The
coalescence1 of two black holes -- a very violent and exotic event -- is one of the most sought-after observations of modern astronomy. But, as these
mergers3 emit no light of any kind, finding such
elusive4 events has been impossible so far. Colliding black holes do, however, release a phenomenal amount of energy as gravitational waves. The first
observatories5 capable of directly detecting these 'gravity signals' --
ripples6 in the
fabric7 of spacetime first predicted by Albert Einstein 100 years ago -- will begin observing the universe later this year.
When the gravitational waves rolling in from space are detected on Earth for the first time, a team of Northwestern University astrophysicists predicts
astronomers8 will "hear," through these waves, five times more colliding black holes than
previously9 expected. Direct observations of these mergers will open a new window into the universe.
"This information will allow astrophysicists to better understand the nature of black holes and Einstein's theory of gravity," said Frederic A. Rasio, a theoretical astrophysicist and senior author of the study. "Our study indicates the observatories will detect more of these energetic events than previously thought, which is exciting."
Rasio is the Joseph Cummings Professor in the department of physics and astronomy in Northwestern's Weinberg College of Arts and Sciences.
Rasio's team,
utilizing10 observations from our own
galaxy11, report in a new modeling study two significant findings about black holes:
Globular clusters (spherical collections of up to a million
densely13 packed stars found in galactic haloes) could be factories of
binary14 black holes (two black holes in close orbit around each other); and
The sensitive new observatories potentially could detect 100
merging15 binary black holes per year forged in the cores of these
dense12 star clusters. (A burst of gravitational waves is emitted whenever two black holes
merge2.) This number is more than five times what previous studies predicted.
The study has been accepted for publication by the journal Physical Review Letters and is scheduled to be published today (July 29).