Detection of gravitational waves

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Discussion Overview

The discussion revolves around the current state of gravitational wave detection, focusing on the sensitivity of existing instruments, the identification of potential sources for detection, and the overall feasibility of detecting gravitational waves. It encompasses theoretical and experimental aspects of gravitational wave observatories.

Discussion Character

  • Exploratory, Technical explanation, Debate/contested

Main Points Raised

  • One participant questions the current sensitivity of instruments for detecting gravitational waves and whether serious questions are arising regarding their detectability.
  • Another participant mentions LISA and LIGO as key instruments in gravitational wave detection.
  • A further contribution details LIGO's expected event rate and its limitations, noting that an upgraded version, Advanced LIGO, is anticipated to significantly improve sensitivity and detection capabilities.
  • The same participant highlights LISA's advantages, particularly its ability to detect lower frequency sources due to its space-based location, which is free from seismic noise.
  • One participant references an external thread in Cosmology for additional context on the topic.

Areas of Agreement / Disagreement

Participants express varying views on the current capabilities and future potential of gravitational wave detection instruments, indicating that multiple competing perspectives exist regarding the effectiveness and sensitivity of these technologies.

Contextual Notes

There are unresolved assumptions regarding the expected event rates and the specific capabilities of LIGO and LISA, as well as the implications of these limitations on the detectability of gravitational waves.

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What is the state-of-the-art of detecting gravity waves. Are the instruments available now sufficiently sensitive to detect gravity waves? Have we identified 'low-hanging' sources from whom gravity waves should have been detectable. Have we yet reached that point where serious questions are arising as to the direct detectiblity of gravity waves?
 
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LISA (Laser Interferometer Space Antenna)
LIGO (Laser Interferometer Gravitational-Wave Observatory)
 
To add some detail to the above;

LIGO is the current state of the art right now. However, its expected event rate is about 3 per century if I recall correctly, so it isn't terribly surprising that we haven't seen any yet. An upgraded version of LIGO called Advanced LIGO should be ready in 2014. It is about 10 times more sensitive than LIGO, and can thus see 1000 times more sources, so it should see a good amount of events every year. Its best sources are compact binaries (black holes or neutron stars). In ~2019-2020 LISA should come online. It is a gravitational wave observatory in space. Since it isn't limited by seismic noise, it can see sources with lower frequencies sources like white dwarf binaries, and extreme mass ratio events. This image illustrates their sensitivity curves: http://imgur.com/VDNpR
 
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