Scientists may soon be able to tease out a faint signal of gravitational waves
from black hole collisions too distant to be detected directly, scientists with LIGO, the Advanced Laser Interferometer Gravitational - Wave Observatory, report in the April...
Not exact matches
Collisions between supermassive
black holes (SN Online: 8/31/15) can be heard
from much farther away, but they send out long, undulating waves to which LIGO is deaf.
Gravitational waves detectable
from Earth are generated by
collisions of massive objects, such as when two
black holes or neutron stars merge.
From simulations run by others, the researchers conclude that the optical and UV bursts likely originated from the collision of stellar debris on the outer perimeter of the black h
From simulations run by others, the researchers conclude that the optical and UV bursts likely originated
from the collision of stellar debris on the outer perimeter of the black h
from the
collision of stellar debris on the outer perimeter of the
black hole.
LIGO, the Laser Interferometer Gravitational Wave Observatory, is a pair of three - mile - long gravitational - wave detectors in Washington and Louisiana that cost $ 365 million and took 11 years to build, and yet they may just barely be able to pick up signals
from the ultraviolent
collisions that give birth to massive
black holes.
And a spacecraft called Lisa Pathfinder launched last December to test technology for a proposed space - based observatory that will be sensitive to longer - wavelength gravitational waves
from supermassive
black hole collisions.
They travel like waves on a pond, spreading outwards
from sources of extreme gravitational disturbance such as the
collision of a star with a
black hole.
Intermediate - mass
black holes are thought to form either
from the merging of several smaller, stellar - mass
black holes, or as a result of a
collision between massive stars in dense clusters.
The faster the
black hole spins, the larger its ergosphere becomes, which allows high - energy
collisions further
from the event horizon.
The objects causing these low - frequency ripples — such as orbiting supermassive
black holes at the centers of distant galaxies — would be different
from the higher frequency ripples, emitted by
collisions of much smaller
black holes, that have so far been detected on Earth.
The two signals that have been produced so far came
from the
collision and merger of two
black holes in some remote part of the universe.
Through these efforts, astronomers are attempting to understand recently discovered phenomena such as the first detections of gravitational waves
from neutron star
collisions and the accompanying electromagnetic fireworks as well as regular stars being engulfed by supermassive
black holes.
Unlike the recently detected waves
from the Big Bang (SN: 4/5/14, p. 6), the waves LIGO picks up will most likely come
from black hole or neutron star
collisions.
Energy released
from the
collisions of particles within the hot core travels to the outer part through conduction, causing pressure that drives much of the gas in the outer region beyond the reach of the
black hole.
An unusual object about 90 million light - years
from Earth might be a supermassive
black hole kicked out of its home galaxy during a
collision with another galaxy, a new study suggests.
The powerful blasts of particles and light energy known as gamma - ray bursts come
from violent cosmic events in deep space, such as stellar explosions and
black hole collisions.
Light
from the
collision should help test Einstein's theory of general relativity, and tell us more about two huge bubbles of hot gas at the centre of the Milky Way that the
black hole may have spawned.
Comparison with the SXS simulations revealed that the signal was
from the
collision of two hefty
black holes 29 and 36 times more massive than the sun and located 1.3 billion light - years
from Earth.
One possibility is that the dust was acquired
from a
collision with a small neighboring galaxy, after the
black hole had already formed.
From just that signal, scientists already knew that this wasn't another
black -
hole collision.
For example, the waves detected by the Laser Interferometer Gravitational - Wave Observatory (LIGO) operated by Caltech and Massachusetts Institute of Technology came
from the
collision and merging of two major
black holes 1.3 billion years ago.
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.
When a
black hole is created
from a supernova
from a massive star or a
collision between neutron stars (or a neutron star with a
black hole), one of a pair of bi-polar jets of gamma rays travelling at near light - speed may be directed at the Earth (more).
In 2005, astronomers announced that GRB 050709 and GRB 050509B may be have created by
collisions involving two neutron stars (more
from Chandra X-Ray Observatory) and ESO), but that the presence of a second flare by GRB 050724 was more likely to have been produced by a neutron star's merger with a
black hole (ESO).
LIGO announces the first discovery of strong gravitational waves
from a
collision of two
black holes
Professor Mavalvala worked with researchers at the US - based underground detectors Laser Interferometer Gravitational - wave Observatory (LIGO) Laboratory to build sophisticated sensors to detect gravitational ripples created
from the
collision of two
black holes some 1.3 billion years ago and had been hurtling through space to reach Earth on September 14, 2015.
The waves came
from a catastrophic event — the
collision of two
black holes located about 1.3 billion light years away
from Earth — and the released energy undulated across the universe, much like ripples in a pond.
Researchers have «dissected» the mysterious gases oozing
from two supermassive
black holes on the verge of
collision in galaxy NGC 6240 for the first time.
The LIGO experiment confirms the third detection of gravitational waves
from two
black holes in
collision The GRG - UIB group, led by Alicia Sintes, a member of MultiDark, participates in the LIGO Scientific Collaboration
When an energetic event occurs (like a
black hole merger or neutron star
collision), spacetime becomes violently disturbed and energy is carried away
from the event in the form of gravitational waves — like ripples traveling across the water's surface after dropping a pebble in a pond.
From supermassive
black holes at galactic centers to giant bursts of star formation to titanic
collisions between galaxies, these discoveries allow astronomers to probe the current properties of galaxies as well as examine how they formed and developed.
Last week, the ultrasensitive telescope her team built detected gravitational waves for the first time, created
from the
collision of two
black holes some 1.3 billion years ago.