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Well, there's no product constriction anymore in the wavefunction, because you're not forced to take f(x_1,x2) = g(x_1)h(x_2). Why would separation of variables be a requirement?
dextercioby said:Well, there's no product constriction anymore in the wavefunction, because you're not forced to take f(x_1,x2) = g(x_1)h(x_2). Why would separation of variables be a requirement?
Just to get you right: you think that the problem is that the potential can't be written in product form, not the specific \frac{1}{|\vec r_e - \vec r_p|} form of the Coulomb potential?dextercioby said:I didn't say <something is missing>, but stated that what's missing is a treatment of the H atom starting with the initial (that is non quasiparticle separated) Hilbert space as H_el ⊗ H_p derived from the axiom of states description for multiparticle systems. To this original tensor product one has to say that it's of no use, because of the non-separability of the potential.
dextercioby said:I didn't say <something is missing>, but stated that what's missing is a treatment of the H atom starting with the initial (that is non quasiparticle separated) Hilbert space as H_el ⊗ H_p derived from the axiom of states description for multiparticle systems. To this original tensor product one has to say that it's of no use, because of the non-separability of the potential. That's why I invoked the isomorphism which allows for a use of f(x_e,x_p,t) as a wafunction, that is L^2(R^6).
If by the Hilbert space H you mean the hydrogen atom wavefunction, why would you go to L2(R6)=L2(R3) ⊗ L2(R3) if its subsystems e and p are clearly not separable states?dextercioby said:The isomorphism is needed to go from an abstract Hilbert space H to L2(R3) or to L2(R6) or to L2(R3) ⊗ L2(R3)
I don't think it is so simple when dealing with wave functions and position as opposed to spin. Even before we get to the hamiltonian. You seem to be assuming that the hydrogen atom is a separable state, If the tensor product you write above can be written in general you are getting rid of the distinction separable/entangled for states, making all of them separable by definition.vanhees71 said:Somehow this simple issue becomes more and more confusion. So I try again:
The Hilbert space for a hydrogen atom in the non-relativistic approximation, neglecting spin (i.e., what you deal with in QM 1 usually after a few weeks of introduction to QT) is the tensor product of the Hilbert space of a single electron and a single proton (in sense of Hilbert spaces of course, i.e., inducing the scalar product from the spaces in the product).
It consists of all superpositions of an arbitrary product basis (or generalized basis). One example for a product basis are the simultaneous generalized position eigenvectors,
$$|\vec{x}_e \rangle \otimes |\vec{x}_p \rangle=|\vec{x}_e,\vec{x}_p \rangle.$$
An arbitrary state $$|\Psi \rangle \in \mathcal{H}_e \otimes \mathcal{H}_p$$ is then represented by the wave functions
$$\Psi(\vec{x}_e,\vec{x}_p)=\langle \vec{x}_e,\vec{x}_p|\Psi \rangle.$$
Now, it's clear that due to the Coulomb-interaction term in the Hamiltonian, the energy eigenstates are not product states of an electron and a proton state. That's all. There's no reason to confusion.
As you know, because you have explained it here, the Hilbert spaces used depending on how realistic or how good you want the approximation are: ##L^2(R^3)## , or the ##cm \times rel## exploiting the symmetry of the potential (or even Pauli's ##L^2(R^3)\otimes C^2##) but you will never see on any textbook describing the H atom with ##H_e \otimes H_p## and getting any reasonable result, the reason is that it is not a separable state which is the condition to treat H as a pure(elementary) tensor hilbert space. But for some strange reason that you might try and explain, you and other sources keep saying that it can be described by ##H_e \otimes H_p## as a matter of fact, is it any more than a rhetorical claim without any base in the practice of QM?vanhees71 said:I don't understand this. What other Hilbert space, do you think is needed to describe the hydrogen atom?
But why do you restrict the discussion to the time-independent situation, I'm referring to the general situation that includes dynamics.vanhees71 said:I still don't understand this statement. The Hilbert space is ##L^2(\mathbb{R}^6,\mathbb{C})##, and the energy eigenfunctions are
$$u_{\vec{P},nlm}(\vec{R},r,\vartheta,\varphi)=N \exp(\mathrm{i} \vec{P} \cdot \vec{R}) R_n(r) Y_{lm}(\varphi,\vartheta),$$
with ##\vec{R}=(m_e \vec{r}_e+m_p \vec{r}_p)/(m_e+m_p)##, ##\vec{P}=\vec{p}_e+\vec{p}_p##, ##\vec{r}=r(\cos \varphi \sin \vartheta,\sin \varphi \sin \vartheta,\cos \vartheta)=\vec{r}_e-\vec{r}_p)##. As you see, the energy eigenfunctions are indeed in ##\mathcal{H}_e \otimes \mathcal{H}_p##. Why do you think, it's not? Of course the energy eigenstates are not a product of electron and proton wave functions, but it's still in ##\mathcal{H}_e \otimes \mathcal{H}_p##. Again, what other Hilbert space should it be, if you have a system consisting of an electron and a proton?
vanhees71 said:I still don't understand this statement. The Hilbert space is ##L^2(\mathbb{R}^6,\mathbb{C})##, and the energy eigenfunctions are
$$u_{\vec{P},nlm}(\vec{R},r,\vartheta,\varphi)=N \exp(\mathrm{i} \vec{P} \cdot \vec{R}) R_n(r) Y_{lm}(\varphi,\vartheta),$$
with ##\vec{R}=(m_e \vec{r}_e+m_p \vec{r}_p)/(m_e+m_p)##, ##\vec{P}=\vec{p}_e+\vec{p}_p##, ##\vec{r}=r(\cos \varphi \sin \vartheta,\sin \varphi \sin \vartheta,\cos \vartheta)=\vec{r}_e-\vec{r}_p)##. As you see, the energy eigenfunctions are indeed in ##\mathcal{H}_e \otimes \mathcal{H}_p##. Why do you think, it's not? Of course the energy eigenstates are not a product of electron and proton wave functions, but it's still in ##\mathcal{H}_e \otimes \mathcal{H}_p##. Again, what other Hilbert space should it be, if you have a system consisting of an electron and a proton?
vanhees71 said:The operator, representing the Coulomb potential then acts on these functions in the straight-forward way
$$\hat{V} \Psi(\vec{x}_e,\vec{x}_p)=-\frac{e^2}{4 \pi |\vec{x}_e-\vec{x}_p|} \Psi(\vec{x}_e,\vec{x}_p).$$
There's no need to expand it in a sum of products of functions of ##\vec{x}_e## and ##\vec{x}_p##.
Shyan, thanks a lot for finding that proof!Shyan said:It seems to me that this is relevant here and may help. The author proves that the tensor product of infinite dimensional Hilbert spaces do not exist.
But the standard formalism never uses the tensor product for systems like the hydrogen atom in practice as we have seen in this thread! As other posters said it is only used (when continuous operators and dynamic interactions are involved, I'm not obviously talking about 2-dimensional Hilbert spaces like those involving spin) as a very crude approximation for certain problems in chemistry.vanhees71 said:Well, then why does the standard formalism work so well for the hydrogen atom?
Obviously, and?We are working in rigged Hilbert space, by the way!
This operator doesn't have the form of a pure tensor and therefore cannot be the Hamiltonian acting linearly on a completed tensor product Hilbert space state.vanhees71 said:I also don't understand the principle problem for general states. The time evolution of the wave function is governed by the two-body Schrödinger equation with the Hamiltonian
$$\hat{H}=-\frac{1}{2m_e} \Delta_e - \frac{1}{2m_p} \Delta_p-\frac{e^2}{4 \pi |\vec{x}_e-\vec{x}_p|}.$$
If this is true, and I believe so, then the wave function can be explicitly written as an expansion of terms of the form ##\mathcal{H}_e \otimes \mathcal{H}_p##. A sum can describe electron-proton correlation even if the individual terms do not. I would like to see the result of such an exercise.vanhees71 said:As you see, the energy eigenfunctions are indeed in ##\mathcal{H}_e \otimes \mathcal{H}_p##. Why do you think, it's not? Of course the energy eigenstates are not a product of electron and proton wave functions, but it's still in ##\mathcal{H}_e \otimes \mathcal{H}_p##.
In the discrete case.vanhees71 said:Yes, of course
$$|\Psi \rangle = \int \mathrm{d}^3 \vec{x}_e \int \mathrm{d}^3 \vec{x}_p |\vec{x}_e,\vec{x}_p \rangle \langle \vec{x}_e,\vec{x}_p |\Psi \rangle.$$
That writes any state of the electron-proton system in terms of (generalized) product states, ##|\vec{x}_e,\vec{x}_p \rangle##.
And what is the result for NR H ?vanhees71 said:Yes, of course
$$|\Psi \rangle = \int \mathrm{d}^3 \vec{x}_e \int \mathrm{d}^3 \vec{x}_p |\vec{x}_e,\vec{x}_p \rangle \langle \vec{x}_e,\vec{x}_p |\Psi \rangle.$$
That writes any state of the electron-proton system in terms of (generalized) product states, ##|\vec{x}_e,\vec{x}_p \rangle##.
Well, it is used actually, but not in the naive form of a tensor product of free particle Hilbert spaces ##\mathcal{H}_e \otimes \mathcal{H}_p##. Indeed, the free case has strictly positive energy, hence would have a hard time describing negative-energy bound states.TrickyDicky said:But the standard formalism never uses the tensor product for systems like the hydrogen atom in practice as we have seen in this thread!
dextercioby said:From my point of view, everything that needed to be said was said. This is not going into a positive direction. I can sum up my posts here as follows:
The H-atom in its simplest description (a non-specially relativistic Hamiltonian without spin) is a 2-particle system made up of an electron interacting with a proton through the Coulomb potential. You need an axiom (or at least a statement) of QM to describe how the Hilbert space of the whole system is built, if you already know the Hilbert space of the subsystems. I claimed that natural proposal of the tensor product is useless for the H atom (and as reinforced by the posters here also for other models), because the potential operator is ill-defined in such a tensor product space. For the potential operator to be well-defined, it needed to be described as a tensor product. There's a mathematical statement which cures this issued mentioned in the OP which tells us that the the correct Hilbert space is L2(R6) which solves the problem raised by the potential operator.
Since most textbooks of QM don't speak about the Hilbert spaces of the various models being described (and the H-atom appears in almost every textbook), I think that this argument I made is useful. Entanglement and means to solve the spectral problem of the Hamiltonian are only secondary.
vanhees71 said:I disagree. It's all well-defined, and the Hilbert space of a hydrogen atom in this approximation is the tensor-product space of the electron and proton Hilbert spaces. I've given the reasons for this in the previous postings. It's standard textbook knowledge. At least you find it already in Sommerfeld's "Atombau und Spektrallinien".
Yes, I know. I went a bit overboard in #74 trying to emphasize my point and on rereading it I think some explanation is in order. What you (and vanhees) say about the two-body functionally independent treatment of the hydrogen atom is of course true in the context of E<0. But my point was that when applying the naive tensor product one obtains 6 coordinates, 3 for the free center of mass and three for the relative degrees of freedom, and we obviously concentrate on the latter to solve the bound state problem using the spherical symmetry, this was what I meant when I referred to ##L^2(R^3)##,that in practice we are using just those three degrees of freedom to solve the problem, i.e. the translational invariance of the potential allows us to treat it as a one particle with reduced mass problem. So as you say we are not using the naive ##\mathcal{H}_e \otimes \mathcal{H}_p## tensor product but a bit less naive ##\mathcal{H}_{CoM} \otimes \mathcal{H}_{rel}##(BTW this was already pointed out by vanhees in a previous post) that in actuality gets us back to ##L^2(R^3)## FAPP.strangerep said:Well, it is used actually, but not in the naive form of a tensor product of free particle Hilbert spaces ##\mathcal{H}_e \otimes \mathcal{H}_p##. Indeed, the free case has strictly positive energy, hence would have a hard time describing negative-energy bound states.
The useful tensor product involves a product between spaces representing functionally independent degrees of freedom. I.e., the CoM and relative degrees of freedom. This is even intuitively "natural": we think of the H-atom as sitting motionless in front of us, hence (in our imagination) we have already separated out these functionally independent degrees of freedom.
But this tends to be done when we're still thinking in classical terms, with a classical phase space. Then we bother only about the detailed quantization of the relative degrees of freedom. But, strictly speaking, we still have some kind of (possibly generalized) tensor product of the (quantizations of) the CoM and relative degrees of freedom.
Yes, entanglement is basis-dependent, therefore context dependent. But I still think that in the dynamic case(so I'm not referring here to the time-independent Schrodinger equation that we have been discussing above but the time-dependent situation in which the time evolution operator needs to include an interaction Hamiltonian that is not in the form of a pure tensor), there is no way to avoid entanglement and therefore there is no separability, so the tensor product postulate in the OP loses generality if this is not added. This obviously even before entering on the validity of the above-mentioned proof about impossibility of tensor products for infinite-dimensional HS.BTW, this also relates to the earlier confusion about "entanglement" in the context of this problem: if one has a non-elementary system, it is possible (in general) that decomposing it one way may result in entangled pieces, but decomposing it a different way might not. I.e., entanglement is not necessarily invariant under different decompositions of a given system. (Ref: ch 21 of Ballentine, 2015 edition.)
Agreed.This highlights the lesson of this thread, (according to me, anyway), that for quantization of a complex system to work, an essential technique is that one must think in terms of functionally independent degrees of freedom (and associated symmetries) of the total system, rather than arbitrarily restricting oneself to one particular (fictitious) decomposition of that system
Yes we can :dextercioby said:But what about the potential? Well, I claim that it's not possible to write it in a tensor product way, due to the complicated form: square root, power of -1, sum.
We can(in the stationary case) basically because of what dextercioby explained, the isomorphism between separable infinite dimensional Hilbert spaces. The tensor product salvaged by this isomorphism is basically a cartesian product that dodges the impossibility proof by Garrett mentioned previously.my2cts said:Yes we can :
$$|\Psi \rangle = \int \mathrm{d}^3 \vec{x}_e \int \mathrm{d}^3 \vec{x}_p |\vec{x}_e,\vec{x}_p \rangle \frac{-e^2}{4 \pi |\vec{x}_e-\vec{x}_p|}\langle \vec{x}_e,\vec{x}_p |.$$
This puts the potential on a basis of product states, ##|\vec{x}_e,\vec{x}_p \rangle##.
This type of integrals is routinely calculated in Quantum Chemistry codes for the description of e-e repulsion on a basis set.
my2cts said:Yes we can :
$$|\Psi \rangle = \int \mathrm{d}^3 \vec{x}_e \int \mathrm{d}^3 \vec{x}_p |\vec{x}_e,\vec{x}_p \rangle \frac{-e^2}{4 \pi |\vec{x}_e-\vec{x}_p|}\langle \vec{x}_e,\vec{x}_p |.$$
This puts the potential on a basis of product states, ##|\vec{x}_e,\vec{x}_p \rangle##.
This type of integrals is routinely calculated in Quantum Chemistry codes for the description of e-e repulsion on a basis set.
Physics Monkey said:I gather this has already been said by various people, but I wanted to add my voice to those pointing out that the Coulomb potential can be defined in the tensor product Hilbert space.
To make things conceptually simple, let us agree to regulate everything, say by putting the system in a box of some arbitrary large size and introducing a lattice cutoff. The details are not crucial and can be negotiated but it renders most objections about infinite dimensional Hilbert spaces and so forth moot. Furthermore, I claim no physics can depend on the presence of a cutoff provided it is made suitably small (or large) as appropriate.
Then we could write the potential as
\hat{V} = \sum_{x_e, x_p} V(x_e - x_p) |x_e \rangle \langle x_e| \otimes |x_p \rangle\langle x_p |.
There are also other versions of this formula, e.g. in many particle physics, where we replace the projectors onto electron and proton positions with densities.
Dirac formalism is often deceiving, see below.Physics Monkey said:I gather this has already been said by various people, but I wanted to add my voice to those pointing out that the Coulomb potential can be defined in the tensor product Hilbert space.
...
Then we could write the potential as
\hat{V} = \sum_{x_e, x_p} V(x_e - x_p) |x_e \rangle \langle x_e| \otimes |x_p \rangle\langle x_p |.
In the general case(that includes dynamics) to both, it multiplies the two particle wave function ##ψ(r1, r2)## and that is the problem.dextercioby said:I was thinking about the same things when I first wrote the OP. Namely try to express the potential operator simply as
\hat{V} = \frac{1}{4\pi\epsilon_0 |\vec{x}_e-\vec{x}_p|} \hat{1}_{e}\otimes\hat{1}_{p}
But now I wonder if this makes any sense because the fraction could belong to any of the 2 unit operators, or perhaps to both at the same time?
I don't think that this by itself is useful. \hat{1}_{e}\otimes\hat{1}_{p} is the identity in the big space. Either, the fraction is also an operator, then you can omit the identity. Or the fraction is a number, then \hat V is proportional to the identity and doesn't describe an interaction in the first place.dextercioby said:I was thinking about the same things when I first wrote the OP. Namely try to express the potential operator simply as
\hat{V} = \frac{1}{4\pi\epsilon_0 |\vec{x}_e-\vec{x}_p|} \hat{1}_{e}\otimes\hat{1}_{p}
Right. It was addressed in #87. Is it also not useful?kith said:I don't think that this by itself is useful. \hat{1}_{e}\otimes\hat{1}_{p} is the identity in the big space. Either, the fraction is also an operator, then you can omit the identity. Or the fraction is a number, then \hat V is proportional to the identity and doesn't describe an interaction in the first place.
Is that different from introducing quasiparticle states either in the H atom like above or in the lattice?What you can do is insert another identity in front and decompose both identities in terms of simultaneous eigenstates of \hat{\vec X_e} and \hat{\vec X_p}. The existence of these eigenstates may be a problem but let's follow Physics Monkey's suggestion and have a look at the approximated case first.
I tried to explain that the only problem is time-dependency in the inf-dim. case(and it is not an issue just for the tensor product postulate). The rest is fine. Do you agree?kith said:For a start, does everyone agree that there's no problem with interacting systems in the case of finite-dimensional spaces or is this controversial?
TrickyDicky said:Right. It was addressed in #87. Is it also not useful?
I didn't get your point. If you are okay with the fact that the interaction Hamiltonian is not in pure tensor form for finite dimensional spaces (like two distinguishable spin-1/2 systems), which step exactly fails in the infinite dimensional case?TrickyDicky said:I tried to explain that the only problem is time-dependency in the inf-dim. case(and it is not an issue just for the tensor product postulate). The rest is fine. Do you agree?
Why should it lead to quasiparticles? You get Physics Monkey's result this way.TrickyDicky said:Is that different from introducing quasiparticle states either in the H atom like above or in the lattice?
|x_e\rangle lives in \mathcal{H}_e and we can forget about the rigged Hilbert space if we use Physics Monkey's approximation. I don't really understand what your issue is. Do you think it is also present if we have two (distinguishable) spin-1/2 systems? If not, what's the crucial difference?dextercioby said:I'm still having a trouble to understand why those projectors can be used in a tensor product decomposition, since the |x_e\rangle\ from that product is not even known, not to mention that the (possibly rigged) Hilbert space in which it "lives" is also not known.
The composite 2-dimensional HS case is clearly different, any sum of products can be expressed as a pure tensor with a unitary transformation, the projection operator is orthogonal so it is not affected by time-dependent perturbation.kith said:I didn't get your point. If you are okay with the fact that the interaction Hamiltonian is not in pure tensor form for finite dimensional spaces (like two distinguishable spin-1/2 systems), which step exactly fails in the infinite dimensional case?
But that approximation amounts to ignoring the interaction(the projection operators are not unitary here). Unless the interaction is so weak that allows you to do it(not the case for hydrogen), you need some simplyfying geometric or energy decomposition in the form of Com/rel or simlar, and that only for the time independent case.You get Physics Monkey's result this way.
This is very misleading. The author just shows that in the category ##Hilb## of Hilbert spaces, there are no tensor products in the sense of tensor products of modules. However, not all tensor products are tensor products of modules. The general definition of tensor product is captured by the concept of a monoidal category. The category of (##R##-)modules is just a particular example of a monoidal category. In ##Hilb##, we have a different definition of tensor product, so this is just a terminology issue. When we talk about tensor products in ##Hilb##, we really mean the completion of the tensor product of modules with respect to the canonically defined inner product. With this definition of tensor product, ##Hilb## can be shown to satisfy all properties of a monoidal category and so it is legitimate to talk about tensor products of Hilbert spaces.Shyan said:It seems to me that this is relevant here and may help. The author proves that the tensor product of infinite dimensional Hilbert spaces do not exist.
It is not a finite versus infinite issue. The issue arises for time-dependent interactions of 3 or more dimensions Hilbert spaces states, it is there where one has to deal with unavoidable entanglement (non-separability) which is not compatible with the HS tensor product definition.Physics Monkey said:I do not concede that there is any problem with the infinite dimensional statements, but for conceptual simplicity I think its best to first be clear about the finite dimensional case (which, again, I claim is sufficient for physics). So let us consider \mathbb{C}^n \otimes \mathbb{C}^n. Then
1. Not every operator O is equivalent under unitary transformation to a pure tensor product. For example, consider a density operator (positive, normalized, hermitian) on the tensor product. Because the spectrum of the operator is invariant under unitary transformations we can get a contradiction by counting eigenvalue degrees of freedom. A generic pure tensor product density matrix has 2(n-1) free eigenvalues (2 for the two product density matrices and n-1 because each product density matrix must be normalized). Meanwhile a generic density operator on the tensor product has n^2-1 free eigenvalues.
2. The finite dimensional approximation (and maybe its not even an approximation in quantum gravity) in no way amounts to ignoring the effects of interactions. Interaction effects are present in both statics and dynamics. For example, one can calculate the low lying states of hydrogen to high accuracy using a lattice regulated system.