Forces & Fields Vol. 1 Pixel Sticker Sheet
7 Physics s
7 pixel-art physics stickers on one A5 (5.83″ × 8.27″) white kiss-cut sheet: Forces & Fields Vol. 1. Every character below has its own sticker page with the full physics panel.
Azurwake
A charged particle moving through a medium faster than light travels in that medium emits light in a cone, like a sonic boom. The cone angle depends on the particle's speed and the refractive index, and Frank and Tamm's formula gives how many photons come out per unit length.
cos θ = 1/(nβ), β > 1/n
θ: angle between the emitted light and the particle's path (the wavefront cone has half-angle 90° − θ) (rad); n: refractive index of the medium, about 1.33 for water; β: particle speed as a fraction of c; N: number of photons emitted; x: distance travelled by the particle (m); λ: wavelength of the emitted light (m)
Bremsella
Any accelerating charge radiates. Larmor's formula says the power grows with the square of the charge and the square of its acceleration, which is why electrons that slow down sharply in matter give off braking radiation.
P = q²a²/(6πε0c³)
P: power radiated by the accelerating charge (non-relativistic Larmor formula) (W); q: charge of the particle (C); a: magnitude of its acceleration (m/s²); ε₀: vacuum permittivity (F/m); c: speed of light (m/s)
Capacitwin
Charge one capacitor C to voltage V and join it to an identical empty one. Charge is conserved, so each ends at V/2 with half the charge. But the stored energy is now Q²/4C instead of Q²/2C: half the energy is gone. This holds however small the wire resistance is.
ΔE = ½ · C1C2/(C1 + C2) · (V1 − V2)²
ΔE: energy lost when the capacitors are joined (J); C1, C2: capacitances (F); V1, V2: starting voltages (V)
Diagonix
A polarizer passes the fraction cos²θ of already-polarized light. Two crossed polarizers block everything, but slip a third one between them at 45° and one-eighth of the original unpolarized light gets through.
I = I0 cos²θ
I: intensity after one ideal polariser (W/m²); I₀: intensity arriving (unpolarised for the three-polariser line) (W/m²); θ: angle between the light's polarisation and the polariser's transmission axis (rad); I_(out): intensity after the vertical, 45° and horizontal polarisers in turn (W/m²)
Gyrolla
A magnetic field bends a charged particle into a circle without changing its speed. Faster particles make bigger circles, but each lap takes the same time, so the cyclotron frequency depends only on charge, mass and field. That is what makes the cyclotron accelerator work.
r = mv/(qB)
q: charge of the particle (C); v: speed perpendicular to the field (m/s); B: magnetic flux density (T); m: mass of the particle (kg); r: radius of the circle (m); f_c: cyclotron frequency, laps per second (non-relativistic; at high energy it falls by 1/γ) (Hz)
Kibbla
A Kibble balance runs in two modes. In weighing mode, a current I in a coil sitting in a radial magnetic field pushes up with force BLI, balancing the weight mg. In moving mode, the same coil is moved at speed v and a voltage U = BLv is induced. The hard-to-measure product BL cancels between the two, leaving a match between mechanical and electrical power.
mgv = UI
m: test mass (kg); g: local gravitational acceleration (m/s²); v: coil velocity (m/s); U: induced voltage (V); I: coil current (A)
Lenzor
A changing magnetic flux induces a voltage, and the induced current always flows so as to oppose the change. A magnet dropped through a copper pipe therefore drives eddy currents that brake it, so it drifts down at a steady terminal speed.
ℰ = −dΦB/dt
mathcalE: EMF induced around one ring of the pipe (V); Φ_B: magnetic flux through that ring (Wb); t: time (s); m: mass of the falling magnet (kg); g: gravitational acceleration (m/s²); F_(eddy): upward drag from the eddy currents; it grows with the magnet's speed (N)
Shipping calculated at checkout by destinationMade to order, ships in 2–5 business days
Details
What you getA5 sheet
One A5 kiss-cut sheet (5.83″ × 8.27″) on white sticker paper, made to order.
ShippingBy destination
Shipping calculated at checkout by destination.
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.
The physics
Equations
| Symbol | Meaning | Unit |
|---|---|---|
| \(n\) | Azurwake: refractive index of the medium, about 1.33 for water | \(\mathrm{1}\) |
| \(\beta\) | Azurwake: particle speed as a fraction of c | \(\mathrm{1}\) |
| \(P\) | Bremsella: power radiated by the accelerating charge (non-relativistic Larmor formula) | \(\mathrm{W}\) |
| \(q\) | Bremsella: charge of the particle | \(\mathrm{C}\) |
| \(a\) | Bremsella: magnitude of its acceleration | \(\mathrm{m/s^2}\) |
| \(c\) | Bremsella: speed of light | \(\mathrm{m/s}\) |
| \(\Delta E\) | Capacitwin: energy lost when the capacitors are joined | \(\mathrm{J}\) |
| \(C_1, C_2\) | Capacitwin: capacitances | \(\mathrm{F}\) |
| \(V_1, V_2\) | Capacitwin: starting voltages | \(\mathrm{V}\) |
| \(I\) | Diagonix: intensity after one ideal polariser | \(\mathrm{W/m^2}\) |
| \(I_0\) | Diagonix: intensity arriving (unpolarised for the three-polariser line) | \(\mathrm{W/m^2}\) |
| \(\theta\) | Diagonix: angle between the light's polarisation and the polariser's transmission axis | \(\mathrm{rad}\) |
| \(q\) | Gyrolla: charge of the particle | \(\mathrm{C}\) |
| \(v\) | Gyrolla: speed perpendicular to the field | \(\mathrm{m/s}\) |
| \(B\) | Gyrolla: magnetic flux density | \(\mathrm{T}\) |
| \(m\) | Gyrolla: mass of the particle | \(\mathrm{kg}\) |
| \(r\) | Gyrolla: radius of the circle | \(\mathrm{m}\) |
| \(m\) | Kibbla: test mass | \(\mathrm{kg}\) |
| \(g\) | Kibbla: local gravitational acceleration | \(\mathrm{m/s²}\) |
| \(v\) | Kibbla: coil velocity | \(\mathrm{m/s}\) |
| \(U\) | Kibbla: induced voltage | \(\mathrm{V}\) |
| \(I\) | Kibbla: coil current | \(\mathrm{A}\) |
| \(\mathcal{E}\) | Lenzor: EMF induced around one ring of the pipe | \(\mathrm{V}\) |
Sources
- Cherenkov (1934) Visible emission of clean liquids by action of γ radiation, Dokl. Akad. Nauk SSSR 2, 451 — reprinted in Usp. Fiz. Nauk 93, 385 (1967) (opens in a new tab)
- Frank & Tamm (1937) Coherent visible radiation of fast electrons passing through matter, Dokl. Akad. Nauk SSSR 14, 109 — reprinted in Usp. Fiz. Nauk 93, 388 (1967) (opens in a new tab)
- NobelPrize.org — The Nobel Prize in Physics 1958 (Cherenkov, Frank and Tamm) (opens in a new tab)
- Encyclopaedia Britannica — Cherenkov radiation (opens in a new tab)
- NobelPrize.org — Pavel A. Cherenkov, Biographical (1934 observation while working under S. I. Vavilov; Lebedev Institute of Physics) (opens in a new tab)
- Larmor, J. (1897) On a dynamical theory of the electric and luminiferous medium, Phil. Mag. 44, 503
- Jackson, J. D., Classical Electrodynamics, 3rd ed., Ch. 14 (Larmor formula) and Ch. 15 (bremsstrahlung)
- Wikipedia, Bremsstrahlung (opens in a new tab)
- R. A. Powell (1979) Two-capacitor problem: A more realistic view, Am. J. Phys. 47, 460 (opens in a new tab)
- Encyclopaedia Britannica — Étienne-Louis Malus (1809 paper on the polarization of light by reflection) (opens in a new tab)
- Feynman Lectures on Physics Vol. I Ch. 33: Polarization (opens in a new tab)
- Lawrence & Livingston (1932) The Production of High Speed Light Ions Without the Use of High Voltages, Phys. Rev. 40, 19 (opens in a new tab)
- NobelPrize.org — The Nobel Prize in Physics 1939 (Ernest Lawrence, for the invention and development of the cyclotron) (opens in a new tab)
- NIST CODATA — proton charge to mass quotient e/m_p (gives f/B = 15.245 MHz/T) (opens in a new tab)
- I. A. Robinson & S. Schlamminger (2016) The watt or Kibble balance: a technique for implementing the new SI definition of the unit of mass, Metrologia 53, A46 (opens in a new tab)
- Lenz (1834) Ueber die Bestimmung der Richtung der durch elektrodynamische Vertheilung erregten galvanischen Ströme, Ann. Phys. 107, 483–494 (opens in a new tab)
- MacLatchy, Backman & Bogan (1993) A quantitative magnetic braking experiment, Am. J. Phys. 61, 1096 (opens in a new tab)
- Feynman Lectures on Physics Vol. II Ch. 17: The Laws of Induction (opens in a new tab)
- Encyclopaedia Britannica — Faraday’s law of induction (Faraday’s observations of 1831) (opens in a new tab)
- Encyclopaedia Britannica — Lenz’s law (deduced in 1834 by the Russian physicist H. F. E. Lenz; conservation of energy) (opens in a new tab)