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I don't understand this. What other Hilbert space, do you think is needed to describe the hydrogen atom?
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}