GW170104

GW170104
The signal of GW170104 measured by Hanford and Livingston.
Other designations GW170104
Event type Gravitational wave event edit this on wikidata
Date 4 January 2017 Edit this on Wikidata
Instrument LIGO Edit this on Wikidata
Redshift 0.18 ±0.08 Edit this on Wikidata
Total energy output ≈ 2 M☉ × c2
Preceded by GW151226 Edit this on Wikidata
Followed by GW170608 Edit this on Wikidata
Related media on Wikimedia Commons

GW170104 was a gravitational wave signal detected by the LIGO observatory on 4 January 2017. On 1 June 2017, the LIGO and Virgo collaborations announced that they had reliably verified the signal, making it the third such signal, after GW150914 and GW151226.[1][2]

Event detection

The signal was detected by LIGO at 10∶11:58.6 UTC, with the Hanford detector picking it up 3 milliseconds before the Livingston detector. Automated analyses did not initially identify this event as information about the state of the Hanford detector was not being correctly recorded.[1] The event was found by a researcher at the Max Planck Institute for Gravitational Physics by visual inspection of triggers from the Livingston detector.[1][3][4] The gravitational wave frequency at peak GW strain was 160 to 199 Hz.

Astrophysical origin

Analysis indicated the signal resulted from the inspiral and merger of a pair of black holes (BBH) with 31.2+8.4
−6.0 and 19.4+5.3
−5.9 times the mass of the Sun, at a distance of 880+450
−390 megaparsecs (2.9+1.5
−1.3 billion light years) from Earth. The resulting black hole had a mass of 48.7+5.7
−4.6 solar masses, two solar masses having been radiated away as gravitational energy. The peak luminosity of GW170104 was 3.1+0.7
−1.3×1049 W.[1]

Implication for binary black hole formation

The spin axes of the black holes were likely misaligned with the axis of the binary orbit. The probability that both spin axes were positively aligned with the orbit is less than 5%. This configuration suggests that the binary black hole system was formed dynamically in a dense star cluster such as a globular cluster, i.e., as a result of gravitational interaction between stars and binary stars, in which case randomly aligned spin axes are expected. The competing scenario, that the system was formed out of a binary star system consisting of two normal (main sequence) stars, is not ruled out but is disfavored as black holes formed in such a binary are more likely to have positively aligned spins.[1]

Graviton mass upper limit

The analysis of GW170104 yielded a new upper bound on the mass of gravitons, if gravitons are massive at all. The graviton's Compton wavelength is at least 1.6×1016 m, or about 1.6 light-years, corresponding to a graviton mass of no more than 7.7×10−23 eV/c2.[1] This Compton wavelength is about 9×109 times greater than the gravitational wavelength of the GW170104 event.

See also

References

  1. 1 2 3 4 5 6 B. P. Abbott; et al. (LIGO Scientific Collaboration and Virgo Collaboration) (1 June 2017). "GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2". Physical Review Letters. 118 (22): 221101. arXiv:1706.01812 [gr-qc]. Bibcode:2017PhRvL.118v1101A. doi:10.1103/PhysRevLett.118.221101. Cite uses deprecated parameter |class= (help)
  2. ↑ Overbye, Dennis (1 June 2017). "Gravitational Waves Felt From Black-Hole Merger 3 Billion Light-Years Away". New York Times. Retrieved 1 June 2017.
  3. ↑ "Former U.P. resident helps detect colliding black holes in space". Detroit Free Press. 6 June 2017. Retrieved 17 November 2017.
  4. ↑ ""Gravitationswellen-Entdecker"". Berliner Zeitung. 5 June 2017. Retrieved 17 November 2017.
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