Schneibster
Registered Member
Well, then don't mind me while I satisfy myself you're right.no-- i have been on these science sites since 2011-12-ish, i have met many here on other sites, i know farsight's pathetic shenanigans very well.
Well, then don't mind me while I satisfy myself you're right.no-- i have been on these science sites since 2011-12-ish, i have met many here on other sites, i know farsight's pathetic shenanigans very well.
hilarious-- not at this moment-- but again, i suspect it was at the site that is now shutdown and you are very well aware of the truth of my accusations. i am sure there are some here whom remembers and can show it.Bah, you can't find a link can you? You troll.
Since I think this last statement is incorrect, let's agree that....Flat spacetime is homogenous and isotropic.
Flat spacetime + field is not.
That would be a tensor field that has the same value everywhere, not just an ordinary real tensor field like you find in our universe. But OK. I don't know if I agree whether that's what Farsight's Einstein quote means; and since it's immaterial I won't bother taking a position on that.Since I think this last statement is incorrect, let's agree that....
Spacetime is homogeneous if the metric is the same everywhere - in the jargon the metric tensor field is constant. OK? (This is the essence of Farsight's Einstein quote.)
I'll point out that it's not just the Ricci term in the curvature; the scalar curvature and the metric tensor come in as well, and so does the cosmological term. Perhaps I am not familiar with what you mean when you talk about the "Ricci field." Yes, I agree with the part about derivatives and second-order derivatives, but I'm pretty sure that the total curvature is given by either side of the whole equation, not just by one term of it.And since, at least in GR, curvature is given by the Ricci field, which is a second order derivative of the metric field with respect to local coordinates (albeit indirectly via the connection), then all that is required for the curvature tensor to vanish everywhere (i,e for spacetime to be flat) is for the metric field to be constant, by the definition of second order derivatives.
Yeah, got that.NOTE that it need not be everywhere zero, only the same everywhere.
That doesn't mean anything to me; I'm not familiar with the Laplace equation. It's aside from the point though.This is the GR equivalent of the famous Laplace equation.
Can you show this in his science or just in popular writing where he had to be imprecise?That's the way Einstein used it.
Yes, and you are quite adept at ignoring the specifics of what he wrote in his science and cherry-picking specific quotes from his imprecise popular works.Einstein said what he said.
Einstein used specific mathematical abstractions to talk about space. He also loved quantum mechanics, as one can read in his letters.No. I'm referring to space as in physics and cosmology. Not to some mathematical abstraction.
No, QuarkHead's definition of field is exactly how Einstein defined a field. You cannot find a contrary definition in any of the scientific literature that Einstein wrote.Your definition of a field is not how Einstein described a field.
In one popular work talking in a very specific context. In practice, Einstein discussed many homogeneous and isotropic gravitational fields; e.g., the various cosmological models he explored.Einstein described a gravitational field as a place where space was neither homogeneous nor isotropic.
The wave function provides probabilities for various possible events.
The collapse phrase seems like weird semantics.
You can construct a list of probabilities for dice throws. When a pair of dice is thrown & the result is 7, does anyone state the following?The collapse phrase seems semantically weird, suggesting activity stranger than that implied byThe collapse phrase implies that the wave function is some physical process rather than being analogous to a list of probabilities.
Your analogy is flawed. It's the quantum state that collapses that they're talking about when they speak about collapse. I.e. suppose the wave function is
|Psi> = |S1> + |S2> + |S3> + |S4>
If a measurement is made and the state is found to be in the state |S2> then the state goes from
|S1> + |S2> + |S3> + |S4>
to
|S2>
The its said that the wave function collapsed from |Psi> to |S2>. There's nothing wrong with that statement. See more of this at: https://en.wikipedia.org/wiki/Wave_function_collapse
I cannot parse this - you seem to be saying that it is not worthwhile to talk about the properties of something in the limiting case, in this case the metric tensor field, if the limiting doesn't occur in Nature.That would be a tensor field that has the same value everywhere, not just an ordinary real tensor field like you find in our universe.
I have already "shown" you that the Ricci curvature tensor at a point depends on the metric at the same point. And surely you shouldn't have to be told that the trace of the matrix representation depends on the matrix itself - in other words the Ricci scalar depends on the Ricci curvature tensor, which in turn depends on the metric.I'll point out that it's not just the Ricci term in the curvature; the scalar curvature and the metric tensor come in as well, and so does the cosmological term.
The "=" sign in the field equations tell you that everything on the RHS is the same as everything on the LHS - it's true that these equations are non-linear, but not so extravagantly as to make the LHS depend on the RHS and vice versabut I'm pretty sure that the total curvature is given by either side of the whole equation, not just by one term of it.
It's not aside from the point. The Laplace equation says that, where a (scalar) field exists, in the absence of a source the divergence of its gradient is zero. Or $$\nabla^2\phi =0$$I'm not familiar with the Laplace equation. It's aside from the point though.
Yes, because the wavefunction is the particle. A photon is a wave in space, not some probabilistic point-particle. When you measure the wavefunction you're measuring it with more of the same. We make electrons (and positrons) out of photons in pair production, and we can diffract electrons. An electron is a wave in space too, not some probabilistic point-particle.On that note, I'm still looking to pin down your views on measuring the wavefunction. Do you believe that the wavefunction of a single particle can, even in principle, be measured?
Because these waves in space propagate at c.And if so, how does that not lead to superluminal communication with entangled particles?
Are you thinking of somebody else? I haven't aggressively stated that I don't want to do any maths, and I didn't think I was distinguishing space and spacetime "vehemently".Schneibster said:He very aggressively states he doesn't want to do any math... You shouldn't really distinguish them so vehemently...
Right it is not a matter of not wanting to do the math, it is a matter of not being able to do the math.Are you thinking of somebody else? I haven't aggressively stated that I don't want to do any maths,
Do note that it's space that's homogeneous or inhomogeneous. And that the metric field is an abstract thing derived from your measurements. For example you could place optical clocks at various locations throughout an equatorial slice through the Earth and the surrounding space. When you plot the clock rates, your plot ends up looking like the Riemann curvature depiction because lower clocks tick slower and higher clocks tick faster. Also note that the clocks don't tick at different rates because spacetime is curved. Instead they tick at different rates because a concentration of energy in the guise of a massive planet "conditions" the surrounding space altering its metrical properties, this effect diminishing with distance in a non-linear fashion.Spacetime is homogeneous if the metric is the same everywhere - in the jargon the metric tensor field is constant. OK? (This is the essence of Farsight's Einstein quote.)
Note that the second derivative relates to the tidal force, whilst the first derivative relates to the force of gravity. In theory you could have flat-but-tilted spacetime where there's no curvature but the force of gravity is not zero.And since, at least in GR, curvature is given by the Ricci field, which is a second order derivative of the metric field with respect to local coordinates (albeit indirectly via the connection), then all that is required for the curvature tensor to vanish everywhere (i,e for spacetime to be flat) is for the metric field to be constant, by the definition of second order derivatives.
Space is a sub-manifold of spacetime. As such they MUST have the same topological propertiesDo note that it's space that's homogeneous or inhomogeneous.
This is ass-backwards, as always - the metric field ALLOWS measurements, not the other way around.And that the metric field is an abstract thing derived from your measurements
So gravity is a "force"?the first derivative relates to the force of gravity.
Ok. If I understand you right, you're saying that a measurement on one photon can't affect the wavefunction of another, spacelike-separated photon because all the waves involved only propagate at c. Does the same argument apply to entangled photons? If it does, please explain Bell inequality violations. If it does not, please re-answer the original question about superluminal communication for the case where entangled photons are used.Because these waves in space propagate at c.
Space has its metrical properties. You typically measure things using the motion of light. There's no motion in spacetime.Space is a sub-manifold of spacetime. As such they MUST have the same topological properties
There is no metric field per se. There's space, and light moving through it. When space is homogeneous light moves uniformly and there's no gravitational field. The massive planet alters the surrounding space.This is ass-backwards, as always - the metric field ALLOWS measurements, not the other way around.
Yes. See the Einstein digital papers. There's plenty of instances where Einstein referred to gravitational force.So gravity is a "force"?
Am I saying that? Note this from Wikipedia:Ok. If I understand you right, you're saying that a measurement on one photon can't affect the wavefunction of another, spacelike-separated photon because all the waves involved only propagate at c.
Yes, because you can't send information instantly. There is no superluminal communication.Does the same argument apply to entangled photons?
I can't explain it simply. And now I have to go I'm afraid.If it does, please explain Bell inequality violations. If it does not, please re-answer the original question about superluminal communication for the case where entangled photons are used. (As much as I realize this is somewhat talking past the GR discussion that's dominating the rest of the thread, I feel like it's a lot more relevant to the OP and the original topic, so I'll keep exploring the issue.)
Listen to yourself, Farsight! You are claiming that space has a metric but spacetime does not.Space has its metrical properties. You typically measure things using the motion of light. There's no motion in spacetime.
But their IS - this is the definition of a (semi-)Riemann manifold. This is precisely the model that your hero employs. You should not cherry-pick like thisThere is no metric field per se.
And so? You will forgive my sacrilegious view , but if he does he is wrong. According to his own General TheoryThere's plenty of instances where Einstein referred to gravitational force.
No, I'm trying to relate what you're saying to your claim that spacetime with a bunch of gravity fields in it is homogenous and isotropic when it's got all these bumps in it. I'm not finding that what you've claimed (spacetime + field is homogenous and isotropic) is supported. Flat spacetime is homogenous and isotropic; flat spacetime +fields is not.I cannot parse this - you seem to be saying that it is not worthwhile to talk about the properties of something in the limiting case, in this case the metric tensor field, if the limiting doesn't occur in Nature.
I have concluded that it cannot be physical because I view time symmetry as being too valuable to discard.This, to me, begs the question whether you think that a superposed state is physical or not.
Agreed on the first point, disagreed with the rest. The Transactional Interpretation is an example of one which would not require wave function physicality, and there are others. The Bell hidden variables are simply "hiding" in the future measurements.Schnieibster said:The alternative to superposed states being physical seems to me to be the assertion that a propagating particle has some value for its parameters even when they are Heisenberg uncertain, and this is belied by the three-polarizers experiment, as well as various Bell tests. And if superposed states are physical, then the wavefunction is a description of a real thing; it's not the thing itself, but a representation of the superposed state.
Actually we know that QM is not time symmetric; it is CPT-symmetric. You can reverse the Feynman diagram, but do do so you have to reverse the handedness and charges of all the particles. Time symmetry alone is only a feature of classical mechanics, not QM. But that is aside from the point.I have concluded that it cannot be physical because I view time symmetry as being too valuable to discard.
To be very clear, I think you are saying that you agree that superposed states are physical, but denying that particles change state when they interact. I find this very confusing. To me, the rest is logically required if you accept the first point. I'm also not at all clear on how particles cannot change state when they interact with other particles.Agreed on the first point, disagreed with the rest.
Bohm's interpretation is one of the others and the hidden variables hide in the "pilot wave."The Transactional Interpretation is an example of one which would not require wave function physicality, and there are others. The Bell hidden variables are simply "hiding" in the future measurements.