Do Scientists Actually Detect Gravitational Waves: Debunking the Myths

Gravitational waves have been a subject of intense debate, with some scholars questioning whether they have truly been detected. Let's dive into the intricacies and complexities surrounding this topic.

Official Confirmation: Gravitational Waves Have Been Detected

It has officially been confirmed that gravitational waves have been detected with unprecedented precision. However, the question arises: what exactly were these waves? The ambiguity surrounding this detection has led to various interpretations and debates among scientists.

Challenging the Detection of Gravitational Waves

One individual, who remains anonymous, presents a compelling argument that the detected phenomenon was not gravitational waves as commonly understood. According to this person, the detectable frequency of space waves or metric waves is 111101 Hz. They emphasize that a correct interpretation of the detected frequency might provide more clarity on what was truly observed.

In response to the question, "What if you shake the Sun by one meter per second," the argument is that we would feel retarded potentials rather than gravitational waves. The gravitational potential would propagate to our location with a delay of 8 minutes and 48 seconds, similar to how the LIGO detector sensed the merger of two black holes a billion light-years away.

Faults in the Detection Method

The author also questions the validity of calling the detected dynamic propagation of matter's retarded potentials as gravitational waves. Instead, the author suggests that metric waves, as predicted by General Relativity (GR), might be a more appropriate term. According to GR, space is stretched by matter, and matter motion drags the stretched metric along. However, the author argues that waves should not be generated by this dragging, but rather by the release of the medium.

Metaphorically, in terms of gravitation, waves would be generated at the apogees and perigees of orbits. The author's calculations indicate that these waves would have a higher frequency compared to those generated during the merger of black holes. However, they would be much weaker due to the lack of proximity to twin black holes and the lack of asymmetric elliptical orbits in our giant gaseous planets.

Thus, it is argued that detecting gravitational waves might be possible but would need to be done at different frequencies, specifically at the apogees and perigees of massive bodies' orbits. The LIGO detector, it is suggested, might lack the capability to detect such waves.

Questioning the Reliability of the Experiment

Furthermore, the author raises concerns about the reliability of the experiment. According to a document that details the experiment, the lead researcher filled the project with students who had struggled academically. This raises questions about the credibility of the research and the expertise of the team.

The article also emphasizes the importance of skepticism, especially in the realm of 'big science.' The author, with experience in a 'big science' field, highlights the potential for mismatches between the intentions of the group and the actual work being done. Such mismatches can lead to misunderstandings and misinterpretations of results.

Conclusion

The detection of gravitational waves is a subject that continues to spark discussions and debates. While official confirmations exist, various arguments challenge the interpretation and reliability of the detected phenomenon. As the field of astrophysics evolves, it is crucial to remain open to new interpretations and to scrutinize the research conducted by leading scientists.