Thursday, July 30, 2015

Dense Star Clusters Shown as Binary Black Hole Factories

The coalescence of two black holes -- a very violent and exotic event -- is one of the most sought-after observations of modern astronomy. But, as these mergers emit no light of any kind, finding such elusive events has been impossible so far.

Colliding black holes do, however, release a phenomenal amount of energy as gravitational waves. The first observatories capable of directly detecting these 'gravity signals' -- ripples in the fabric of spacetime first predicted by Albert Einstein 100 years ago -- will begin observing the universe later this year.

An artist's conception of a black hole binary in a heart of a quasar, with the data showing the periodic variability superposed.
An artist's conception of a black hole binary in a heart of a quasar
Credits: Santiago Lombeyda, Center for Data-Driven Discovery, Caltech

When the gravitational waves rolling in from space are detected on Earth for the first time, a team of Northwestern University astrophysicists predicts astronomers will "hear," through these waves, five times more colliding black holes than previously 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, utilizing observations from our own galaxy, report in a new modeling study two significant findings about black holes:

Globular clusters (spherical collections of up to a million densely packed stars found in galactic haloes) could be factories of binary black holes (two black holes in close orbit around each other); and

Supercomputer models of merging black holes reveal properties that are
crucial to understanding future detections of gravitational waves. This
movie follows two orbiting black holes and their accretion disk during
their final three orbits and ultimate merger. Redder colors correspond
to higher gas densities.
Credit: NASA 

The sensitive new observatories potentially could detect 100 merging binary black holes per year forged in the cores of these dense star clusters. (A burst of gravitational waves is emitted whenever two black holes merge.) 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).

"Gravitational waves will let us hear the universe for the first time, through the ripples made by astronomical events in spacetime," said Carl L. Rodriguez, lead author of the paper. He is a Ph.D. student in Rasio's research group.

"Up until now, all of our observations have been from telescopes, literally looking out at the universe. Detecting gravitational waves will change that. And the cool part is we can hear things we could never see, such as binary black hole mergers, the subject of our study," he said.

Rodriguez and colleagues used detailed computer models to demonstrate how a globular cluster acts as a dominant source of binary black holes, producing hundreds of black hole mergers over a cluster's 12-billion-year lifetime.

By comparing the models to recent observations of clusters in the Milky Way galaxy and beyond, the results show that the next generation of gravitational-wave observatories could see more than 100 binary black hole mergers per year.

Frame from a simulation of the merger of two black holes and the resulting emission of gravitational radiation (colored fields). The outer red sheets correspond directly to the outgoing gravitational radiation that one day may be detected by gravitational-wave observatories.
Credit: NASA/C. Henze 

Advanced LIGO (Laser Interferometer Gravitational-Wave Observatory) is one of the new gravitational-wave observatories. Slated to begin operation later this year, Advanced LIGO is a large-scale physics experiment designed to directly detect gravitational waves of cosmic origin. Laser interferometers detect gravitational waves from the minute oscillations of suspended mirrors set into motion as the waves pass through the Earth.

Rasio and Rodriguez are members of Northwestern's Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA).

For the study, the research team used a parallel computing code for modeling star clusters developed through a CIERA-supported interdisciplinary collaboration between Northwestern's physics and astronomy department and electrical engineering and computer science department.




Contacts and sources:
Megan Fellman
Northwestern University

The title of the paper is "Binary Black Hole Mergers From Globular Clusters: Implications for Advanced LIGO."

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