A discovery would confirm one of general relativity's most extraordinary predictions and provide an unprecedented glimpse of cataclysmic events such
as black hole mergers.
Not exact matches
That's why it was a surprise when physicists with the Laser Interferometer Gravitational - Wave Observatory (LIGO) announced in February 2016 that they had detected ripples in space from the violent
merger of two
black holes 29 and 36 times
as massive
as our sun.
«We know very well that
black holes can be formed by the collapse of large stars, or
as we have seen recently, the
merger of two neutron stars,» said Savvas Koushiappas, an associate professor of physics at Brown University and coauthor of the study with Avi Loeb from Harvard University.
There, young stars, born during the
merger, will explode
as supernovas, and a quasar — a giant
black hole ignited by the galactic collision — might spew energetic radiation.
All the previous gravitational - wave detections since the first in September 2015 had been the result of two merging
black holes — objects much more massive than a neutron star — which have left only gravitational waves
as fleeting clues of their
merger.
If the new model is correct, then such
black hole mergers may occur
as frequently
as once a year somewhere in the Universe.
As to whether astronomers will detect a supermassive
black hole merger, «it'll be interesting either way,» Mingarelli says.
A
black hole merger in a massive galaxy like M87 would yield detectable gravitational waves for 4 million years, for instance, while a more modest galaxy such
as the Sombrero Galaxy would offer a 160 - million - year window.
Frustratingly for the Virgo team, the steel wires are expected to have the most impact on sensitivity to gravitational waves with lower frequencies than neutron star
mergers, such
as those from the
mergers of
black holes.
In their latest finds, physicists with the Laser Interferometer Gravitational - Wave Observatory spotted the
merger of
black holes spinning in different orientations,
as shown in this artist's conception.
MAKING WAVES The first gravitational wave signal detected by LIGO came from the
merger of two
black holes spiraling inward,
as depicted in this numerical simulation.
The
merger of two
black holes, such
as the one which produced the gravitational waves discovered by the LIGO Observatory, is considered an extremely complex process that can only be simulated by the world's most powerful supercomputers.
Each time a
merger occurred, material from the new galaxy got incorporated into the accretion disk around the
black hole, spinning in the same direction
as the
black hole and eventually contributing to its growth.
One of the most important scientific consequences of detecting a
black -
hole merger would be confirmation that
black holes really do exist — at least
as the perfectly round objects made of pure, empty, warped space - time that are predicted by general relativity.
A
black -
hole merger occurs when two
black holes start to spiral towards each other, radiating energy
as gravitational waves.
If they can reach that goal, then, extrapolating from the current observations, LIGO might eventually spot
as many
as one
black hole merger per day.
And if, García - Bellido says, any
black hole in a LIGO
merger proves to weigh less than our sun, this would be a «smoking gun» for primordial
black holes,
as such relatively minuscule
black holes are thought impossible to form from stars.
Rodriguez and colleagues used 52 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.
Besides
black hole mergers and neutron star smashups, in the future, scientists might also spot waves from an exploding star, known
as a supernova.
As long as the black holes get a just little closer than their final separation in the simulation, they will start giving off gravitational waves — ripples in space - time that carry energy away — which would then guarantee a final merger, he say
As long
as the black holes get a just little closer than their final separation in the simulation, they will start giving off gravitational waves — ripples in space - time that carry energy away — which would then guarantee a final merger, he say
as the
black holes get a just little closer than their final separation in the simulation, they will start giving off gravitational waves — ripples in space - time that carry energy away — which would then guarantee a final
merger, he says.
Gravitational waves are tiny ripples in space and time itself, set off by cosmic cataclysms such
as the
merger of two neutrons stars or
black holes.
Its detectors looked for those ripples in space - time that result from the
merger of two
black holes as shown in this computer simulation.
But Goldstein and Racusin said that LIGO is expected to detect more merging
black holes in the coming years,
as many
as 100 such
mergers per year at the instrument's peak design sensitivity, Goldstein said.
«We were looking for orbiting pairs of supermassive
black holes, with one offset from the center of a galaxy,
as telltale evidence of a previous galaxy
merger.
Any model that presumed a one - time cataclysm, such
as a star's dying flash or the
merger of stars or
black holes, was out.
The first direct detection of gravitational waves occurred in mid-September 2015 (but announced February 11, 2016) with twin LIGO detectors in Hanford, WA and Livingston, LA (both USA) when ripples of spacetime from the last fraction of a second of the
merger of two
black holes with masses 29 and 36 solar masses combined to form a 62 - solar mass
black hole with 3 solar masses of energy radiated away
as gravitational waves in that last fraction of a second.
This illustration shows the
merger of two
black holes and the gravitational waves that ripple outward
as the
black holes spiral toward each other.
So far, only the gravitational waves from
black hole mergers have been detected, but
as the sensitivity of laser interferometers increases, scientists hope to detect collisions between neutron stars, for example.
The increasing amplitude and frequency of the waves during the
merger if converted to audio sound waves would make a sound like a chirp of a bird, so the LIGO scientists refer to it
as the chirp of a
black hole merger.
Subsequently, matter from the debris of the
merger that swirls rapidly around the newly created new
black hole has been modelled
as amplifying the strength of the combined magnetic field left over by the neutron stars after their
merger over the next 11 milliseconds.
Dense star clusters may serve
as breeding grounds for successive generations of
black hole mergers, resulting in gargantuan
holes, generating gravitational waves that researchers hope to detect.
Late time cosmology with LISA probing the cosmic expansion with massive
black hole binary
mergers as standard sirens Nicola Tamanini 2017 March 20, 12:00 IA / U.
Until that moment, gravitational wave detectors had only discerned the
merger of
black holes billions of light - years away, so to measure a weak signal at a comparatively close distance came
as a surprise.
Urry will conclude with the big picture: the evolution of the universe over the last 13 billion years,
as indicated by computer simulations, and future prospects for observing
black hole growth and
mergers across the cosmos.
Figure 2: Several properties of
black -
hole mergers as a function of time.
Black holes in the centers of galaxies could accelerate
mergers between objects and produce more ripples in space - time, also known
as gravitational waves, a new study suggests.
This latest detection originated from a
merger creating a
black hole of 49 solar masses (another «heavy»
black hole like the first one), but the
merger happened over twice
as far away than previous events.