If astronomers are right, the next generation of gravitational wave detectors are going to be very busy.
According to a new survey of all the matter in the universe,
the cosmos is teeming with black holes. And lots of black holes mean
lots of black hole mergers -- the cosmic collisions that generate
gravitational waves.
The new model of the universe's matter was created by a team
of scientists from Europe and the United States. Researchers say it's
the most complete model yet compiled. Its credibility is bolstered by
the fact that it predicted the collision that produced the space-time
shock waves recently measured by LIGO, the Laser Interferometer
Gravitational-wave Observatory.
The types of binary black holes that produced the waves
detected by LIGO aren't like most black holes. They're especially
massive, formed from ancient stars that burn a purer form of hydrogen.
The stars that birthed these black holes upon their deaths were, at
their peak, 40 to 60 times more massive than our sun.
While such massive pairs of black holes aren't common in the
modern universe, there are plenty in some distant regions of the
universe.
The new model --
detailed in the journal Nature
-- has yielded a number of insights into the likely nature of these
supermassive black holes. Simulations suggest their spin rates are
constant and their orbits remain on a single plane. The kickback
produced by their wave-inducing collisions isn't enough to augment their
positioning, but it is large enough to influence the axes of smaller
black holes.
Researchers say their model is already being used by several
other gravitational wave research projects, and will help astronomers
better anticipate and analyze the next black hole collision -- of which
the model suggests there will be several.
"LIGO is not going to see 1,000 black holes like these each
year, but many of them will be even better and more exciting because we
will have a better instrument -- better glasses to view them with and
better techniques," O'Shaughnessy said.
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