• White Levitah physics T-shirt, front view (flat-lay mockup), view 1

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Levitah

Held by Sound Physics

\[U = \frac{4\pi}{3}a^{3}\left[f_1\,\tfrac{1}{2}\kappa_0\langle p^{2}\rangle - f_2\,\tfrac{3}{4}\rho_0\langle v^{2}\rangle\right]\]
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Size guide S–5XL · inches

Levitah holds a row of pearls still in mid-air, caught in a column of sound no one can see.

The Physics

Sound carries momentum, and a strong standing wave exerts a steady average force, the acoustic radiation force, on small objects. King computed it for spheres in 1934. Gor'kov (1962) wrote it, for a sphere much smaller than the wavelength in an ideal fluid, as the gradient of a potential U, with a compressibility factor f₁ and a density factor f₂.

For a small bead much denser and much less compressible than air (ρ_p ≫ ρ₀, κ_p ≪ κ₀), both factors are close to 1. U is then lowest where the pressure amplitude vanishes and the velocity amplitude peaks, so the bead collects near the pressure nodes, which are the velocity antinodes, half a wavelength apart. At 40 kHz in air the wavelength is about 8.6 mm, so the trapping sites are about 4.3 mm apart.

U = (4π/3) a³ [ f₁ · ½ κ₀ ⟨p²⟩ − f₂ · ¾ ρ₀ ⟨v²⟩ ], F = −∇U

  • U: radiation potential (J)
  • a: sphere radius, a ≪ wavelength (m)
  • f₁ = 1 − κ_p/κ₀: compressibility contrast
  • f₂ = 2(ρ_p − ρ₀)/(2ρ_p + ρ₀): density contrast
  • κ₀, ρ₀: compressibility and density of the air
  • ⟨p²⟩, ⟨v²⟩: time-averaged squared acoustic pressure and velocity

King, Proc. R. Soc. Lond. A 147, 212 (1934); Gor'kov, Sov. Phys. Dokl. 6, 773 (1962).

Honest caveat: It is not anti-gravity, and it does not work on any object: size and density limits apply. Dense, rigid beads collect near pressure nodes (velocity antinodes), not at velocity nodes; in a vertical levitator gravity holds each bead slightly below its node.

On the shirt

Front: Levitah, the pixel-art character, with “HELD BY SOUND”. Back: Gor'kov's potential, the force, the pressure-node rule, the 40 kHz spacing and the 1934 and 1962 sources. Printed on a unisex tee.

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Details

Size & fitS–5XL

Unisex heavy cotton (Gildan 5000), classic fit.

Unisex tee size chart, inches
SizeWidthLengthSleeve
S182815.1
M202916.5
L223018
XL243119.5
2XL263221
3XL283322.4
4XL303423.7
5XL323525

Para ter uma escala: o tamanho M tem 20 in (50.80 cm) de largura, cerca de 3.143 × 1034 comprimentos de Planck (lP = 1.616255 × 10−35 m). Uma fita métrica é mais rápida.

Measurements in inches, ±1.5 in tolerance.

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Shipping calculated at checkout by destination. Printed to order for you.

Delivery times & where we ship

Returns & replacements21 days

Every item is printed to order, so we can’t accept returns or exchanges for change of mind, or if you ordered the wrong size or colour.

Print defect, misprint, damage or the wrong item? We’ll send a free replacement, or a refund if you prefer. Report it within 21 days of delivery with a photo; no need to send it back.

Full refund & replacement policy

The physics

I hold beads in mid-air with nothing but sound.

A standing sound wave pushes on a small sphere with a steady radiation force. Lev Gor'kov packaged it in 1962 as a potential, U, set by the time-averaged squares of pressure and air velocity; the force is −∇U, valid for spheres much smaller than the wavelength. Louis King had worked out the force on spheres in 1934. For dense, stiff beads in air the pressure term wins, and they settle near the pressure nodes, half a wavelength apart.

At 40 kHz in air the wavelength is about 8.6 mm, so the nodes sit about 4.3 mm apart. It is not anti-gravity, and it does not work on just anything: size and density both matter.

Equations

\[U = \frac{4\pi}{3}a^{3}\left[f_1\,\tfrac{1}{2}\kappa_0\langle p^{2}\rangle - f_2\,\tfrac{3}{4}\rho_0\langle v^{2}\rangle\right]\]
\[\mathbf{F} = -\nabla U \qquad (a \ll \lambda)\]
\[40\ \mathrm{kHz\ in\ air:}\ \lambda \approx 8.6\ \mathrm{mm},\ \text{nodes } 4.3\ \mathrm{mm}\ \text{apart}\]
Symbols
SymbolMeaningUnit
\(U\) acoustic radiation potential (Gor'kov) \(\mathrm{J}\)
\(a\) sphere radius \(\mathrm{m}\)
\(f_1,\ f_2\) monopole and dipole scattering coefficients \(\mathrm{1}\)
\(\kappa_0\) compressibility of the air \(\mathrm{1/Pa}\)
\(\langle p^{2}\rangle\) time-averaged squared acoustic pressure \(\mathrm{Pa²}\)
\(\rho_0\) density of the air \(\mathrm{kg/m³}\)
\(\langle v^{2}\rangle\) time-averaged squared acoustic velocity \(\mathrm{m²/s²}\)
\(\mathbf{F}\) radiation force on the sphere \(\mathrm{N}\)
\(\lambda\) wavelength \(\mathrm{m}\)