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I just found this blog post, which gives an interpretation of virtual particles I haven't seen before.

Consider a 1D system of springs and masses, where the springs are slightly nonlinear. A "real particle" is a regular $\cos(kx-\omega t)$ wavepacket moving through the line, where $\omega$ satisfies the dispersion relation $\omega = \omega(k)$. When two real particles collide, the region where they collide temporarily looks really weird, as they interact nonlinearly, pulling and pushing on each other.

Formally, we can write this weird region as the sum of a bunch of $\cos(kx-\omega t)$ waves, but there's no guarantee they'll have the right dispersion relation. Thus, each term in the resulting expansion is a off-shell "virtual particle". If you add up all the virtual particles, you get the actual intermediate field state, which is just a weird ripple in the field where the two particles are interacting.

As another example, consider the statement "a static EM field is made of virtual particles". Under this interpretation, what that really means is, "a static field (e.g. $1/r^2$) is not equal to $\cos(kx-\omega t)$, but may be expanded in terms of such sinusoids", which is much less mysterious sounding. In fact, this is exactly what we do when we consider scattering off a potential in normal QM, e.g. in the Born approximation.

The above gives some intuition for what a 'virtual particle' means in classical field theory. They are the Fourier components of the field with $(\omega, k)$ not satisfying the dispersion relation, and they are useful in classical perturbation theory. However, they are not propagating degrees of freedom, so they only appear during interactions.

The picture above is entirely classical. Does this picture generalize to quantum field theory, giving a physical intuition for virtual particles there?

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    – David Z
    Commented Aug 20, 2016 at 14:44

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I will use the expressions "virtual particles" and "internal lines in a Feynman diagram" interchangably in this answer.

This interpretation fails because you can draw Feynman diagrams in both position and momentum space. When you draw them in momentum space and squint really hard, you might be able to convince yourself they have something to do with "Fourier components of the field", but the Fourier transform simply appears because you obtained the momentum space expressions from the position space expressions by a Fourier transform - it's not a characteristic of virtual particles.

In particular, virtual particles do not appear because we expand the field. They appear because we expand the interaction part of the time evolution operator - the n-point function we want to compute is something like $\langle \mathcal{T}\prod_{i = 1}^n \phi_i(x_i)\exp(-\mathrm{i}\lambda\int V(\phi(x))\mathrm{d}^d x)\rangle$ and the virtual particles appear when we expand the exponential as its power series and represent the resulting expressions graphically.

That we expand the time evolution operator suggests another "intuition" however: Virtual particle represent (fictitious) intermediate states over which we must sum. The time evolution operator there essentially means that when we compute the n-point function in an interacting theory, we must not only compute the "naive" n-point function, but also that in the presence of 1, 2, 3, 4, (i.e. finitely many) interactions (the vertices). At weak coupling $\lambda$, each interaction term suppresses the contribution of the summand it appear in, meaning the diagrams with few vertices contribute the most.

Heuristically: If you compare this to usual time-dependent perturbation theory in ordinary quantum mechanics (semi-randomly picked reference from a Google search [pdf]), it should be familiar: Expand the time evolution operator into its Dyson series, insert identies $1 = \sum_m \lvert m \rangle\langle m \rvert$, compute up to desired/feasible order. If we interpret $V(\phi)$ as the vertices, then the internal lines correspond to the inserted identities, meaning you may view virtual particles simply as generic "intermediate states" over which we must sum. You may even draw the same types of diagrams to organize such perturbation series in general.

What I think the blog post by Matt Strassler you're citing is getting at is that there is, regardless of all "virtual particles", of course an actual intermediate state during a QFT scattering, however complicated to describe it may be. He's saying that "virtual particles" are what physicists call that intermediate state which is...close enough, but more precisely we need to keep in mind that the intermediate states of perturbation theory aren't the same as the actual state of the system, they are computationally convenient fictions.

Finally, let me reiterate what I've said many times: Statements like "A static EM field is made out of virtual particles" are nonsense, since virtual particles are a tool in perturbation theory, not a fundamental entity in the theory. If you can manage to compute the relevant quantities without perturbation theory, then you'll never use the notion of virtual particle. Since physics does not depend on the specific mathematical method chosen to evaluate the relevant quantities, such statements have no basis in general QFT, and fail completely at strong coupling where no perturbative expansion is accessible. The only rigorous sense in which a static EM field is "made out of virtual particles" is that the Coulomb potential may be recovered from a diagram with a virtual particle in it. (Note that also in that case the Fourier transform is because we're computing stuff in momentum space, not because of the virtual particle as such.)

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    $\begingroup$ But you've given away the game in the first sentence. I know that's the standard way to define "virtual particle", but it is not the definition Strassler is advocating, which is non-perturbative. $\endgroup$
    – Rococo
    Commented Aug 23, 2016 at 5:29
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    $\begingroup$ @Rococo You may be right, but then I don't get the point of Strassler's post at all - sure, if you redefine the term "virtual particle", then it can be whatever you want. But redefining a term with an established meaning and then purporting to have "explained" it by that strikes me as a word game rather than giving any actual insight. In particular, maybe his new definition is "better" in a sense, but it doesn't answer OP's demand for an intuition of virtual particles at all, then. OP also seems to be under the impression that we're looking at an interpretation, not a redefinition. $\endgroup$
    – ACuriousMind
    Commented Aug 23, 2016 at 11:59
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    $\begingroup$ @ACuriousMind Thanks for the answer! I'm still slightly unsatisfied. I specifically care about the momentum-space case because it's only there that you get "off-shellness", which is what really confuses me. (I think an expansion in position space is already intuitive.) $\endgroup$
    – knzhou
    Commented Aug 23, 2016 at 18:05
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    $\begingroup$ Let me sharpen exactly what I'm asking for. Let's consider the exact photon propagator in QED, which is well described by perturbation theory, and the one-loop correction due to a virtual electron/positron pair. The "sum over intermediate states" described in your answer is a $d^4k$ integral over momentum states of the electron/positron field. My core question is, is there some sense in which the state of the actual electron field of a propagating (dressed) photon looks like the result of that integral? $\endgroup$
    – knzhou
    Commented Aug 23, 2016 at 18:08
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    $\begingroup$ @knzhou: The result of that integral is a number. I don't see what a number could possibly have to do with a quantum state, and I would also advise against the phrase "state of the field". Quantum fields are operators, they do not "have states". $\endgroup$
    – ACuriousMind
    Commented Aug 24, 2016 at 11:39
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CuriousMind, and many others, define a "virtual particle" as "an internal line in a Feynman diagram." Prof Strassler is advocating for another definition*.

Suppose you have a propagator for some system, with a form like:

$$G(k,\omega)=\frac{1}{\omega-\epsilon(k)-\Sigma(k,\omega)} $$

where $\omega$ is the frequency/energy, $k$ is the wavenumber/momentum, and $\Sigma$ is the (exact) self-energy. Strassler is suggesting that we define a "real particle" for this system as a configuration where $\omega=\epsilon(k)+\Sigma$, and a "virtual particle" as any pair of $(\omega,k)$ where this is not satisfied. This implies that the real particle obeys some dispersion relation between $k$ and $\omega$ and has an infinite lifetime, while neither of these are true in general for the virtual particle (since $\Sigma$ is generally complex). In practice, we usually relax this somewhat and call any very sharply defined resonance a real particle.

How does this definition of virtual particle relate to the definition in terms of a Feynman diagram? Well, roughly speaking a virtual particle in the sense of an internal line to a Feynman diagram is like a perturbative approximation to a virtual particle in the sense of Strassler.

As an example, take one of the simplest Feynman diagrams for electron-positron (Bhabka) scattering:

{scatter}

In this diagram, a real electron and a positron go in, they annihilate to a virtual photon, which then produces another real electron and positron that go out. This diagram will produce an amplitude that is schematically like

$$M(k_1,k_2,k_3,k_4)=\int\bar{\psi}(k_1)\psi(k_2)G(k_i)\bar{\psi}(k_3)\psi(k_4) dk_i$$ where $\psi,\bar{\psi}$ are the electron/positron spinors and $G$ the photon propagator, and the integral is over the four-momentum of the photon without any constraint relating the components**.

But really this is just the first perturbative term (or actually only one of the first perturbative terms) for the true electron-positron interaction, which will be a sum of many Feynman diagrams with the same real particles but a variety of virtual particles. This can be represented symbolically as:

{scatter2}

This exact interaction between the electron and positron, as mediated by the electromagnetic field, is what corresponds to the Strassler sense of a virtual particle. Physically, it is a general disturbance in the electromagnetic + electron/positron fields. It does not have any constraint relating energy and momentum; both enter into it as independent variables. It is described by some complicated propagator, which practically speaking can only be evaluated perturbatively. In the limit of only the simplest tree-level diagrams, it will sometimes be identical to the internal line sense of a virtual particle, but the identification does not seem to me to be that precise.

Of course, whether this redefinition is an improvement is a subjective question that you may decide for yourself. The advantages of it are that it makes "virtual particle" into an actual physical phenomenon, which is important but doesn't seem to currently have a snappy name, it is at least somewhat related to the definition in terms of internal diagram lines, and it makes those popular pop-sci statements like "the Couloumb force/ Casimir effect is due to virtual photons" at least closer to being truthful. The main disadvantage, in my opinion, is simply that careless use of the term "virtual particle" already causes a lot of confusion and promoting another definition might only add to that.

*I take responsibility, of course, for any errors in understanding or interpretation of this viewpoint. Also, I will use "virtual particle" to mean the Strassler sense, except where noted.

**Since this integral does include the values in which the real particle dispersion relation happens to be satisfied, it seems to me that in the Strassler definition it is really a broader category of disturbance that includes real particles as a special class, rather than being mutually exclusive.


knzhou asks, how does this relate to the state of the photon field? Well, the Feynman diagram I've written above (in perturbative and exact forms) represents the amplitude for the process:

$$\langle 0, k_4 k_3 | 0, k_1 k_2 \rangle $$

where the quantum numbers are the state of the EM field, the electron, and the positron. Which is to say, scattering that leaves the EM field undisturbed asymptotically. To find the actual state of the EM field and how it evolves, you would have to find the amplitudes that it is changed as well: $\langle 1_q, k_4 k_3 | 0, k_1 k_2 \rangle $, $\langle 1_q 1_{q'}, k_4 k_3 | 0, k_1 k_2 \rangle $, and so on as high as you like. Then for a given pair of input momenta, you can Fourier transform all of these back to real time and string these together to find out how the field configuration evolves, either in the Fock basis that it was calculated or the actual spatial profile just by adding the appropriate cosine terms for each photon occupation. If you undertake that, please do let me know what it turns out looking like ;)

I can hear you protesting now: I've only given you a recipe for the EM field configuration in terms of asymptotic final states, when you asked specifically for the intermediate state (and in particular, how this relates to virtual particles). But this is the only thing it makes sense to specify. This is already true in regular quantum mechanics. For an atom decaying from an excited state, maybe with a state that looks like

$$|\psi(t)\rangle = e^{-t/\Gamma}|e\rangle + \sqrt{1-e^{-t/\Gamma}}|g\rangle$$

you will sometimes hear people ask what the state is "in the middle of the decay." It is a natural question, but ill-defined nonetheless. So it seems to me that the statement that "virtual particles do not have a state" is true for either of the definitions of virtual particle discussed here.

In conclusion, it seems to me that the fields are divided up somewhat differently in QED than in classical electrodynamics. In the classical theory it's totally normal to consider the total E and B fields from both sources and radiation, and add them up and look at the impact of this total field on some charged particle. But in QED there is no state associated with this "total electric field"- you look at effects from radiation and effects from other charges (mediated by the EM field) separately. The former are real photons, and the latter are what Strassler would call virtual photons.

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    $\begingroup$ Thanks for the answer! However, I wanted something more specific -- how exactly does the integral over photon four-momenta in your answer relate to the actual intermediate state of the photon field? I'm trying to build intuition for the 'actual state', and I think propagators are one level removed from that. $\endgroup$
    – knzhou
    Commented Aug 23, 2016 at 18:12
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    $\begingroup$ @knzhou I see what you're getting at. I have written some thoughts about this, which ended up as a bit of a treatise, so apologies for that... $\endgroup$
    – Rococo
    Commented Aug 24, 2016 at 4:41
  • $\begingroup$ I would welcome any elaboration from the downvoter... $\endgroup$
    – Rococo
    Commented Aug 28, 2016 at 19:52
  • $\begingroup$ @Rococo-Why are the $D$'s and $\bar D$ in the above expression for $M(k_1 , k_2 , k_3 , k_4)$ propagators and not Dirac spinors (and their adjoints)? $\endgroup$ Commented Apr 7, 2017 at 0:50
  • $\begingroup$ @descheleschilder you are quite right, I don't know what I was thinking there. I have (belatedly) fixed it. $\endgroup$
    – Rococo
    Commented Jun 28, 2017 at 2:07
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I want to share my thoughts too as I have pondered about this before.

Basically, we have two different ways to calculate the correlation functions of the interacting theory $\langle 0| \Pi _i \phi(x_i) |0\rangle$:

  1. The path integral which involves a sum over contributions of all field configurations, which includes off-shell intermediate field configurations.

  2. The perturbation series involving the propagator, which involves intermediate propagators with off-shell mass-energy relations.

We want to know if the presence of off-shell intermediate field cofigurations in $(1)$ directly leads to the presence of off-shell intermediate propagators in $(2)$.

$(1)$ and $(2)$ are related in the sense that you can use $(1) $ to derive $(2) $. But in my opinion, there no deep connection between the presence of off-shell quantities in $(1)$ and $(2)$.

This is because the presence of off-shell mass-energy relations in $(2)$ is not natural, but is somewhat forced. The original version of the perturbation series in $(2)$ only involves tensor products of Green's function of the field.

It's only after that you re-express the Green's function in terms of its Fourier transform that you get the off-shell mass-energy relations. The Green's function itself knows nothing about off-shell momenta and is simply a function of space-time co-ordinates.

So the presence of off-sheel mass-energy in the perturbation series is nothing deep, but merely our algebraic freedom to re-express the result in terms of a Fourier transform. This fact gets clouded after we plug-in the perturbation series into the LSZ-reduction formula, because the LSZ formula cancels out the space-dependence of the Green's function and leaves us with merely the sum in the Fourier space.

Furthermore, the perturbative expansion of interacting classical field theories is also a perturbative expansion in the Green's function. So one can choose to re-write this series as a sum over off-shell propagators. But obviouly, this can't be anything deep because classical theories do not have off-shell quantities.

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Firstly, in the classical context, at least in the linear case, the notion of a virtual particle does not work. The reason is that the state of a particular system would be superpositions of solutions of that system's equations of motion. Hence, all such states would be "on-shell." One may find evanescent solutions, which might be considered analogous to virtual particles, but they differ from virtual particles in the sense that they are still on-shell. Virtual particles do not satify the equations of motions for the free-field and are therefore "off-shell." How much this scenario changes when the classical system becomes slightly nonlinear, I cannot say.

As for the quantum (field theoretical) interpretation of virtual particles, I want to be contrarian and argue in favour of the idea that one can indeed consider them as the constituents of the static EM field. For this purpose consider a Feynman diagram for the scattering between two fermions via the exchange of a photon (tree-level). In this diagram the vertices represent points is space-time (which we integrate over) and the internal line represents a propagator or Greens function, which also represents an integral over momentum space; i.e. one can get such a progagator from an integral over all plane waves in momentum space. Momentum conservation at the vertices requires that the internal line is (mostly) off-shell and therefore it is interpreted as representing a virtual particle.

So on the one hand we have the notion of a propagator composed of several plane waves and on the other hand we have the virtual particles. To match these two notions we need to include the possibility of plane waves that are off-shell, connecting the two vertices in the diagram. Being off-shell, the strength of the contribution of a particular configuration of this diagram will depend on the distance between the two vertices; the contribution becomes smaller as the vertices move further apart.

Now consider the situation where we fix the one vertex. One can see this vertex as the one fermion (charged particle) producing a static field that the other charge particle feels. This field is precisely that which is represented by the internal line. Prior to the integrations, the line is just one off-shell plane wave. The integrations now represent a complicated (inverse) Fourier transform processes that reproduces the whole scenario of a particle from the diagram. So that in the end we have a charge particle with the static field around it and another charge particle that scatters from this static field.

I do realise that this explanation leaves one the option to either accept or reject it, but we need to understand that questions of this kind are difficult to answer in a scientific manner.

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