Nereid wrote:I'm not sure what this post is really about, Aristarchus, but it's interesting in any case.
That General Relativity (GR) and quantum field theory are mutually incompatible, at a very deep level, has been known almost since the 1920s, shortly after each became accepted by the physics community.
A serious experimental programme to test this fundamental incompatibility is impossible with today's capabilities, because the physical regimes in which the mutual incompatibility is most evident - at Planck scales - are impossible to create in any lab.
First, you state you don't what my previous post was about, and then you comment in contradiction of your assertion. I believe you think that throwing in such caveats will somehow qualify as a substantiation of your argument without doing the leg work of definitive research.
Secondly, you then demonstrate your willingness to reply with a comment that is simply evidence that you will not debate the premise of my previous post. We're not discussing the issues of the 1920's, or what is the capability of what can be produced in the lab today. We're discussing a major funding project to one of the top physics research institutions in the United States, i.e., the Gravity B Probe, which has stated that its research is not only inconclusive, but also that it might bring into question positing on dark energy:
"to date, there is no direct experimental evidence for the existence of either component, and there are strong theoretical reasons (the "cosmological constant problem") to be suspicious of dark energy in particular."
Finally, you continue your line of reasoning and deflection by restating something that doesn't address my post, and you completely defy the reasons behind the Gravity Probe B project with a response from you that fails to rise to even the level of "don't believe our lying eyes."
A Brief Overview of Gravity Probe B
The idea of testing general relativity by means of orbiting gyroscopes was suggested independently in late 1959-early 1960 by Stanford physicist Leonard Schiff and MIT physicist George Pugh. Pugh’s Proposal for a Satellite Test of the Coriolis Prediction of General Relativity appeared in an unusual location for scientific papers: the U.S. Department of Defense Weapons Systems Evaluation Group (WSEG) Memo #11 (November, 12, 1959). Schiff, then chairman of the Stanford University Physics Department, published a paper summarizing the experiment, Possible New Experimental Test of General Relativity Theory in the March 1, 1960 issue of Physical Review Letters. Also during this time, Schiff teamed up with two colleagues from the Stanford faculty: low-temperature physicist William Fairbank and gyroscope expert Robert Cannon of the Department of Aeronautics & Astronautics. Thus was born the collaboration between the Stanford Physics and Engineering departments that has been essential to the success of Gravity Probe B.
The Gravity Probe B Bailout
As this story went to press, GP-B project head Francis Everitt notified IEEE Spectrum that ”a significant non-NASA agency” had committed $2.7 million to continue Gravity Probe B. This, Everitt hopes, will enable his group next year to reach a conclusion on a par with its original goal of testing the two Einsteinian effects down to the 1 percent confidence level.
The project was on very shaky ground, because even after years of data massaging, GP-B had weakly confirmed one of the effects, frame dragging, to only the 25 to 33 percent range. But as Everitt and GP-B spokesman Bob Kahn, of Stanford, told IEEE Spectrum via e-mail, a recent breakthrough in the modeling of behavior of the satellite’s instruments has increased the data’s accuracy ”by a factor of 5 to 10”. The new results are to be presented early this month at an International Space Science Institute workshop on the nature of gravity.
NASA’s science advisory committee for the project has called the recent effort ”heroic.” With this summer’s work, says the report, the GP-B team ”has brought the experiment from what seemed like a state of potential failure, to a position where the [committee] now believes that they will obtain a credible test of relativity, even if the accuracy does not meet the original goal. In the opinion of the SAC Chair [Washington University physics professor Clifford Will], this rescue warrants comparison with the mission to correct the flawed optics of the Hubble Space Telescope, only here at a minuscule fraction of the cost.”
The issue at hand is that the experiments have moved out of the lab to seeking the perfecting of intrumentation in a space probe, and it still has become inconclusive and even brought into question comcepts to our understanding of dark energy.
Gravity Probe B Webcast: Mission and Science Q&A
I think Luis' question is probably relating to the Heisenberg Uncertainty Principle, which says that any time you observe an experiment, you affect it in some way. That's true, but that affect really only matters on the quantum mechanical level. In other words, if you get to the atomic or subatomic scale, then Heisenberg's principal can come into play.
In the case of Gravity Probe B, the real issue that we had was trying to make sure that so-called classical disturbance torques, the Newtonian torques, are absolutely minimized or eliminated, because the relativity effects that we’re trying to see are so subtle and so small that we really have to get rid of any other systemic noises.
That's the kind of issue we had to deal with and Heisenberg doesn’t really play into that significantly here.
Furthermore ...
Actually, it could not. In principle, what you need for Gravity Probe B is a very quiet platform, and the ISS does give you a microgravity type of environment (in other words, a very low-gravity environment), but GP-B requires an even quieter environment. Probably three or four orders of magnitude, in other words 1,000 or 10,000 times less noisy or less motion oriented than the space station is. So you really couldn't do it on the space station, even though that platform is suitable for other kinds of high-precision instrumentation.
Obviously, the experimentations have moved out of the lab, thus the onus is on you to provide information contrary to the Gravity B Probe.
An object is cut off from its name, habits, associations. Detached, it becomes only the thing, in and of itself. When this disintegration into pure existence is at last achieved, the object is free to become endlessly anything. ~ Jim Morrison