As an explanation for the first quasars, each of these pathways for the formation
of black hole seeds has the same problem: the seeds would have to grow extraordinarily quickly within the first billion years of cosmic history to create the earliest quasars.
Building on the work of several other research groups, my collaborator Giuseppe Lodato and I published a set of papers in 2006 and 2007 in which we proposed a novel mechanism that could have produced more
massive black hole seeds from the get - go.
Observations suggest that these black holes are formed either due to the merger of smaller intermediate - size «seeds,» or a supermassive
black hole seed from a giant star — about 100 times the sun's mass — that ultimately forms into a black hole after it runs out of fuel and collapses.
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.
But Bromm is more optimistic, especially if such direct -
collapse black hole seeds also formed slightly later in the history of the universe.
In effect, if the first quasars grew from Population
III black hole seeds, they would have had to eat faster than the Eddington rate.
Traditional black hole seeds, on the other hand, which derive from dead stars, are likely to be too faint for the JWST or other telescopes to see.
If black hole seeds come from stars, the process should have given every dwarf galaxy its own supermassive black hole.
Huge gas clouds left by the big bang might have quickly shrunk under their own gravity and, instead of splintering into many stars, condensed
into black hole seeds 10 thousand to 100 thousand times heavier than the sun.
Simulations show that a
small black hole seed will never grow fast enough to become supermassive before the universe is a billion years old.
In the May 2018 Monthly Notices of the Royal Astronomical Society, Schleicher and colleagues show that such clusters also could create
massive black hole seeds, as newly formed stars accrete gas left over in the cluster.
«In this way, a massive direct
collapse black hole seed can form in the second galaxy, which can evolve rather quickly to a billion solar mass black hole by the time they are observed in the universe,» he said in the statement.
Instead
these black hole seeds would have formed directly from gas.
To grow to 109 solar masses,
a black hole seed of 10 solar masses would have to gobble stars and gas unimpeded at the Eddington rate for a billion years.
A merger would give
the black hole seed a copious new source of gas to eat, so the black hole should start growing rapidly.
«The massive
black hole seeds are the ones that won the birth lottery and got the best start in life.»