No clue why GP thinks it "shouldn't work": it's an extremely difficult engineering problem, but the physics of it is relatively straightforward.
No clue why GP thinks it "shouldn't work": it's an extremely difficult engineering problem, but the physics of it is relatively straightforward.
Amusingly Einstein both identified gravitational waves in his then new general relativity and then changed his mind about whether they existed. Indeed he had found three different types of these waves, and two of them were simply coordinate artifacts (they could be made to travel at any speed, Eddington famously quiped that they could be made to move at the "speed of thought"). The third type however didn't have this problem (though again here Einstein would write a paper where he claimed these gravitation waves required singularities, but these turned out these were all coordinates singularities .... sort of like how late and long coordinates misbehave at the poles)
In some ways the physics of it is straightforward, in other ways....not so much.
This question is important enough that there have been papers written on it. I suggest you read https://pubs.aip.org/aapt/ajp/article-abstract/65/6/501/5300... which may strengthen your understanding.
This is a physics education journal: its papers are supposed to be interesting and accessible to undergrads, not on the frontier of the field.
What the linked paper amounts to is noticing that the sensitivity of a detector depends on the relative length scales of the arms and the waves you're trying to detect. This is true, and also one of the first things you would consider when figuring out what size your detector should be. It's a good homework problem, but not news to anyone actually working on LIGO.
> No clue why GP thinks it "shouldn't work"
It's also possible you think that this is all about laser interferometry, and aren't properly considering how it could work in the context of compressing space, since a laser interferometry system in compressed space wouldn't produce interference.
I think this misrepresents the situation, but I can't say how, so I can't dismiss it quite so quickly.
Stronger signals from some black holes depending on which way they're oriented relative to the arms. And if there were many different simultaneous signals, some could mask the others.
Clearly, we need a 3-armed, space-based LIGO. Or better, a dozen of them.
[0] https://en.m.wikipedia.org/wiki/LIGO
[1] https://en.m.wikipedia.org/wiki/Virgo_interferometer
[2] https://en.m.wikipedia.org/wiki/GEO600
[3] https://en.m.wikipedia.org/wiki/KAGRA
[4] https://en.m.wikipedia.org/wiki/Laser_Interferometer_Space_A...