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I disagree, but I would invite you to check it by yourself.A. Neumaier said:I don't have Schlosshauers book at hand but believe he only works on this level.
Correct; they cannot, because they rely on a traditional interpretation.Demystifier said:do B&P claim anywhere that they solve the measurement problem? I don't think so. In fact, I think they don't even address the measurement problem.
Fine. But if some approach could explain evolution towards a single fixed point of the density matrix, that would be a solution of the measurement problem. Hence their approach cannot explain evolution towards a single fixed point of the density matrix. So how exactly can the thermal interpretation do that?A. Neumaier said:Correct; they cannot, because they rely on a traditional interpretation.
But I do, with their help; their calculations are independent of any interpretation and hence apply also in the context of the thermal interpretation.
Without telling what the beables are, there cannot be a solution of the measurement problem. That's the difference. The thermal interpretation has from the start unique outcomes, and only must explain which ones occur. Note that this does not involve convergence of the density matrix; only the pointer reading, i.e., in the thermal interpretation a q-éxpectation (not an eigenvalue) matters!Demystifier said:Fine. But if some approach could explain evolution towards a single fixed point of the density matrix, that would be a solution of the measurement problem. Hence their approach cannot explain evolution towards a single fixed point of the density matrix. So how exactly can the thermal interpretation do that?
But if the density matrix does not converge, then how can the expected value, uniquely determined by the density matrix, converge? If the density matrix isA. Neumaier said:Without telling what the beables are, there cannot be a solution of the measurement problem. That's the difference. The thermal interpretation has from the start unique outcomes, and only must explain which ones occur. Note that this does not involve convergence of the density matrix; only the pointer reading, i.e., in the thermal interpretation a q-éxpectation (not an eigenvalue) matters!
Some function of a matrix can converge even if the matrix itself dos not converge. Just like ##x_k=(k^{-1}-1)^k## does not converge but its squares converge.Demystifier said:But if the density matrix does not converge, then how can the expected value, uniquely determined by the density matrix, converge?
This state is only an average state. The true reduced state satisfies a nonlinear stochastic dynamics under which it is unstable and decays after tiny random displacements. Averaging never preserves a nonlinear dynamics.Demystifier said:If the density matrix is
$$\rho=\frac{1}{2}\rho_1 + \frac{1}{2}\rho_2$$
then the expected value of the observable ##O## is
$$\langle O\rangle ={\rm Tr}O\rho=\frac{ \langle O\rangle_1 + \langle O\rangle_2 }{2}$$
where ##\langle O\rangle_k={\rm Tr}O\rho_k##. I don't see how can ##\langle O\rangle## converge to ##\langle O\rangle_1## or ##\langle O\rangle_2##.
I'd like to see such an example, too. But this stuff is quite technical, and not easy to simplify. In the thermal interpretation, no eigenstate is selected, only one of two values for the q-expectation of the pointer variable. Such a 2-valuedness is what generically happens when perturbing a metastable stagte in a double-well potential. Instability in more complicated systems is similar, though in detail more complicated. But detectors are quite special systems, created to produce outcomes of a certain kind.stevendaryl said:I would like to see a worked-out "toy" example of how metastability leads to the selection of an eigenstate of the observable being measured. To me, it's very counter-intuitive.
I also think that one needs to assume beables of some sort to get definite results. Both Bohmian mechanics and the thermal interpretation introduce such beables, but in quite different ways.stevendaryl said:I actually feel that there should be a proof that it is impossible without assuming something beyond the minimal interpretation of quantum mechanics (which Bohmian mechanics does, as does the "objective" collapse models).
If that's true, then why cannot it solve the measurement problem by itself?A. Neumaier said:The true reduced state satisfies a nonlinear stochastic dynamics under which it is unstable and decays after tiny random displacements.
But expected values (that is, beables in thermal interpretation) are linear in the density matrix.A. Neumaier said:Some function of a matrix can converge even if the matrix itself dos not converge. Just like ##x_k=(k^{-1}-1)^k## does not converge but its squares converge.
Because without beables no solution of the measurement problem. The thermal interpretation provides intuitive beables.Demystifier said:If that's true, then why cannot it solve the measurement problem by itself?
Yes, but the reduced dynamics is nonlinear in the density operator. Thus there is no reason to consider your particular mixture, it is an artifact of the ignorance of the stochasticity in ##\rho##.Demystifier said:But expected values (that is, beables in thermal interpretation) are linear in the density matrix.
I have a proof that you are wrong, which I will present in a separate thread.A. Neumaier said:Yes, but the reduced dynamics is nonlinear in the density operator. Thus there is no reason to consider your particular mixture, it is an artifact of the ignorance of the stochasticity in ##\rho##.
I specified precisely what my hidden variables are. I haven't tried to classify them in terms of the notions you mention. Probably any deterministic interpretation with a wholistic dynamics for the universe looks conspiratorial, but maybe the technical meaning of this term is different.charters said:Which type of hidden variables are you contemplating here?
A. Neumaier said:I specified precisely what my hidden variables are. I haven't tried to classify them in terms of the notions you mention. Probably any deterministic interpretation with a wholistic dynamics for the universe looks conspiratorial, but maybe the technical meaning of this term is different.
If superdeterminism means that everything is determined by the state of the universe in the Heisenberg picture then the TI is superdeterministic. I don't see fine tuning as a problem - the universe is what it is, we need to describe it but not explain why it is the way it is. Moreover, most of what happens in the solar system is fairly independent of the details of the state of the universe, fine-tuning matters only for the analysis of systems fine-tuned by human preparation, such as long distance entanglement experiments.charters said:about superdeterminism
charters said:I do think you would benefit from speaking more directly on where you stand on this in the papers, as it is one of the basic frameworks for how folks mentally categorize interpretations
Actually into 6, here.A. Neumaier said:I leave it to others to classify the TI. DarMM gave recently a classification into 5 categories, and he placed the TI in the first one, together with Bohmian mechanics.
How to classify is clearly researcher-dependent...DarMM said:Category 1. Though I should rephrase it possibly.
You don't hear any of the positive statements about the TI.vanhees71 said:it's still not clarified what the interpretation of the "thermal interpretation" really is (you only told us what it is not ;-)).
I meant to say, in any fixed picture, ##\rho## is a beable. In the thread where you posted this, we were silently using the Schrödinger picture. Picture change are like coordinate changes.vanhees71 said:How can ##\rho## (assuming it's what's called the statistical operator in the standard interpretation) be a "beable", if it depends on the picture of time evolution chosen? The same holds for operators representing observables.
Yes, this physical quantity is the q-observable ##P(t,a|\rho)=\langle B\rangle##, wherevanhees71 said:What's a physical quantity (...) are
$$P(t,a|\rho)=\sum_{\beta} \langle t, a,\beta|\rho(t)|t,a,\beta \rangle,$$
where ##|t,a,\beta## and ##\rho(t)## are the eigenvectors of ##\hat{A}## and ##\rho(t)## the statistical operator, evolving in time according to the chosen picture of time evolution. In the standard minimal interpretation ##P(t,a|\rho)## is the probability for obtaining the value ##a## when measuring the observable ##A## precisely at time ##t##.
I do not forbid it; I only remove it from the foundations, and allow q-expectations (rather than eigenvalues) to be interpreted as the true properties (beables). See the previous post #590.vanhees71 said:Now, before one discuss or even prove anything concerning an interpretation, one must define, what's the meaning of this expression in the interpretation. I still didn't get, as what this quantity is interpreted in the thermal interpretation, because you forbid it to be interpreted as probabilities.
I agree. This implies that the exact state of the universe is ##\rho=e^-S/k_B##, where the entropy operator ##S## of the universe is approximately given by an integral over the energy density operator and particle density operators, with suitable weights (intensive fields). The coarse-graining inherent in the neglect of field products in an expansion of ##S## into fields makes ##S## exactly equal to such an expression and defines exact local equilibrium as an approximate state of the universe.vanhees71 said:On the other hand, I think it's pretty safe to say the universe, on a large space-time scale, is close to local thermal equilibrium, as defined in standard coordinates of the FLRM metric, where the CMBR is in local thermal equilibrium up to tiny fluctuations of the relative order of ##10^{-5}##.
For a density operator ##\rho## with positive spectrum, ##S:=-k_B\log\rho## is a well-defined operator, and I can give it any name I like. I call it the entropy operator, since its q-expectation is your entropy. In this way, the entropy operator is well-defined, and its q-expectation agrees in equilibrium with the observable thermodynamic entropy, just as the q-expectation of the Hamiltonian agrees in equilibrium with the observable thermodynamic internal energy. Thus everything is fully consistent.vanhees71 said:Last but not least, entropy is not an observable, and there's no operator for it. It's just defined (based on information theory, which you are not allowing in your thermal interpretation either, because also this information-theoretical definition of entropy is based on the probabilistic meaning of the quantum state) as ##S=-k_{\text{B}} \mathrm{Tr} \hat{\rho} \ln \hat{\rho}##.
No. The relevant state is an objective state of the full universe, independent of anyone's knowledge or even its knowability. Subjective is only its approximation by something explicit. But the same holds for the state of a Laplacian universe. Any bounded subsystem of it can know only a very limited part of this state.vanhees71 said:On the other hand you argue within this information-theoretical paradigma.
I granted your interpretation in the important case where you actually make a large number of experiments, since in this case, the statistical interpretation follows form the thermal interpretation, as I explained in detail in Section 3 of Part II. However, there are many cases where one never actually measures more than once, and these have a different interpretation since statistics is mute about such instances.vanhees71 said:not giving the explanation what this means in the lab if not an expectation value in the sense of probability theory.
This is not an operator representing an observable, because it's time evolution in a general picture is not given by the time-evolution operator for an observable but by that for a state.A. Neumaier said:For a density operator ##\rho## with positive spectrum, ##S:=-k_B\log\rho## is a well-defined operator, and I can give it any name I like. I call it the entropy operator, since its q-expectation is your entropy. In this way, the entropy operator is well-defined, and its q-expectation agrees in equilibrium with the observable thermodynamic entropy, just as the q-expectation of the Hamiltonian agrees in equilibrium with the observable thermodynamic internal energy. Thus everything is fully consistent.
Nothing information theoretic is involved, unless you read it into the formulas.
We argue in circles :-(. If you never actually measure more than once, the expectation value is provided by the measurement device. That's for sure the case for any measurement concerning a system, where classical (i.e., non-quantum) physics is a good approximation. E.g., measuring the length of the edge of my desk with an ordinary meter provides such a coarse grained observable, namely the "length of my table".A. Neumaier said:I granted your interpretation in the important case where you actually make a large number of experiments, since in this case, the statistical interpretation follows form the thermal interpretation, as I explained in detail in Section 3 of Part II. However, there are many cases where one never actually measures more than once, and these have a different interpretation since statistics is mute about such instances.
But this is the operator ##S## I was talking about in post #591, and hence gives sense to my comments about the state of the universe. Its transformation behavior is the same as that of the density operator, which is adequate for this purpose.vanhees71 said:This is not an operator representing an observable, because it's time evolution in a general picture is not given by the time-evolution operator for an observable but by that for a state.
Well, this is why the q-expectation is measurable. But it is not an expectation value in the sense of Born's rule, which is about actual measurements and not about imagined ones.vanhees71 said:If you never actually measure more than once, the expectation value is provided by the measurement device.
And why is this an expectation value?? Of which operator?vanhees71 said:measuring the length of the edge of my desk with an ordinary meter provides such a coarse grained observable, namely the "length of my table".
vanhees71 said:Interpretation is about the connection of the formal entities of the theory (for QT the Hilbert space, the statistical operators, and the operators representing observables) with physics.
Whereas I don't understand why you don't accept my definition as a definition; it satisfy your quoted requirement and others had no problem with this. You didn't say why my post #479 is not sufficient interpretation - it refers to plenty of connections between the formal entities of quantum theory with experiment (which surely is physics).vanhees71 said:I also don't understand, why you deny to define your interpretation
Yes, physicists (including myself) often forget that von Neumann equationvanhees71 said:This is not an operator representing an observable, because it's time evolution in a general picture is not given by the time-evolution operator for an observable but by that for a state.