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GW190814

Gravitational wave of a "mass gap" collision From Wikipedia, the free encyclopedia

GW190814
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GW 190814 was a gravitational wave (GW) signal observed by the LIGO and Virgo detectors on 14 August 2019 at 21:10:39 UTC,[2] and having a signal-to-noise ratio of 25 in the three-detector network.[1] The signal was associated with the astronomical super event S190814bv, located 790 million light years away, in location area 18.5 deg2[n 1][1][3][4] towards Cetus or Sculptor.[5][6][7][8][9][10] No optical counterpart was discovered despite an extensive search of the probability region.[11]

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Discovery

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Simulated example of two black holes merging.

In June 2020, astronomers reported details of a compact binary merging, in the "mass gap" of cosmic collisions, of a first-ever 2.50–2.67 M "mystery object", either an extremely heavy neutron star (that was theorized not to exist) or a too-light black hole, with a 22.2–24.3 M black hole, that was detected as the gravitational wave GW190814.[1][12]

"We don't know if this object is the heaviest known neutron star or the lightest known black hole, but either way it breaks a record."

Vicky Kalogera, professor at Northwestern University.[13]

The mass of the lighter component is estimated to be 2.6 times the mass of the Sun (M1.9891×1030 kg), placing it in the aforementioned mass gap between neutron stars and black holes.[1][13][14][15][16][17]

Despite an intensive search, no optical counterpart to the gravitational wave was observed. The lack of emitted light could be consistent with either a situation in which a black hole entirely consumed a neutron star or the merger of two black holes.[14]

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See also

Notes

  1. The relatively large and distant area of the sky within which it is claimed to be possible to localize the source.

References

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