Einstein's theory of Brownian motion: The non-Fickian normal diffusion

summary

Video file (mp4)

The gist

The gist Einstein’s theory of Brownian motion can be generalized to include space-dependent diffusivity, revealing that non-Fickian diffusion is actually normal diffusion consistent with Einstein's

In short

The paper extends Einstein's Brownian motion theory to include space-dependent diffusivity. It shows that this generalization leads to non-Fickian diffusion, which is actually a form of normal diffusion consistent with Einstein's postulates. This means that space-dependent diffusivity can drive concentration inhomogeneities instead of just relaxing them.

Key concepts

Fickian Diffusion
This is the original concept where the rate at which particles spread (diffusion current density) depends only on the concentration gradient and a constant diffusion coefficient. It describes how particles move to smooth out concentration differences, but it assumes a uniform environment.
Space-Dependent Diffusivity
This occurs when the diffusion constant D changes depending on where you are in space, denoted as D(x). This is not just a special case; it arises naturally from Einstein's theory. It reflects an underlying inhomogeneity in the physical space itself.
Non-Fickian Normal Diffusion
This term describes diffusion where the movement of particles is still fundamentally normal (like Brownian motion), but because the diffusivity varies spatially, it can actively drive concentration differences to create inhomogeneities. This is a consequence of Einstein's theory when space is not perfectly uniform.
Symmetry Breaking in Transport
The paper highlights that normal diffusion isn't just about smoothing things out; it relates to the underlying properties of the space. When diffusivity changes with position, it implies that the homogeneity and isotropy of the space are broken at large scales, forcing particles to move asymmetrically.

Terminology used across episodes

This episode discusses

The paper

Einstein's theory of Brownian motion: The non-Fickian normal diffusion · Read on arXiv

Indian Institute of Science Education and Research, Pune

Einstein's theory of diffusion defines what is considered normal diffusion. Historically, Einstein considered homogeneous diffusion characterised by a diffusion constant in his original calculations, resulting in what is known as Fickian diffusion, which thermally relaxes concentration inhomogeneities. However, in the same derivation of Einstein, the seed of generalisation of the theory to non-Fickian diffusion in the presence of space-dependent diffusivity is hidden. This indicates that non-Fickian diffusion, which can drive concentration inhomogeneities, can also be normal diffusion. The present article discusses the origin of the normal non-Fickian diffusion in Einstein's theory of diffusion.

Transcript

Introduction to the show: ident: Quantum Radio. Generated commentary on the latest quantum physics and condensed matter papers.

Kai: We're looking at the paper: "Einstein's theory of Brownian motion".

Mira: Here's the gist of the paper. The gist Einstein’s theory of Brownian motion can be generalized to include space-dependent diffusivity, revealing that non-Fickian diffusion is actually normal diffusion consistent with Einstein's postulates.

Kai: Einstein's Original Theory and Fickian Diffusion Albert Einstein provided the physical basis of Fickian diffusion in 1905, building on his theory of Brownian motion The local Fickian diffusion current density jF (r) is given by the equation jF (r, t) = −D∇C(r, t) Fickian diffusion is the phenomenon of thermal transport that relaxes concentration inhomogeneities in, for example, a collection of non-interacting particles that respond to thermal fluctuations at a constant temperature everywhere in space The diffusion constant is proportional to the ensemble-averaged squared displacement of a diffusing particle per unit time at the large time limit The Fickian diffusion current density as defined in eqn.(1), when combined with the conservation of particle number through the equation of continuity, gives us the well-known diffusion equation, as derived by Einstein, for the dynamics of the concentration under Fickian diffusive transport as ∂C(r) / ∂t = D∇2C(r) The solution of the diffusion equation (eqn.(2)), for an initial isotropic concentration at the position r = 0 being C(0) is C(r, t) = C(0) (4πDt) 3/2 exp − r / 2 4Dt Generalization to Space-Dependent Diffusivity The diffusion constant is proportional to the ensemble-averaged squared displacement of a diffusing particle per unit time at the large time limit In such a situation, non-Fickian diffusion arises essentially from Einstein’s theory of Brownian motion, and this aspect has not received detailed attention, probably due to our long-held notion that diffusion only relaxes concentration inhomogeneities, which is actually a special case The Fickian and non-Fickian (as described below) diffusion processes are consequences of the same theory of Brownian motion introduced by Albert Einstein, without altering any of the fundamental assumptions he set forth While Fickian diffusion relaxes concentration inhomogeneities because a constant diffusivity corresponds to an underlying homogeneous space, non-Fickian diffusion drives them because the diffusivity is space-dependent, reflecting the inhomogeneity of the underlying space in which the broken symmetry must show up in the transport process Mathematical Derivation of Inhomogeneous Diffusion When considering a jump distribution function position dependent, that is ϕ(x, ∆), eqn.(5) should be written as f(x, t + τ)dx = dx Z ∞ −∞ f(x + ∆)ϕ(x + ∆, ∆)d∆ Using the eqn.(10) in eqn.(9), and separating the integration on ∆ from the derivatives with x, we get the equation ∂f(x, t) / ∂t = ∂2 / ∂x2 D(x)f(x, t), where D(x) = R ∞ −∞ ∆2 2τ ϕ(x + ∆, ∆)d∆ The diffusion current density corresponding to the above equation is jdif f = −D(x) ∂f(x,t) / ∂x − f(x, t) / ∂D(x) ∂x Equilibrium Distributions and Interpretation The diffusion equation (12) will result in a steady state, equilibrium (when temperature is constant everywhere in space) distribution of particles C(x) ≡ feq(x) = α / D(x) In the presence of a not-so-strong conservative force F(x) = − ∂V (x) / ∂x, the equilibrium solution of the diffusion equation (12) will be feq(x) = (α/D(x))e −V (x)/kBT These equilibrium distributions, as shown in equation (14) and (15), that apparently defy our existing notion of diffusion as a process that evens out concentration inhomogeneities, whereas we see that diffusion, when inhomogeneous, drives them Underlying Symmetry and Conclusion The underlying reason that dictates normal diffusion cannot be solely a concentration-relaxing process The diffusivity (or equivalently, the damping coefficient) does not enter the Hamiltonian of a system Therefore, independent of the existence of any system in the otherwise homogeneous and isotropic space (in the absence of diffusion), the presence of diffusion characterises the underlying properties of the space in which the Hamiltonian of a system (when present) will introduce additional lifting of symmetries When diffusion becomes inhomogeneous, for whatever reason, an otherwise free particle experiences an underlying space whose homogeneity and isotropy are broken at large scales at which the diffusion is inhomogeneous The particle must respond asymmetrically in accordance with the underlying broken symmetry of space (which is actually due to a hidden thermal/mechanical/hydrodynamical origin), and diffusion in such a situation can drive concentration inhomogeneities This is a fundamental picture; when kept in mind, it can help us re-examine the long-held notion that normal diffusion only relaxes concentration inhomogeneities References

1: A.

Mira: Einstein, On the motion of small particles suspended in liquids at rest required by the molecular-kinetic theory of heat, Annalen der physik 17, 208 (1905)

2: G.

Kai: Crispin, Stochastic methods, in A Handbook for the Natural and Social Sciences, Springer Series in Synergetics, Vol.

Title and authors: Kai: So we're looking at this paper today titled "Einstein's theory of Brownian motion: The non-Fickian normal diffusion." It really dives into how what Einstein first described as simple Fickian diffusion can be extended to include things that aren't purely Fickian.

Mira: Exactly. It looks at how the theory of Brownian motion, which is super fundamental, naturally allows for space-dependent diffusivity without breaking those original postulates. It suggests that non-Fickian diffusion might actually just be a different flavor of normal diffusion consistent with Einstein’s math >

Lev: From my side, I’m curious about the actual experimental setup here. If we take this theory and try to build some kind of hardware, how much overhead are we talking for modeling that space-dependent D(x)? We need to make sure we can actually measure these effects in a real system >

Kai: Right. It starts by setting up the Fickian diffusion current density jF (r) as jF (r, t) = −D∇C(r, t), which is what we know from Einstein’s original work one <ref:2610.30194#pg1>. But the paper points out that this setup can be generalized to include a space-dependent diffusivity D(x) and still stay consistent with the core assumptions of Brownian motion two > <ref:2610.30194#pg1>

Mira: That's interesting because usually, when we move away from constant diffusion, we jump straight to anomalous diffusion, which implies something non-local or time-dependent in a way that doesn't fit Einstein’s original picture >

Lev: So what the paper is doing is showing that this non-Fickian behavior isn't an anomaly; it's just the natural consequence of having a spatially dependent diffusion constant D(x) reflecting an inhomogeneous space, not a new physical process >

Kai: It mentions that when you look at the jump distribution function position dependent, phi(x,), it leads to an equation where you get d f(x, t) / d t = d squared / d x squared D(x)f(x, t) > <ref:2610.30194#pg1>

Mira: And then they define the diffusion current density as jdif f = −D(x) ∂f(x,t) / d x − f(x, t) / d D(x) ∂x. That looks like a standard diffusion term mixed with something else because of that D(x), right >

Lev: If we were running this on real hardware, I’d be thinking about how the measurement precision for that current density jdif f would be affected by the spatial variation in D(x). It's going to require really high spatial resolution in our simulations or measurements to capture those differences accurately >

Kai: The paper then goes on to look at equilibrium distributions and says that under a constant temperature, you get C(x) f eq(x) = alpha / D(x) >

Mira: And if you have a conservative force F(x), which is the negative gradient of a potential V, then the equilibrium solution becomes f eq(x) = (alpha/D(x))e-V(x)/kBT >

Title and authors: Lev: That second form is what I’d need to simulate if we want to study systems under external potential gradients, like temperature variations or chemical potentials. It shows that diffusion is actively driving the particles in response to that gradient, which is a key distinction from just relaxing things out >

Kai: So the big point they are making here, concerning "Einstein's theory of Brownian motion: The non-Fickian normal diffusion," is that what we call non-Fickian diffusion doesn't necessarily mean anomalous behavior in this context >

Mira: It means the underlying mechanism is still rooted in Einstein’s basic postulates, but the space itself isn't uniform, which changes how concentration inhomogeneities behave >

Lev: So for someone building error correction hardware, it tells us that if we model transport on a non-uniform medium using this framework, we shouldn't assume it’s inherently anomalous unless the underlying physics forces that jump distribution phi to be something specific >

Kai: The paper argues that the reason normal diffusion can drive inhomogeneities is because the diffusivity itself doesn't enter the Hamiltonian of a system >

Mira: That’s a crucial assumption, because if diffusivity were part of the Hamiltonian, it would fundamentally change what we mean by normal transport and separate it from these underlying spatial symmetry properties >

Lev: If you can decouple that damping coefficient from the Hamiltonian, then even in a homogeneous space where there's no force F(x), diffusion alone can cause concentration changes, which is counter-intuitive to our standard view of equilibrium >

Kai: The implication for us is that when we look at complex systems, we need to check if the spatial variation in D(x) is just an effect of the geometry or a hidden symmetry breaking >

Mira: It shifts the focus away from just looking at concentration relaxation and pushes us toward understanding how the underlying space dictates what kind of transport happens >

Lev: For our hardware, this means we need to account for spatially varying D(x) if we are simulating things like grain drying or mass transport in polymers, because standard Fickian models will just give us the wrong answer when D is not constant >

Kai: So to wrap up this paper, "Einstein's theory of Brownian motion: The non-Fickian normal diffusion," it shows that normal diffusion can drive concentration inhomogeneities when the diffusivity depends on space >

Mira: It reframes non-Fickian diffusion not as a totally different process, but as a consequence of Einstein's original framework when the space itself is inhomogeneous >

Lev: Lev's final thought is that this theory gives us a way to understand that spatial inhomogeneity can break symmetries in the underlying space, and that’s what drives transport behavior >

Kai: That’s all we have for this paper today. We'll be back soon with more arXiv papers.

The paper's summary: Kai: So we’ve been looking at how Einstein’s original Brownian motion theory can be stretched to include things that aren't purely Fickian diffusion, and this paper says that what looks like non-Fickian diffusion is actually just normal diffusion under different conditions.

Mira: Exactly. They show that when you allow the diffusivity, D(x), to change depending on where you are in space, it doesn't break Einstein’s original assumptions; it just reflects an inhomogeneous space rather than a new type of physics >

Lev: From my side, the real question is how much overhead this spatial dependence adds to running something on real hardware. If we have a system with a spatially varying D(x), we need incredibly high spatial resolution in our simulations to capture that accurately, right?

Kai: Right. It starts by defining the Fickian current density jF (r) as being proportional to the negative gradient of concentration, but then they generalize it to include D(x), making it d f(x, t) / d t = d squared / d x squared D(x)f(x, t) >

Mira: And when you look at the steady state, the equilibrium distribution C(x) becomes alpha over D(x), and if there’s an external force F, it gets modified by that potential V term >

Lev: That second form is what I’d need to simulate if we want to study systems under external potential gradients, like temperature variations or chemical potentials. It shows diffusion is actively driving the particles in response to that gradient >

Kai: The paper argues that the reason normal diffusion can drive concentration inhomogeneities is because the diffusivity itself doesn't enter the Hamiltonian of a system >

Mira: That’s a crucial assumption because if diffusivity were part of the Hamiltonian, it would fundamentally change what we mean by normal transport and separate it from those underlying spatial symmetry properties >

Lev: If you can decouple that damping coefficient from the Hamiltonian, then even in a homogeneous space where there's no force F(x), diffusion alone can cause concentration changes, which is counter-intuitive to our standard view of equilibrium >

Kai: So for someone building error correction hardware, this means we need to account for spatially varying D(x) if we are simulating things like grain drying or mass transport in polymers, because standard Fickian models will just give us the wrong answer when D is not constant >

Mira: It shifts the focus away from just looking at concentration relaxation and pushes us toward understanding how the underlying space dictates what kind of transport happens >

Lev: For our hardware, this means we need to check if that spatial variation in D(x) is just an effect of the geometry or a hidden symmetry breaking >

Kai: So to wrap up this paper, it shows that normal diffusion can drive concentration inhomogeneities when the diffusivity depends on space >

Mira: It reframes non-Fickian diffusion not as a totally different process, but as a consequence of Einstein's original framework when the space itself is inhomogeneous >

Lev: Lev's final thought is that this theory gives us a way to understand that spatial inhomogeneity can break symmetries in the underlying space, and that’s what drives transport behavior >

Kai: So we’re looking at how this concept of space-dependent diffusion connects to other things we're working on, like how nonreciprocal systems handle spin transport.

The paper's improvements: Kai: We just talked about how space-dependent diffusion makes normal diffusion look different depending on where you are, and now we’re looking at what this paper suggests we should actually do with that knowledge >

Mira: Right. This paper isn't just describing a phenomenon; it's suggesting improvements to the model itself, specifically focusing on how we define and interpret these non-Fickian processes >

Lev: I’m interested in the practical side here. If we try to build this into an error correction system, what does this suggest about how much noise we can actually tolerate before it becomes intractable? Does it mean our current modeling assumptions are too simple? >

Kai: It suggests a way to make the simulation more robust by incorporating these space-dependent effects directly into the transport description, which is a step up from just using Fickian models that assume uniform D >

Mira: That’s right. They show how we can use this framework to predict equilibrium distributions exactly, including those driven by external conservative forces, which is a big deal for understanding particle movement in potentials >

Lev: So if I’m building hardware, this means we need to design our systems to account for those force-driven solutions rather than just looking at simple concentration relaxation >

Kai: It really points back to the underlying symmetry breaking in space, suggesting that these non-equilibrium transport phenomena are linked to how the geometry itself is structured >

Mira: And it reinforces that we should stop treating normal diffusion only as a way to even things out, because when D(x) changes, diffusion becomes an active driver of concentration gradients >

Lev: I’m still worried about the fidelity. If we introduce this complexity, how much does the required computational time increase for running simulations compared to the constant D case? That overhead is going to be significant >

Kai: The authors acknowledge that while this framework is more fundamental, implementing it accurately requires very specific spatial mapping and careful measurement of those D(x) values >

Mira: So for the broader physics community, the implication is that we need to look beyond just concentration transport and consider how space itself influences dynamics >

Lev: It tells me that if we want to model complex systems, we can’t just pick a constant diffusion coefficient; the geometry has to dictate it >

Kai: So this paper gives us a clearer picture of what non-Fickian normal diffusion actually is, and where the real physical challenges are now >

Conclusion: Tom: So we’re wrapping up this talk on "Einstein's theory of Brownian motion: The non-Fickian normal diffusion," and the main thing is that this paper shows how space-dependent diffusion, D(x), can drive concentration changes even when things are in equilibrium >

Kai: It really solidifies that non-Fickian behavior isn't some weird anomaly; it’s just the natural consequence of having an inhomogeneous space that Einstein’s theory already covers >

Mira: And the implication for us is that we need to think about how geometry breaks symmetries in space, which then dictates what kind of transport happens in a system >

Lev: From my point of view, it means when we build error correction systems on non-uniform materials, we can’t just use standard Fickian assumptions; we have to model that spatial dependence >

Kai: Exactly. It forces us to look at the Hamiltonian and see if the damping coefficient is independent of the system's energy terms or not >

Mira: That’s what I want you to keep in mind: whether you’re looking at a polymer or something else, if D(x) varies, that spatial variation needs to be accounted for in your theory >

Lev: It makes the simulation much harder because the overhead lands on resolution; we need better spatial mapping than we might think is practical for current hardware >

Kai: So, to sum up this paper on "Einstein's theory of Brownian motion: The non-Fickian normal diffusion," it’s a reminder that diffusion is more than just relaxing things out when the environment isn't uniform >

Mira: It reframes non-Fickian diffusion as a consequence of Einstein’s original framework when the space itself has some spatial structure >

Lev: I just think for hardware design, this means we need to be ready to account for those external potential gradients driving particles around, not just static concentration levels >

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