Detecting Continuous Gravitational Waves: Near Future to Next Gen Detectors
Analysis
This paper assesses the detectability of continuous gravitational waves, focusing on their potential to revolutionize astrophysics and probe fundamental physics. It leverages existing theoretical and observational data, specifically targeting known astronomical objects and future detectors like Cosmic Explorer and the Einstein Telescope. The paper's significance lies in its potential to validate or challenge current theories about millisecond pulsar formation and the role of gravitational waves in neutron star spin regulation. A lack of detection would have significant implications for our understanding of these phenomena.
Key Takeaways
- •Focuses on the detectability of continuous gravitational waves.
- •Evaluates detectability using existing data and future detectors.
- •Highlights the potential to validate or challenge theories about neutron stars and pulsars.
- •A lack of detection could challenge current theories.
“The paper suggests that the first detection of continuous gravitational waves is likely with near future upgrades of current detectors if certain theoretical arguments hold, and many detections are likely with next generation detectors.”