As each of these theories predicts different initial masses for the seeds of
supermassive black hole seeds, the collisions would produce different gravitational wave signals.
Not exact matches
And starting with
seeds in this range alleviates the timing problem for the production of the
supermassive black holes that power the brightest, most distant quasars.
If
black hole seeds come from stars, the process should have given every dwarf galaxy its own
supermassive black hole.
«By combining the detection of gravitational waves with simulations we could ultimately work out when and how the first
seeds of
supermassive black holes formed.»
It may have even provided the
seeds for the
supermassive black holes that seem to anchor all of the big galaxies.
And earlier this year, astronomers showed that the early, distant universe is missing the glow of x-ray light that would be expected from a multitude of small
black holes — another sign favoring the sudden birth of big
seeds that go on to be
supermassive black holes.
Simulations show that a small
black hole seed will never grow fast enough to become
supermassive before the universe is a billion years old.
Two blobs spotted in the distant, ancient universe may be the
seeds of the
supermassive black holes that now dominate the core of every galaxy.
Astronomers have previously suggested that these so - called primordial
black holes could account for all or some of the universe's mysterious dark matter and that they might have
seeded the formation of
supermassive black holes that exist at the centers of galaxies.
If the gas cloud named CO -0.40-0.22, located only 200 light - years away from the center of the Milky Way, does contain an intermediate
black hole, it would provide scientists an opportunity to test the theory that
supermassive black holes evolve from these lower - mass
seeds.
One explanation for the existence of
supermassive black holes in the early universe postulates that the first
black holes were «
seeds» that grew into much larger
black holes by gravitationally attracting and then swallowing matter.
The fact that globular clusters have these small
black holes implies that they are excellent candidates to act as the
seeds for the
supermassive black holes that lurk in the centers of nearly all galaxies.
Such direct - collapse
black holes, weighing 100,000 to 1 million suns, could then act as «
seeds» for
supermassive black holes weighing 1 million to 1 billion suns.