Two gravitational events might be a single lensed one

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SUMMARY

The gravitational wave events GW170809 and GW170814, detected by LIGO and Virgo, are proposed to be manifestations of a single event magnified by gravitational lensing. Both events exhibit similar parameters and originate from the same region of the sky, suggesting they could represent a lensed black hole merger. The authors of the related paper argue that many observed gravitational wave events may be influenced by lensing, indicating that the sources are likely smaller and farther away than previously thought. Future observation runs will clarify whether these events are indeed repetitions from a single source.

PREREQUISITES
  • Understanding of gravitational wave detection techniques, specifically LIGO and Virgo.
  • Familiarity with gravitational lensing concepts in astrophysics.
  • Knowledge of black hole mass ranges and stellar black hole observations.
  • Basic principles of binary neutron star mergers.
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  • Research the implications of gravitational lensing on gravitational wave observations.
  • Study the methods used in LIGO and Virgo for detecting and localizing gravitational waves.
  • Explore the characteristics of binary neutron star mergers and their optical counterparts.
  • Investigate the statistical methods for analyzing gravitational wave signal similarities and correlations.
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Astronomers, astrophysicists, and researchers interested in gravitational wave phenomena, gravitational lensing, and black hole mergers will benefit from this discussion.

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It has been proposed that the gravitational wave events GW170809 and GW170814 , named after their date (5 days difference) were actually a single one which appeared twice and magnified due to gravitational lensing. Both events have very similar parameters and come from the same area in the sky.

Twin LIGO/Virgo Detections of a Viable Gravitationally-Lensed Black Hole Merger

Some good discussion on reddit

More generally, the authors of the paper argue that most of the observed events could come from lensing. It would mean the sources are smaller - they would fit to the mass range of stellar black holes we know from other observations. It would also mean they are farther away. Due to the way LIGO/Virgo work we don't expect to see multiple images often, but they should still happen. Future observation runs will easily distinguish between these options. If we see more repetitions then this is probably the case, if not it is probably not.
 
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Wouldn’t their acoustic signatures correlate closely but shifted in time if they were from the same source?
 
That's what they see. Very similar signals, just shifted by 4 days.
 
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mfb said:
That's what they see. Very similar signals, just shifted by 4 days.
Has there been a search done for a viable lensing candidate?
 
I haven't seen anything. Without an optical component the localization is not good, probably too many galaxies in range.
 
mfb said:
I haven't seen anything. Without an optical component the localization is not good, probably too many galaxies in range.
Not to give up just yet, all is not lost - With their approximate angular separation plus that five day time difference it should be possible to come up with an approximate mass and distance to the lensing object and so have an idea of what they're looking for and where!
 
The localization just gives a rough direction in the sky. There is no significant (!) angular separation between the events.

A binary neutron star merger with an optical component would be great in future measurements.
 
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mfb said:
The localization just gives a rough direction in the sky. There is no significant (!) angular separation between the events.

A binary neutron star merger with an optical component would be great in future measurements.
Oops, I forgot they were found using only two detectors...
 
Three detectors (2*LIGO and VIRGO), at least the second one, but the possible area is still 90 square degrees (340 for the other event).
 

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