Multimessenger Astronomy with Continuous Gravitational Waves
Analysis
This paper surveys the exciting prospects of detecting continuous gravitational waves from rapidly rotating neutron stars, emphasizing the synergy with electromagnetic observations. It highlights the potential for groundbreaking discoveries in neutron star physics and extreme matter, especially with the advent of next-generation detectors and collaborations with electromagnetic observatories. The paper's significance lies in its focus on a new frontier of gravitational wave astrophysics and its potential to unlock new insights into fundamental physics.
Key Takeaways
- •Continuous gravitational waves offer a new avenue for exploring neutron star physics.
- •Combining gravitational wave data with electromagnetic observations will provide richer insights.
- •Next-generation detectors are crucial for detecting these signals.
- •Detections could provide unprecedented information about extreme matter.
“The first detections are likely within a few years, and that many are likely in the era of next generation detectors such as Cosmic Explorer and the Einstein Telescope.”