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The Physicists Sticker Sheet

Newton, Curie, Tesla, Feynman & Hawking | 5 Pixel Art s

\[\vec F = \frac{d\vec p}{dt}\]
$19.99 USD
$19.99 USD
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Five pixel-art physicist stickers on one A5 kiss-cut sheet: Isaac Newton, Marie Curie, Nikola Tesla, Richard Feynman and Stephen Hawking. Each sticker is a small piece of real physics, drawn in pixels. Peel one for your laptop, notebook or bottle; the physics panel below has every equation, symbol and source.

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What you getA5 sheet · 5 stickers

One A5 kiss-cut sheet (5.83″ × 8.27″) on white sticker paper with 5 stickers, made to order.

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The physics

Five physicists, five rules: Newton's laws of motion and gravity, Curie's exponential radioactive decay, Tesla's transformer ratio, Feynman's sum over paths, and Hawking's black-hole temperature. Each line on the sheet is the key equation of one sticker.

Five stickers on one sheet. Five physicists, and the equations that still run the world, or at least argue about it.

Newton's line is Gravity Hits Different. The force he published in the Principia in 1687 is here as universal gravitation: every mass pulls every other mass. Written F = G m1 m2 / r², falling apples and orbiting moons become the same problem. The companion formula is the second law as a rate of change of momentum, the form that still works when F = ma does not.

Curie's line is She Literally Glowed Up. The glow was radium's. In 1898 she and Pierre announced polonium and radium; she shared the 1903 Nobel in Physics and took Chemistry alone in 1911, the first person with two Nobels and still the only one across two sciences. The exponential decay law on this page came soon after, from Rutherford and Soddy in 1902, built on measurements like hers.

Tesla's line is AC Slays DC. His 1888 polyphase patents made alternating current useful at the motor end; the transformer ratio here is why AC could travel far while steady DC of the day could not. It was Westinghouse's company, not Tesla alone, that fought Edison's direct-current interests.

Feynman's line is Quantum? It's Complicated. In 1948 he summed amplitudes over every path a particle might take. Square the total and you get a probability. He shared the 1965 Nobel with Tomonaga and Schwinger for quantum electrodynamics.

Hawking's line is Black Holes? Been There, Bent That. In 1974 he showed that black holes should radiate with a temperature inversely proportional to mass. That radiation has not been seen from an astrophysical black hole. Whether information survives evaporation is still open.

Five faces. Five formulas. Peel carefully.

Equations

\[\vec F = \frac{d\vec p}{dt}\]
\[F = \frac{G m_1 m_2}{r^{2}}\]
\[N(t) = N_0 e^{-\lambda t}\]
\[t_{1/2} = \frac{\ln 2}{\lambda}\]
\[\frac{V_s}{V_p} = \frac{N_s}{N_p}\]
\[K(b,a) = \sum_{\text{paths}} e^{iS[x(t)]/\hbar}\]
\[T_H = \frac{\hbar c^{3}}{8\pi G M k_B}\]
SymbolMeaningUnit
\(\vec F\) net force \(\mathrm{N}\)
\(\vec p\) momentum \(\mathrm{kg·m/s}\)
\(G\) gravitational constant \(\mathrm{m³·kg⁻¹·s⁻²}\)
\(m_1, m_2\) masses \(\mathrm{kg}\)
\(r\) separation \(\mathrm{m}\)
\(N\) number of undecayed nuclei \(\mathrm{1}\)
\(\lambda\) decay constant \(\mathrm{s⁻¹}\)
\(t_{1/2}\) half-life \(\mathrm{s}\)
\(V_s, V_p\) secondary, primary voltage \(\mathrm{V}\)
\(N_s, N_p\) turns on secondary, primary \(\mathrm{1}\)
\(K(b,a)\) amplitude to go from a to b (propagator), in d spatial dimensions \(\mathrm{m^{-d}}\)
\(S\) classical action along a path \(\mathrm{J·s}\)
\(\hbar\) reduced Planck constant \(\mathrm{J·s}\)
\(T_H\) Hawking temperature \(\mathrm{K}\)
\(M\) black-hole mass \(\mathrm{kg}\)
\(c, k_B\) speed of light, Boltzmann constant \(\mathrm{m/s, J/K}\)

Sources

  1. Encyclopaedia Britannica — Isaac Newton
  2. Encyclopaedia Britannica — Newton’s laws of motion
  3. NIST CODATA 2022 — Newtonian constant of gravitation G
  4. NobelPrize.org — Marie Curie, Physics 1903, facts
  5. NobelPrize.org — Marie Curie, Chemistry 1911, facts
  6. Encyclopaedia Britannica — Marie Curie
  7. Rutherford & Soddy (1902) The cause and nature of radioactivity — Part I, Phil. Mag. 4, 370–396
  8. Encyclopaedia Britannica — Atom: Discovery of radioactivity (Rutherford and Soddy formulated the exponential decay law; archived 2021)
  9. US Patent 381,968 (Tesla, 1888) — Electro-Magnetic Motor
  10. Encyclopaedia Britannica — Alternating current
  11. Encyclopaedia Britannica — Transformer
  12. Feynman (1948) Space-Time Approach to Non-Relativistic Quantum Mechanics, Rev. Mod. Phys. 20, 367
  13. NobelPrize.org — The Nobel Prize in Physics 1965 (Tomonaga, Schwinger, Feynman)
  14. Hawking (1974) Black hole explosions?, Nature 248, 30
  15. Encyclopaedia Britannica — Hawking radiation

Source Newton, I. (1687). Philosophiæ Naturalis Principia Mathematica (Axioms, Law II; Book III, universal gravitation). London: Royal Society (J. Streater).

Field notes

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