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Atlas / Physics / The Flow Thread

Field · Emerged 1738 – 1904

Fluid Dynamics

What equations govern a substance that has no fixed shape, and why do they so often refuse to be solved?

4 chapters6 min read6 turning points1 open problem

Branched from
Classical Mechanics
Branched into
Elasticity and Continuum Mechanics + Turbulence
Figures
Daniel Bernoulli, Jean le Rond d'Alembert, Leonhard Euler, Claude-Louis Navier, George Gabriel Stokes, Osborne Reynolds, Ludwig Prandtl

In brief

Newton's laws apply to a parcel of water as surely as to a planet, and writing them down for a continuous medium is not difficult: Euler did it in 1757, Navier and Stokes added internal friction by 1845, and the resulting equations have been believed ever since. They are also, for almost every case of interest, unsolvable. The nonlinear term that describes fluid carrying its own momentum couples every scale of motion to every other, and the consequence is that a subject with settled foundations spent two centuries unable to predict the drag on a sphere.

The field's most instructive episode is a paradox. In 1752 d'Alembert proved that a body moving steadily through an ideal fluid experiences no drag at all — a flat contradiction of every observation ever made, derived correctly from the accepted equations. The resolution took 152 years. Ludwig Prandtl showed in 1904 that however small the viscosity, it dominates in a thin layer at the surface, and that this layer determines the drag, the separation of the flow and the lift of a wing. Everything that matters happens in the part of the fluid that the idealisation discards.

Key ideas

Continuum hypothesisEnters 1757

Treat the fluid as a smooth field of density, velocity and pressure rather than as molecules. The approximation holds whenever the mean free path is far smaller than the scale of interest, which is almost always, and fails in rarefied gases and at the walls of microchannels.

Bernoulli's relationEnters 1738

Along a streamline in steady, frictionless flow, pressure falls where speed rises. It is energy conservation for a fluid parcel, and it is the first quantitative statement linking the two things one can measure about a flow.

ViscosityEnters 1822 – 1845

The internal friction by which a fluid resists shearing. It converts a kinematic problem into one with a diffusive term, supplies the condition that fluid sticks to a solid surface, and sets the scale on which velocity differences are smoothed out.

Reynolds numberEnters 1851

The ratio of inertial to viscous forces, Re=UL/ν\mathrm{Re} = UL/\nu. Two flows with the same Reynolds number behave identically whatever their size, which is why a model in a wind tunnel means anything; and whether Re\mathrm{Re} is 10−510^{-5} or 10810^{8} changes the physics completely.

Boundary layerEnters 1904

The thin region next to a solid surface in which the velocity rises from zero to that of the outer flow. Its thickness scales as L/ReL/\sqrt{\mathrm{Re}}, and it carries the drag, decides when flow separates, and is the reason the inviscid theory fails.

NonlinearityEnters 1822 – 1845

The term describing fluid advecting its own momentum is quadratic in the velocity, so solutions cannot be superposed and scales do not decouple. Nearly every unsolved problem in the subject traces back to this one term.

Draws on other domains

Chapter I

Newton's Laws for Something With No Shape

A solid has a shape to keep track of; a fluid does not, and the first problem is deciding what to apply the laws of motion to. The answer that worked was to stop tracking matter and track the field: at each point in space, a density, a pressure and a velocity, changing with time. Leonhard Euler wrote the equations in 1757, and they say exactly what Newton's second law says — the acceleration of the fluid at a point equals the force per unit mass acting there, which for an ideal fluid is the pressure gradient — plus the requirement that mass not appear or vanish.

Daniel Bernoulli had already extracted the most useful consequence, in 1738, before the general equations existed. Along a streamline in steady frictionless flow, pressure and speed trade off: speed up and the pressure drops. This is energy conservation for a fluid parcel, and it is the basis of the venturi, the pitot tube that tells an aircraft its airspeed, and a great many wrong explanations of lift.

What the Euler equations lacked was friction. Claude-Louis Navier supplied a term for it in 1822 by an argument about intermolecular forces that was wrong in its reasoning and right in its result; George Gabriel Stokes rederived it properly in 1845 from the assumption that internal stress depends linearly on the rate at which the fluid is being sheared, and added the condition that has done more work than any other in the subject: at a solid surface, the fluid does not slip. Its velocity there is zero.

Chapter II

The Paradox That Took 152 Years

Before the friction term existed, Jean le Rond d'Alembert had already derived something impossible. Solve the ideal-flow equations around a body moving at constant speed, and the pressure distribution comes out symmetric: whatever pushes back on the front pushes forward on the rear by exactly as much. The net force is zero. An ideal fluid offers no resistance.

Every rower, swimmer and sailor knew otherwise. D'Alembert said plainly that he could not explain it and left it "to geometers". The gap between theory and observation was not small — the theory predicted zero — and it split the subject in two for a century and a half. Mathematicians developed an elegant theory of ideal flow that engineers could not use; engineers compiled empirical tables of resistance with no theory behind them. Water, in the British physicist Horace Lamb's later account of the situation, was studied by one group and hydraulics by another, and the two did not meet.

Ludwig Prandtl closed it in 1904, in eight pages, with an argument about where an approximation fails. Viscosity is small for air and water, in the sense that the Reynolds number is large, so throwing the viscous term away looks safe. But the no-slip condition forces the velocity to zero at the surface while the outer flow is moving at full speed, which means the velocity gradient near the wall is enormous — and the viscous stress is proportional to that gradient. In a thin layer, viscosity is never negligible, however large the Reynolds number is. The layer gets thinner as Re\mathrm{Re} grows, and the stress in it does not vanish correspondingly.

Three consequences follow, and they are the whole of applied aerodynamics. The layer carries the skin-friction drag. The layer can separate from the surface when pressure rises downstream, at which point a large wake forms and the drag rises by an order of magnitude — the difference between a streamlined and a blunt body. And the way the layer leaves a wing's trailing edge fixes the circulation around the wing, which by the Kutta–Joukowski theorem fixes the lift.

Chapter III

A Closer Look: One Number Across Twelve Orders of Magnitude

Non-dimensionalise the Navier–Stokes equations for a flow of speed UU over an object of size LL in a fluid of kinematic viscosity ν\nu, and exactly one parameter survives:

Re=ULν=inertial forcesviscous forces.\mathrm{Re} = \frac{UL}{\nu} = \frac{\text{inertial forces}}{\text{viscous forces}}.

Two flows with the same Re\mathrm{Re} are the same flow, scaled. That is why a model tells you anything about an aircraft, and it is why a single number organises a subject that spans bacteria and hurricanes.

A car on a motorway. U=30U = 30 m/s, L=4L = 4 m, and for air ν=1.5×10−5\nu = 1.5\times10^{-5} m²/s:

Re=30×41.5×10−5=8×106.\mathrm{Re} = \frac{30 \times 4}{1.5\times10^{-5}} = 8\times10^{6}.

Prandtl's estimate puts the boundary layer thickness at roughly 5L/Re5L/\sqrt{\mathrm{Re}}:

δ≈5×48×106=202830=7 mm.\delta \approx \frac{5 \times 4}{\sqrt{8\times10^{6}}} = \frac{20}{2830} = 7 \text{ mm}.

Seven millimetres out of four metres. All of the friction drag, and the decision whether the flow separates behind the rear window, happens in that 0.2% of the length scale. This is why the inviscid theory can be simultaneously correct about the pressure field and useless about the force.

A swimming bacterium. U=30U = 30 µm/s, L=1L = 1 µm, and for water ν=10−6\nu = 10^{-6} m²/s:

Re=(3×10−5)(10−6)10−6=3×10−5.\mathrm{Re} = \frac{(3\times10^{-5})(10^{-6})}{10^{-6}} = 3\times10^{-5}.

Eleven orders of magnitude below the car. Inertia does not merely matter less; it does not exist. Ask how far such an organism coasts if it stops swimming. Its mass is about

m=43π(0.5×10−6)3×1000=5.2×10−16 kg,m = \tfrac{4}{3}\pi(0.5\times10^{-6})^{3} \times 1000 = 5.2\times10^{-16} \text{ kg},

and Stokes drag gives a friction coefficient 6πμa=6π(10−3)(0.5×10−6)=9.4×10−96\pi\mu a = 6\pi(10^{-3})(0.5\times10^{-6}) = 9.4\times10^{-9} kg/s. The coasting distance is mUmU divided by that coefficient:

(5.2×10−16)(3×10−5)9.4×10−9≈2×10−12 m,\frac{(5.2\times10^{-16})(3\times10^{-5})}{9.4\times10^{-9}} \approx 2\times10^{-12} \text{ m},

two picometres — a fiftieth of the width of an atom. A bacterium that stops beating its flagellum stops instantly and absolutely. It cannot glide, cannot throw anything, and cannot swim by any stroke that is merely reversed on the return, because at Re→0\mathrm{Re} \to 0 the equations are time-reversible and a reciprocal motion returns the organism exactly where it began. The corkscrew flagellum and the breaststroke-with-a-twist of a flagellate are solutions to a constraint that has no analogue at human scale.

Between the two lie everything else: Re≈102\mathrm{Re} \approx 10^{2} for a swimming tadpole, 10410^{4} for a sparrow, 10810^{8} for a whale, 10910^{9} for a weather system. The transition from the viscous regime to the inertial one is not a smooth loss of accuracy. Around Re≈2000\mathrm{Re} \approx 2000 in a pipe, steady flow stops being stable at all, and the subject changes into turbulence.

Chapter IV

What Is Settled and What Is Not

The foundations of this field have been secure for 180 years, which makes its unsolved problems unusual in character. Nobody doubts the Navier–Stokes equations; the question is whether they have solutions. For smooth initial data in three dimensions it has never been proved that the velocity stays finite — the nonlinear term pumps energy into ever smaller scales, viscosity removes it there, and whether dissipation always wins is open and carries a million-dollar prize. Two-dimensional flow is proved well behaved, which is of no comfort, since the world is not two-dimensional and the mechanism in question exists only in three.

This is an odd situation for an engineering science. Aircraft are certified using numerical solutions of equations that may, for all anyone can prove, develop infinities. In practice the computations agree with wind tunnels, and the agreement is the justification. How those computations are done, and why the cost grows so steeply with Reynolds number, belongs to numerical methods for partial differential equations and to the next field in this thread.

Applications

Where it is used

  • Aeronautics

    Lift, and why the usual explanation is wrong

    A wing's lift follows from the circulation around it, by the Kutta–Joukowski theorem of 1902–1906, and the circulation is established by the boundary layer leaving the trailing edge cleanly. The popular account — that air takes longer over the curved upper surface and therefore moves faster by Bernoulli — fails on inspection, since the parcels do not arrive together and a flat plate at an angle generates lift perfectly well.

    › Sources (2)
    • Anderson, J. D. (2016). Fundamentals of Aerodynamics, 6th edition. McGraw-Hill.
    • Babinsky, H. (2003). How do wings work? Physics Education 38: 497–503.
  • Physiology↗ Biology

    Blood through tubes that branch thirty times

    Flow in the larger arteries is pulsatile and inertial, while in capillaries 8 µm across the Reynolds number falls below 10−310^{-3} and viscosity rules entirely. Poiseuille's law, that resistance scales as the inverse fourth power of radius, is why a 20% narrowing of an artery more than doubles its resistance, and why the body regulates flow by changing vessel diameter.

    › Sources (2)
    • Poiseuille, J. L. M. (1846). Recherches expérimentales sur le mouvement des liquides dans les tubes de très petits diamètres. Mémoires des Savants Étrangers 9: 433–544.
    • Fung, Y. C. (1997). Biomechanics: Circulation, 2nd edition. Springer.
  • Engineering design

    Model testing and dynamic similarity

    Because flows with equal Reynolds number are the same flow, a scale model in a wind tunnel or towing tank predicts the behaviour of the full-size object — provided the number is matched, which usually means raising the speed or the pressure. The whole practice of experimental engineering design rests on this one dimensionless group, and on the recognition that where several groups matter at once, no single model can match them all.

    › Sources (1)
    • Barenblatt, G. I. (1996). Scaling, Self-Similarity, and Intermediate Asymptotics. Cambridge University Press.

Open problems

Where the map runs out

Open

Existence and smoothness for Navier–Stokes

Open as of 2026; one of the seven Clay Millennium Prize problems, unclaimed.

Given smooth initial data for an incompressible fluid in three dimensions, does a smooth solution exist for all time, or can the velocity become infinite somewhere in finite time? In two dimensions the answer is known to be yes. In three, only short-time existence and weak solutions of uncertain uniqueness have been proved, despite the equations being used every day to design aircraft.

Why it is hard

The nonlinear term transfers energy to ever smaller scales, and the viscous term removes it; whether dissipation always wins is exactly the question. The known conserved quantities do not control the right norms, so the standard route — find a quantity that stays bounded and conclude the solution stays smooth — has no candidate in three dimensions.

What resolving it unlocks

It would say whether turbulence is a feature of the equations or an artefact of our inability to solve them, and whether the computations that aircraft, reactors and weather forecasts rely on approximate something that exists.

› Sources (2)
  • Fefferman, C. L. (2006). Existence and smoothness of the Navier–Stokes equation. In The Millennium Prize Problems, 57–67. Clay Mathematics Institute.
  • Tao, T. (2016). Finite time blowup for an averaged three-dimensional Navier–Stokes equation. Journal of the American Mathematical Society 29: 601–674.

Further reading

  1. Darrigol, O. (2005). Worlds of Flow. Oxford University Press.

    The history from the Bernoullis to Prandtl, including how long the paradox was tolerated.

  2. Batchelor, G. K. (1967). An Introduction to Fluid Dynamics. Cambridge University Press.

    The standard rigorous text; careful about what the continuum assumption costs.

  3. Purcell, E. M. (1977). Life at low Reynolds number. American Journal of Physics 45: 3–11.

    Eleven pages on what the world is like for a swimming bacterium; the best short paper in the subject.