LIGO's Detection of Gravitational Waves: BH-BH & BH-NS Mergers

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In summary, since its detection of GW150914, A-LIGO has discovered a total of 11 confirmed mergers between black holes and neutron stars. The first run in 2015-2016 detected 2 mergers, while the second run in 2016-2017 detected 4 mergers, with the addition of the Virgo detector. The horizontal axis in the graph shows the mass of the objects detected, and the arrows indicate the mergers. However, there were also 8 candidate detections mentioned in a 2017 news release, with 2 more detections made public since then. It is unclear if there are still candidates being worked on or if they did not pan out.
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wolram
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Since it's detection of GW150914, How many BH BH mergers has it detected and how many BH NS mergers has it detected, Is it living up to the potential detection's that are predicted?
 
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  • #2
wolram said:
Since it's detection of GW150914, How many BH BH mergers has it detected and how many BH NS mergers has it detected, Is it living up to the potential detection's that are predicted?

Quoting myself from an earlier discussion. A-LIGO is still down for upgrades for the O3 run scheduled in the autumn.

The original LIGO equipment was much less sensitive than the Advanced LIGO that started gathering data for the first (01) run September 12, 2015 and found the first confirmed merger two days later. Before the first run was ended January, 2016 it discovered one candidate and one additional confirmed merger.

The second more sensitive O2 run started November 30, 2016 but was was suspended between May 8 and June 8 for maintenance, Virgo joined the two LIGOs on August 1 and the run was shut down August 25. This run discovered four mergers, two of them in August alone.
 
  • #4
I really like the attached graphic, which shows the LIGO/VIRGO detected events and how the BH/NS masses compare to objects detected by other means.

4-ligoandvirgo.jpg
 

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  • #5
phyzguy said:
I really like the attached graphic, which shows the LIGO/VIRGO detected events and how the BH/NS masses compare to objects detected by other means.

View attachment 226385
What is the horizontal axis in that graph? Time?
 
  • #6
berkeman said:
What is the horizontal axis in that graph? Time?

I'm not really sure, but I don't think the horizontal axis means anything. The objects are just spread out to differentiate them. The arrows indicate the mergers.
 
  • #7
Interestingly, the 7 July 2017 news release from LIGO (https://www.ligo.org/news.php) references eight candidate detections, although it's not clear whether that number includes the four detections (or five, if you count the not-sufficiently-statistically-significant event LVT151012) which had already been made public at that time. Since then, only two further detections have been made public. It would be nice to know if there are candidates still being worked on, or if they didn't pan out.
 

1. What is LIGO and how does it detect gravitational waves?

LIGO (Laser Interferometer Gravitational-Wave Observatory) is a scientific facility designed to detect and study gravitational waves. It does this by using two identical detectors, each consisting of two 4-kilometer-long arms that are arranged in an L-shape. A laser beam is split and sent down each arm, and then reflected back to a central location where they are recombined. When a gravitational wave passes through the detector, it causes the arms to stretch and compress, resulting in a change in the length of the arms. This change is measured by the interference pattern of the recombined laser beams, allowing scientists to detect the presence of gravitational waves.

2. What is meant by a BH-BH or BH-NS merger?

A BH-BH or BH-NS merger refers to the collision and subsequent merging of two black holes (BH) or a black hole and a neutron star (NS). These events are some of the most powerful and energetic events in the universe, releasing huge amounts of energy in the form of gravitational waves.

3. How does LIGO distinguish between different types of gravitational wave sources?

LIGO can distinguish between different types of gravitational wave sources based on the unique waveform patterns they produce. For example, the waveform produced by a BH-BH merger will be different from that of a BH-NS merger or a neutron star-neutron star merger. By analyzing these waveform patterns, scientists can determine the type of source that produced the gravitational waves.

4. What is the significance of LIGO's detection of BH-BH and BH-NS mergers?

LIGO's detection of BH-BH and BH-NS mergers is significant because it provides direct evidence for the existence of black holes and their interactions with other massive objects. It also confirms Einstein's theory of general relativity, which predicts the existence of gravitational waves. This detection opens up a new window for studying the universe and its most extreme events.

5. How does the detection of gravitational waves from BH-BH and BH-NS mergers contribute to our understanding of the universe?

The detection of gravitational waves from BH-BH and BH-NS mergers allows us to study the universe in a completely new way. These events produce some of the most powerful and energetic phenomena in the universe, and by observing and analyzing them, we can learn more about the nature of gravity, black holes, and the evolution of the universe. It also allows us to test and refine our theories and models of the universe, leading to a deeper understanding of the laws of physics that govern our world.

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