The Advanced Network of Ligo, Virgo and Kagra or LVK gravitational waves detected this gravitational wave during the fourth round of observation of these three laser ierference, according to the . These very sensitive tools are in the US, Italy and Japan.
The eve was named the GW۲۱۳۱۲۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۱۳۹۰ with two maternal black holes iegrated with 1 and 2 times the sun. The two black holes were so huge that the time of merger created a black hole of 5 times the mass of the sun. Earlier, the record was the largest black hole iegration in the year 6, with a volume of 5 times the sun.
“This is the largest binary black hole observed through gravitational waves and reflects a true challenge in our perception of the way black hole formation,” says According to the standard model of the curre star evolution, it is not possible to have black holes with this greatness. But one of the possibility of the eve is that the two black holes in the binary system are formed through the iegration of smaller black holes.
The only ieresting thing about this eve is not the iegration of their huge volume. The signal of the eve appears to indicate that at least one of the black holes of the origin was rotated before the merger.
“The black holes appear to be rotating at a very fast and close to the permissible limit of Einstein’s general relativity,” says Charlie Hui, a member of the LVK team. This makes it difficult to model and ierpret the signal. For this reason, this is a great study to advance the developme of our theoretical tools.
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