Discussion Overview
The discussion revolves around the sensitivity of gravitational wave antennas, particularly focusing on historical attempts to detect gravitational waves using cryo-cooled metal bars, such as Weber bars, and comparing them to modern detectors like LIGO. Participants explore the limitations of early detection methods and the implications of sensitivity on the ability to detect gravitational waves from events like black-hole mergers.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
- Historical
Main Points Raised
- Some participants question how much more sensitivity was needed for early detectors to successfully detect gravitational waves.
- Others provide historical context, noting that Weber's bars were not cooled and suggesting that this impacted their effectiveness.
- One participant mentions that the sensitivity of later detectors was in the 10^-20 range, raising the question of whether earlier detectors were just short of detection or if their narrow bandwidth was a limiting factor.
- There is a discussion about the uncertainty surrounding the required sensitivity for detection, with some suggesting that it was a "shot in the dark" during the early attempts.
- Some participants argue that the nature of gravitational wave frequencies and the limitations of narrow bandwidth detectors could have contributed to missed detections.
- One participant expresses concern about the potential consequences if Weber's detector had successfully detected gravitational waves, speculating on catastrophic outcomes.
- Several participants express frustration that their questions have not been addressed adequately by others in the thread.
- There is a mention of the sensitivity curve for various detectors, including AURIGA, to illustrate the limitations of Weber's equipment.
Areas of Agreement / Disagreement
Participants do not reach a consensus on the reasons for the lack of detection by Weber's bars. There are multiple competing views regarding the impact of sensitivity, bandwidth, and the nature of gravitational waves on detection capabilities.
Contextual Notes
Participants note that the sensitivity required for detection of gravitational waves varies significantly depending on the type of event, with mergers being short events that change frequency rapidly, complicating detection efforts.