The group in which he works is involved in the instrumental development for the LISA PathFinder mission (ESA), a technology precursor mission for a future space - based gravitational - wave observatory, LISA, which will detect the gravitational radiation from low frequency sources like
massive black hole mergers, inspiraling stellar compact objects into massive black holes, and galactic binaries.
A new study published in Nature presents one of the most complete models of matter in the universe and predicts hundreds of
massive black hole mergers each year observable with the second generation of gravitational wave...
A new study published in Nature presents one of the most complete models of matter in the universe and predicts hundreds of
massive black hole mergers each year observable with the second generation of gravitational wave detectors.
Not exact matches
For a fourth time, physicists have spotted gravitational waves — ripples in space itself — set off by the
merger of two
massive black holes.
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.
Physicists concluded that the first detected gravitational waves, in September 2015, were produced during the final fraction of a second of the
merger of two
black holes to produce a single, more
massive spinning
black hole.
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.
The detection of a supermassive
black hole merger would offer new insights into how
massive galaxies and
black holes evolve, 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.
However, Marc Kamionkowski, a theoretical physicist at Johns Hopkins University in Baltimore, Maryland, says the signal from the
merger of more -
massive black holes should be stronger and detectable from a greater distance.
But only some of the most
massive astrophysical events, such
mergers of
black holes and neutron stars, can produce gravitational waves strong enough to be detected on earth.
The existence of
black holes tens of times more
massive than our Sun was confirmed recently by the observation of gravitational waves, produced by the
merger of pairs of
massive black holes, with the LIGO interferometer.
The thought was that when many galaxies are close together, a
merger, two galaxies colliding and melding together, would create instabilities and cause gas to fall into the super
massive black hole in one of the galaxies, creating a quasar.
In a new study, the scientists show their theoretical predictions last year were correct: The historic
merger of two
massive black holes detected Sept. 14, 2015, could easily have been formed through dynamic interactions in the star - dense core of an old globular cluster.
GRBs are jetted explosions triggered either by the collapse of a
massive star or by the
merger of a neutron star with another neutron star or a
black hole.
Physicists working with the Laser Interferometer Gravitational - Wave Observatory have spotted a third
merger of
black holes, the ultraintense gravitational fields left behind when
massive stars collapse.
LISA is tuned to detect lower frequencies and longer wavelengths produced by
mergers between
black holes millions of times more
massive than the sun.
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.