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Optional unit · institution-dependent · Interactive lesson

Landau's criterion and frictionless flow of a Bose gas

Why can an obstacle cross a Bose condensate without drag when a perfect gas of the same atoms cannot? One Galilean transformation turns the question into a race between the obstacle's speed and the cheapest energy per unit momentum the fluid sells, and Bogoliubov's phonons set that price at the speed of sound.

UAQM-15.09 · Lesson 9 of 9 in this unit. Position is not a completion score.
Starting model: Landau's criterion and frictionless flow of a Bose gasEnergy per unit momentum Eₖ/ħk of a sodium condensate's excitations against k. At aₛ = 2.75 nm and n = 1.0 × 10²⁰ m⁻³ the Bogoliubov curve bottoms out at c = 5.14 mm s⁻¹; the ideal-gas line starts at zero. At v = 7.5 mm s⁻¹ the obstacle can emit every k where the flat line lies above a curve, marked by the filled bar (interacting) and open bar (ideal).solid: Bogoliubov Eₖ/ħk, in mm s⁻¹dot: its minimum, c = 5.14 mm s⁻¹dashed: ideal gas ħk/2m, minimum 0flat line: v, bars: bands of k emitted510036k / μm⁻¹
Start with a picture. Change the model in the lab below.

Optional unit · institution-dependent. Units 14 and 15 are the course’s optional extension into open systems and quantum gases. Unit 14 builds on radiation and decay; Unit 15 builds on second quantisation. Keep the fifteen-unit numbering and follow your institution’s required syllabus. Optional work is not a required completion gate.

1

Build the model

Friction needs an excitation the obstacle can afford. Below c, a Bose gas offers none.

The key idea

Landau's criterion: a weak obstacle moving at speed v through a uniform fluid at zero temperature can create elementary excitations, and so feel drag, only if v exceeds vc, the minimum over all k of the energy per unit momentum Eₖ/(ħk) of those excitations.

Example. For sodium with n = 1.0 × 10²⁰ m⁻³ and aₛ = 2.75 nm, Bogoliubov's spectrum gives vc = c = √(gn/m) = 5.1 mm s⁻¹: a weak laser beam swept at 3 mm s⁻¹ creates nothing, whereas in the ideal gas vc = 0.

The complete physical model and assumptions

At zero temperature a fluid can take energy from a moving obstacle only by creating excitations, and energy and momentum together decide whether it may. Seen from the obstacle, a Galilean transformation shifts every excitation's energy from Eₖ to Eₖ − ħk⋅v, and a static obstacle can only create what costs nothing there, which needs v ≥ Eₖ/(ħk). Dissipation therefore begins at Landau's critical velocity vc, the minimum over k of the energy per unit momentum, a number fixed by the spectrum alone. That one line overturns a natural belief. The ideal condensate, every atom in k = 0, has Eₖ/(ħk) = ħk/2m, whose minimum is zero, so it is not a superfluid. Repulsion reshapes the low-k spectrum: Bogoliubov's phonons cost c = √(gn/m) per unit momentum, so the dilute gas carries a weak obstacle without friction below the speed of sound, and the golden rule turns the kinematics into a drag that switches on as (v − c)². The model stops where its assumptions do. It counts only small excitations of a uniform fluid at T = 0. Large obstacles nucleate quantised vortices, non-linear solutions of the Gross-Pitaevskii equation outside Bogoliubov's spectrum, so measured critical velocities usually fall below vc; and in liquid helium, beyond Bogoliubov theory, the measured roton minimum puts vc near 58 m s⁻¹, a quarter of its sound speed.

1Energy and momentum seen from the obstacle

SI units throughout; the physics is Galilean, so no metric signature enters. View N atoms of mass m from a frame moving at velocity v. Every momentum shifts, pᵢ → pᵢ − mv, while the interactions depend only on separations, so a state of total momentum P and energy E has P′ = P − Nmv and E′ = E − P⋅v + ½Nmv² there (derived). Apply it to the gas at rest: the ground state has P = 0, and one excitation adds momentum ħk and energy Eₖ, so in the obstacle's frame that excitation costs Eₖ − ħk⋅v, the ½Nmv² being common to both states. There the obstacle is a static potential: it absorbs any momentum but supplies no energy, so it can create only excitations with Eₖ − ħk⋅v = 0. Such a k exists whenever Eₖ − ħk⋅v is negative for some k, Landau's form of the condition, because turning k away from v raises the value continuously to Eₖ > 0. The lab frame agrees: an obstacle of mass M that hands ħk to the gas loses ħk⋅v − ħ²k²/2M of kinetic energy, which must pay Eₖ, and M → ∞ leaves Eₖ = ħk⋅v.

2The threshold is a property of the spectrum alone

Since ħk⋅v ≤ ħkv, the equation Eₖ = ħk⋅v has a solution for some direction only if v ≥ Eₖ/(ħk). Dissipation therefore starts at vc = min over k of Eₖ/(ħk), Landau's critical velocity (derived). On a plot of E against p = ħk it is the slope of the steepest line through the origin that never rises above the curve. Making several excitations at once does no better, because ΣEᵢ ≥ vc Σ|ħkᵢ| ≥ vc|Σħkᵢ|: below vc nothing at all can be created, at T = 0, by a weak obstacle of any shape. Above vc each allowed excitation leaves at cos θₖ = Eₖ/(ħkv) to the direction of motion, a cone like Cherenkov radiation. Be clear what the criterion is. It is kinematics, a necessary condition for dissipation that says nothing about how strongly the obstacle couples, and it is blind to anything that is not an elementary excitation of the uniform fluid at rest.

3The ideal condensate is not a superfluid

Switch the interactions off. The excitations are atoms kicked out of k = 0, with Eₖ = ħ²k²/2m, so Eₖ/(ħk) = ħk/2m, which falls to zero as k → 0: vc = 0 (derived). At any speed the obstacle can kick atoms onto the sphere k = (2mv/ħ)cos θ, so every k up to 2mv/ħ is open. For sodium ħ/m = 2.76 × 10⁻⁹ m² s⁻¹, and at v = 1.0 mm s⁻¹ the band reaches k = 7.2 × 10⁵ m⁻¹: wavelengths of 8.7 μm and longer, which fit easily in a cloud tens of micrometres across. Macroscopic occupation of one state does not by itself stop friction. An ideal condensate pushed through a rough pipe would be slowed atom by atom, each kick costing an energy per unit momentum as small as you please. What has to change is the price of the cheapest excitation per unit momentum, and only the interactions can raise it.

4Bogoliubov's phonons put the threshold at the sound speed

The previous lesson derived Eₖ = √(εₖ(εₖ + 2gn)), with εₖ = ħ²k²/2m and g = 4πħ²aₛ/m; both are used here, not re-derived. Divide by ħk: Eₖ/(ħk) = √(c² + (ħk/2m)²) with c = √(gn/m). This rises monotonically from c at k → 0, so vc = c (derived): the linear phonon branch is exactly what holds the threshold off zero, and the free-particle tail only climbs higher. Checks: [gn/m] = (J m³)(m⁻³)/kg = m² s⁻², a squared speed, and g → 0 returns the ideal gas's vc = 0. For sodium with n = 1.0 × 10²⁰ m⁻³ and aₛ = 2.75 nm, g = 1.01 × 10⁻⁵⁰ J m³ and c = 5.1 mm s⁻¹, while n aₛ³ = 2.1 × 10⁻⁶ ≪ 1 keeps Bogoliubov's theory safe. The measured number is quoted: in 1997 Andrews, Ketterle and co-workers at MIT launched density pulses along a sodium condensate and filmed them, finding speeds of several mm s⁻¹ that rose with density as √n, as c = √(gn/m) predicts.

5The golden rule turns the threshold into a drag force

Let a weak, heavy point obstacle, U = gᵢδ(r − vt), cross the gas. It couples to the density, whose Fourier component ρ̂ₖ = Σₚ a†ₚ₊ₖaₚ adds momentum ħk and creates one Bogoliubov excitation with |⟨1ₖ|ρ̂ₖ|0⟩|² = N₀εₖ/Eₖ, a factor that makes long phonons couple weakly. The golden rule gives each k a rate (2π/ħ)(gᵢ/V)²N₀(εₖ/Eₖ)δ(Eₖ − ħk⋅v), and the δ-function is Landau's criterion. Sum ħk times this rate over k: the angular integral fixes cos θ = Eₖ/(ħkv), the radial one stops at kₘₐₓ, and F = nσmv²(1 − c²/v²)² for v > c, F = 0 below (derived, with n₀ ≈ n), where σ = m²gᵢ²/(πħ⁴) is the Born cross-section for an atom on the obstacle. Checks: nσmv² is (m⁻³)(m²)(kg)(m² s⁻²) = N, and c → 0 gives the ideal gas, nσv collisions per second each taking mv on average. Measured (quoted): in 2000 the MIT group made impurity atoms inside a sodium condensate with a Raman pulse and saw their collisions strongly suppressed below the sound speed.

6Where the criterion overestimates: helium and vortices

Liquid helium-4 lies outside Bogoliubov theory, being dense and under 10 per cent condensed, but Landau's criterion needs only the spectrum, which neutron scattering measures (quoted): phonons at c = 238 m s⁻¹ and a roton minimum Δ/kB = 8.6 K at p₀/ħ = 1.91 Å⁻¹, with effective mass μ = 0.16 m₄. The steepest line from the origin that stays under the roton branch, E = Δ + (p − p₀)²/2μ, touches it at p = √(p₀² + 2μΔ), giving vc = 58 m s⁻¹ (derived from those quoted numbers), a quarter of c. Experiment is lower still: superflow through channels and films breaks down at mm s⁻¹ to tens of cm s⁻¹, and condensates stirred by a laser heat well below c. Landau counted only small excitations of a uniform fluid; a large obstacle can instead nucleate a quantised vortex, a non-linear object of circulation h/m and core size ξ. Potential flow round a cylinder already reaches 2v at its flanks, where the obstacle also thins the gas and lowers the local c. The Gross-Pitaevskii equation, iħ∂ψ/∂t = (−ħ²∇²/2m + U + g|ψ|²)ψ, describes these vortices; it is named here, not solved.

2

Key equations

Read the units, assumptions and limits before substituting.

Galilean shift of an excitation's energy

E′ = Eₖ − ħk⋅v

Derived. E′ is what the excitation costs in the obstacle's frame, where a static obstacle supplies no energy, so only excitations with E′ = 0 can appear.

Eₖ: excitation energy in the gas frame (J); ħk: its momentum (kg m s⁻¹); v: obstacle velocity (m s⁻¹)

Landau's critical velocity

vc = min over k of Eₖ/(ħk)

Derived. Below vc no excitation, single or several, is kinematically allowed at T = 0, whatever the weak obstacle's shape or strength.

the smallest energy per unit momentum in the spectrum (m s⁻¹), set by the fluid alone

Ideal Bose gas: no threshold

Eₖ/(ħk) = ħk/2m → 0 as k → 0, so vc = 0

Derived. A condensate without interactions dissipates at any speed, into every k below 2mv/ħ.

m: atomic mass (kg); excitations are free atoms with Eₖ = ħ²k²/2m

Bogoliubov gas: threshold at the sound speed

vc = c = √(gn/m), with g = 4πħ²aₛ/m

Derived from Eₖ/(ħk) = √(c² + (ħk/2m)²), which rises from c at k → 0; the spectrum and g = 4πħ²aₛ/m are quoted from the previous lesson. Sodium at 1.0 × 10²⁰ m⁻³: c = 5.1 mm s⁻¹.

n: density (m⁻³); g: contact coupling (J m³); aₛ: s-wave scattering length (m)

Emission band above threshold

0 < k < kₘₐₓ = (2m/ħ)√(v² − c²)

Derived from Eₖ/(ħk) < v. The band opens at k = 0 when v reaches c, so the first excitations made are the longest phonons.

v > c: obstacle and sound speeds (m s⁻¹); kₘₐₓ: largest wavenumber that can be emitted (m⁻¹)

Drag on a weak point obstacle

F = nσmv²(1 − c²/v²)² for v > c, F = 0 for v < c

Derived by the golden rule with n₀ ≈ n. At c → 0 it is the ideal gas's collisional drag nσmv²; just above c it grows only as (v − c)².

σ = m²gᵢ²/(πħ⁴): Born cross-section (m²) of an atom on the obstacle, coupling gᵢ (J m³); F in N
3

Interactive lab

Predict first. Explore the model. Compare the result.

Explore the model

2.75 nm
0 to 5 nm; steps of 0.25.
1.0 10²⁰ m⁻³
0.2 to 3 10²⁰ m⁻³; steps of 0.2.
7.5 mm s⁻¹
0.5 to 12 mm s⁻¹; steps of 0.5.

Try this. At v = {v|1} mm s⁻¹ the drag is {max(1-9.58947*as*n/max(v²,0.01),0)²|3} of the ideal gas's. Lower v below the dot and the filled bar vanishes, the open bar never. Then set aₛ to 0: the solid curve falls onto the dashed line and the ideal condensate dissipates at every speed.

Live results

CRITICAL SPEED c
5.14 mm s⁻¹
LARGEST k EMITTED
3.96 μm⁻¹
DRAG / IDEAL-GAS DRAG
0.282
DILUTENESS n aₛ³
2.08 × 10⁻⁶

Results follow this lesson’s model and assumptions. Displayed values are rounded.

Interactive Advanced Quantum Mechanics modelEnergy per unit momentum Eₖ/ħk of a sodium condensate's excitations against k. At aₛ = 2.75 nm and n = 1.0 × 10²⁰ m⁻³ the Bogoliubov curve bottoms out at c = 5.14 mm s⁻¹; the ideal-gas line starts at zero. At v = 7.5 mm s⁻¹ the obstacle can emit every k where the flat line lies above a curve, marked by the filled bar (interacting) and open bar (ideal).solid: Bogoliubov Eₖ/ħk, in mm s⁻¹dot: its minimum, c = 5.14 mm s⁻¹dashed: ideal gas ħk/2m, minimum 0flat line: v, bars: bands of k emitted510036k / μm⁻¹
Energy per unit momentum Eₖ/ħk of a sodium condensate's excitations against k. At aₛ = 2.75 nm and n = 1.0 × 10²⁰ m⁻³ the Bogoliubov curve bottoms out at c = 5.14 mm s⁻¹; the ideal-gas line starts at zero. At v = 7.5 mm s⁻¹ the obstacle can emit every k where the flat line lies above a curve, marked by the filled bar (interacting) and open bar (ideal).

Predict → change one variable → check

Plan a change before running it. Every other input stays at the saved baseline.

Saved baseline. Scattering length aₛ: 2.75 nm; Density n: 1.0 10²⁰ m⁻³; Obstacle speed v: 7.5 mm s⁻¹

Baseline 2.75; choose 0 to 5, in steps of 0.25.
4. Compared with the saved baseline, this result will…

This experiment is kept only while this page is open. It does not change saved course progress.

4

Catch the common trap

Bose-Einstein condensation is not superfluidity. It is tempting to think that atoms piled into k = 0 are locked in one state and cannot be scattered, so any condensate flows without friction. The ideal condensate refutes this: kicking one atom from k = 0 to k costs ħ²k²/2m, an energy per unit momentum ħk/2m that tends to zero, so an obstacle at any speed can make such kicks, into every k below 2mv/ħ. What forbids dissipation is the shape of the spectrum, and interactions change it: the pair terms turn the cheapest excitations into phonons costing c per unit momentum. Nor does superfluidity need a large condensate. Helium-4, under 10 per cent condensed, has vc ≈ 58 m s⁻¹ from its roton minimum.

5

Practice & worked examples

3 authored examples. Make an attempt, then reveal the reasoning one step at a time.

EasyExample 1

A rubidium-87 condensate (m = 1.443 × 10⁻²⁵ kg, aₛ = 5.3 nm) has uniform density 1.5 × 10²⁰ m⁻³ at T = 0. A weak, narrow laser beam is swept through it at 1.5 mm s⁻¹. Can the beam create excitations? Compare with an ideal gas of the same atoms.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 5 steps revealed.

MediumExample 2

A sodium condensate (m = 3.818 × 10⁻²⁶ kg) with n = 1.0 × 10²⁰ m⁻³ and aₛ = 2.75 nm is crossed by a weak obstacle at 7.5 mm s⁻¹. Find the band of wavenumbers it can emit, its shortest wavelength against the healing length, and the emission angles of the longest phonons and of k = kₘₐₓ/2.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 5 steps revealed.

HardExample 3

A heavy impurity crosses a sodium condensate with n = 1.0 × 10²⁰ m⁻³ and c = 5.135 mm s⁻¹. Its Born scattering length with a sodium atom is aᵢ = 3.0 nm. Using the golden-rule drag, find the drag at 7.5 mm s⁻¹ against an ideal gas of the same density, the speed at which it is half the ideal-gas value, and the speed at which it first reaches 1 per cent of it.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 5 steps revealed.

6

Quick check

Select an answer and explain it before checking.

Consider a weak, heavy impurity moving at 3.0 mm s⁻¹ through a uniform sodium condensate at T = 0 whose Bogoliubov sound speed is 5.1 mm s⁻¹. Which statement is correct?
7

Review & continue

Landau's criterion: a weak obstacle moving at speed v through a uniform fluid at zero temperature can create elementary excitations, and so feel drag, only if v exceeds vc, the minimum over all k of the energy per unit momentum Eₖ/(ħk) of those excitations.

  • Explain the relationship without looking at the equation.
  • Check a sign, a unit and a model assumption in your working.
  • Return to the lab or worked example if a step is still unclear.

Extra challenging questions

Connect several ideas, explore supplied data, and compare your reasoning with a worked solution.