SUMMARY
Gravity wave time distortions cannot be measured with the same accuracy as space distortions, such as those measured by LISA, due to the inherent observer dependence of time and space in both special and general relativity. The discussion highlights that gravitational waves cause spacetime distortions, where the relative phase change of laser beams in experiments like LIGO is attributed to changes in distance and time simultaneously. The concept of "time distortion" lacks a universally accepted definition, complicating the measurement and understanding of these phenomena. The use of harmonic coordinates can eliminate perceived time distortions, but this is contingent on the chosen coordinate system.
PREREQUISITES
- Understanding of general relativity and spacetime concepts
- Familiarity with gravitational wave detection methods, specifically LIGO and LISA
- Knowledge of coordinate systems in physics, particularly harmonic coordinates
- Basic grasp of laser interferometry and its application in measuring spacetime distortions
NEXT STEPS
- Research the principles of general relativity and its implications on spacetime measurements
- Study the methodologies used in LIGO and LISA for detecting gravitational waves
- Explore the concept of harmonic coordinates and their role in simplifying spacetime analysis
- Investigate the definitions and implications of "time distortion" in various physical contexts
USEFUL FOR
Physicists, astrophysicists, and researchers in gravitational wave astronomy who are interested in the complexities of measuring spacetime distortions and the theoretical underpinnings of general relativity.