using primitively formed pairs showed that binary black holes formed faster around the same time as the first black holes appeared. In simulations without primitively formed pairs, binary pairs still appeared through dynamic processes, but only after millions of years it was at the very heart of a star cluster. In both simulations, the clusters discharged many of the binary black holes on a sufficiently long timescale and quickly integrated.

Final statistical analysis of 35 model star clusters showed that, unless there are large binary stars when formed in star clusters, the majority of black hole mergers come from primitive binary pairs. They also found no clear relationships between how large and dense the star cluster was and the number of dynamic mergers it generated. Dynamic mergers are relatively rare, but we saw how frequently metals in star clusters occurred. They also reported that a small portion of the merged black hole pairs are part of a larger group of three or four black holes!

The team admitted that they rely on a model of binary star evolution, where their outcomes remain uncertain. However, their conclusions argued that many astrophysicists challenged the core assumption that the most detected black holes merged from large, dense clusters of stars. By showing that primitive binaries are the dominant source of mergers, and knowing that most stars form in small clusters, they argued that most ligo detections are likely to come from small star clusters in the distance of the universe.

Post view: 249