by Adrian Cho
June 16, 2016

from Sci-Hub Website






Second gravitational-wave detection

augurs bumper crop of sightings


The biggest discovery in science this year - the observation of ripples in space-time called gravitational waves - was no fluke.


For a second time, physicists working with the two massive detectors in the Laser Interferometer Gravitational-Wave Observatory (LIGO) have detected a pulse of such waves, the LIGO team reported on 15 June at a meeting of the American Astronomical Society in San Diego, California.


Once again the waves emanated from the merger of two black holes, the ultra-intense gravitational fields left behind when massive stars collapse into infinitesimal points.


The new observation suggests that after fine-tuning, LIGO will spot dozens or even hundreds of the otherwise undetectable events each year.

"It's very reassuring," says Gabriela Gonzalez, a physicist at Louisiana State University, Baton Rouge, and chair of the 1000-member LIGO Scientific Collaboration.


"You need another one to be completely convinced and this is it."

Cole Miller, an astrophysicist at the University of Maryland, College Park, who is not a member of the collaboration, says that the new find shows that LIGO,

"is genuinely a new window on the universe."

Astrophysicists' catalog of stellar-mass black holes, he says,

"is going to be overwhelmingly increased by LIGO."

The new observation came at 3:38.53 Coordinated Universal Time on 26 December 2015 - late on Christmas day at LIGO's detectors in Livingston, Louisiana, and Hanford, Washington.


As in the first event, the detectors sensed an oscillating stretching of space-time, the signal, according to Einstein's general theory of relativity, of massive objects in violent motion.


Computer modeling indicated that its source was two black holes spiraling together about 1.4 billion light-years away. (LIGO researchers had seen a weaker signal on 12 October 2015 that may be a third black hole merger.)

The gravitational waves that LIGO has detected originated in the southern sky.

The purple and yellow lines define the likely signal source regions.

The first signal LIGO spied, recorded in September 2015 and unveiled to the world in February (Science, 12 February, p. 645), emanated from surprisingly heavy black holes, with masses 36 and 29 times that of the sun.


It lasted only 0.2 seconds, and physicists glimpsed only the last 10 cycles of the black holes' spiraling motion before their collision.


The December 2015 sighting involved smaller black holes, 14 and 7.5 times as heavy as the sun. Physicists witnessed 55 cycles of the death spiral, a full second.

The first observation remains a riddle. Those two black holes were twice as massive as the relatively nearby stellar-mass black holes identified from the x-rays emitted by hot gas swirling into them.


Astrophysicists don't know how such jumbo black holes formed.


The black holes in the new event,

"are much more garden variety," says Sebastian Heinz, an astrophysicist at the University of Wisconsin, Madison.

Nevertheless, the latest event yields new insights.


For example, physicists determined that one of the black holes was spinning frenetically, at roughly 20% of the maximum spin rate allowed by general relativity.


And because the new event includes many more cycles, it tests predictions of general relativity somewhat more stringently than the first event, Gabriela Gonzalez says. (Einstein's theory passes the test.)

Most important, the second observation shows that going forward, LIGO should reap a vast harvest of black hole mergers.


Rebuilt from 2010 to 2015, the new LIGO detectors have not yet reached their design sensitivity.



On 26 December 2015, LIGO detected gravitational waves

from two black holes spiraling together.


If they do, they should see as many as one black hole merger per day, estimates Stephen Fairhurst, a gravitational-wave astrophysicist and LIGO team member at Cardiff University in the United Kingdom.


The resulting sample should lay bare the mysterious evolution of black hole binaries, he says, showing whether they start out as pairs of stars that turn into black holes or as black holes that form independently and ultimately find each other.

Reaching the design sensitivity - a factor of 2.5 better than today's - is a challenge, as the instruments currently suffer from a "mystery noise" at low frequencies.


David Reitze, LIGO's executive director at the California Institute of Technology in Pasadena, says he's cautiously optimistic that physicists can eliminate the noise and reach design sensitivity by 2019.

"I won't say with 100% confidence that we will get there, but I won't say that we won't either," he says.

Physicists hope LIGO will eventually detect waves from other kinds of cosmic collisions.


Mergers involving neutron stars, for example, would plumb the mysterious physics of these objects, which are essentially gigantic atomic nuclei with masses between 1.5 and three times that of the sun.


LIGO physicists are combing their data for such signals, but finding them is a long shot at the present sensitivity, Gonzalez says.

LIGO's next big splash will likely come in 2017.


The detectors, now restarting after tune-ups, are expected to begin a second data run this fall. They should also be joined by the revamped VIRGO detector, an interferometer near Pisa, Italy, that will help pinpoint sources in the sky and measure their distances.


LIGO may well have more surprises in store, Sebastian Heinz says:

 "There's always that great possibility of finding something unexpected."