danshawen
Valued Senior Member
Fine, and good luck with that. No wonder guys like Schmelzer think they can just toss out relativity's assumptions and somehow bring back the aether while keeping GR's results.Translation: BNS orbital decay data can and has been numerically equated to standard linearized GR quadrupole GW emission formula, but there is to date no direct evidence via LIGO etc. We all know that. The extent to which such interferometry-based setups can be considered 'local' was discussed in those earlier threads. There have to actually be GW's there for the differential techniques to reveal any such - as discussed in those threads. Point is though your comments above are skew of the main misinfo appearing in #16 ('local' restriction), #17 (equating a hoped-for GW wavelength with some small multiple of the relevant planetary orbital size). Wrong, and wrong - as discussed in those earlier threads.
Many I think actually read them, but agreed the understanding bit is often lacking. There are various possible reasons for the latter.![]()
You all seem to think, the problem with Michaelson Morely was that the interferometer JUST WASN'T SENSITIVE ENOUGH. No, that isn't even close to the right answer.
LIGO "wasn't sensitive enough" either. So, you don't think the 1/3 wavelength analysis is correct. Where is your calculation of a typical gravity wave's wavelength? What exactly would render such a wave immune to analysis that holds for every other kind of wave, both EM AND MECHANICAL, and on all scales?
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