Skip to product information
1 of 7
Regular price $29.99 USD
Regular price Sale price $29.99 USD
Sale Sold out
Taxes included. Shipping calculated at checkout. Free US shipping on everything; free international shipping on tees, sticker sheets & 4+ stickers.
Color
White · Black
Size
S–5XL
Made
To order · shipping times
Color
Size

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

Measurements in inches, ±1.5 in tolerance.

ShippingFree

Free shipping on every order with a tee, in the US and in every country we ship to. Printed to order for you.

Delivery times & where we ship

The physics

Exclusor works one door, and he does not check names. He checks states.

Behind him is a neon atom: ten electrons, seated 1s² 2s² 2p⁶. Each box on his chart is one orbital: two electrons at most, one spin-up, one spin-down. Every seat in the second shell is taken. Hence the sign.

Wolfgang Pauli wrote the rule in 1925, before anyone knew what the second seat in each box was for. To account for atomic spectra he needed a fourth quantum number with only two values, and he ruled that no two electrons in an atom could share all four. Later that year George Uhlenbeck and Samuel Goudsmit identified it as electron spin. Pauli received the 1945 Nobel Prize.

The modern form is the first three lines on this page. Swap two identical electrons and their joint wavefunction changes sign. Put both in the same state, a equal to b, and the determinant has two identical columns: the wavefunction is zero. That state does not exist.

The badge says ½ because the rule binds him too. Markus Fierz in 1939 and Pauli in 1940 showed that relativistic quantum theory makes every particle of half-integer spin obey it.

Neon has no stable negative ion. An eleventh electron would have to sit in 3s, and neon will not hold it.

Scale it up. In 1926 Ralph Fowler showed that electrons packed this tightly push back: degeneracy pressure, the last formula. It holds up white dwarfs, to about 1.4 solar masses, Chandrasekhar's limit. Exclusion is not a force. Together with electric attraction, it keeps bulk matter from collapsing, as Dyson and Lenard proved in 1967, and Lieb and Thirring, far more simply, in 1975.

Exclusor never shoves. He just knows who is already inside.

Equations

\[\psi(x_1,x_2) = \frac{1}{\sqrt{2}}\begin{vmatrix} \phi_a(x_1) & \phi_b(x_1) \\ \phi_a(x_2) & \phi_b(x_2) \end{vmatrix}\]
\[\psi(x_2,x_1) = -\,\psi(x_1,x_2)\]
\[\phi_a = \phi_b \;\Rightarrow\; \psi = 0\]
\[P = \frac{(3\pi^{2})^{2/3}}{5}\,\frac{\hbar^{2}}{m_e}\,n_e^{5/3}\]
Symbols
SymbolMeaningUnit
\(\psi(x_1,x_2)\) joint wavefunction of two identical electrons (unit for two particles in 3-D) \(\mathrm{m^{-3}}\)
\(x_1, x_2\) coordinates of electrons 1 and 2: position plus spin projection (unit of the position part) \(\mathrm{m}\)
\(\phi_a, \phi_b\) single-electron states a and b, each fixing orbital and spin (unit in 3-D) \(\mathrm{m^{-3/2}}\)
\(P\) electron degeneracy pressure (non-relativistic, zero temperature) \(\mathrm{Pa}\)
\(\hbar\) reduced Planck constant \(\mathrm{J·s}\)
\(m_e\) electron mass \(\mathrm{kg}\)
\(n_e\) number density of electrons \(\mathrm{m^{-3}}\)

Sources

  1. Pauli (1925) Über den Zusammenhang des Abschlusses der Elektronengruppen im Atom mit der Komplexstruktur der Spektren, Z. Phys. 31, 765 (opens in a new tab)
  2. Uhlenbeck & Goudsmit (1925) Ersetzung der Hypothese vom unmechanischen Zwang durch eine Forderung bezüglich des inneren Verhaltens jedes einzelnen Elektrons, Naturwissenschaften 13, 953 (opens in a new tab)
  3. NobelPrize.org — The Nobel Prize in Physics 1945 (Wolfgang Pauli, "for the discovery of the Exclusion Principle") (opens in a new tab)
  4. Fierz (1939) Über die relativistische Theorie kräftefreier Teilchen mit beliebigem Spin, Helv. Phys. Acta 12, 3 (E-Periodica) (opens in a new tab)
  5. Pauli (1940) The Connection Between Spin and Statistics, Phys. Rev. 58, 716 (opens in a new tab)
  6. Feynman Lectures on Physics Vol. III Ch. 4: Identical Particles (opens in a new tab)
  7. Encyclopaedia Britannica — Pauli exclusion principle (opens in a new tab)
  8. NIST Handbook of Basic Atomic Spectroscopic Data — Neon (Ne I ground state 1s² 2s² 2p⁶ ¹S₀) (opens in a new tab)
  9. Ning & Lu (2022) Electron Affinities of Atoms and Structures of Atomic Negative Ions, J. Phys. Chem. Ref. Data 51, 021502 (opens in a new tab)
  10. Andersen, Haugen & Hotop (1999) Binding Energies in Atomic Negative Ions: III, J. Phys. Chem. Ref. Data 28, 1511 (opens in a new tab)
  11. Fowler (1926) On Dense Matter, MNRAS 87, 114 (opens in a new tab)
  12. Chandrasekhar (1931) The Maximum Mass of Ideal White Dwarfs, ApJ 74, 81 (opens in a new tab)
  13. Encyclopaedia Britannica — Chandrasekhar limit (opens in a new tab)
  14. Dyson & Lenard (1967) Stability of Matter. I, J. Math. Phys. 8, 423 (opens in a new tab)
  15. Lieb & Thirring (1975) Bound for the Kinetic Energy of Fermions Which Proves the Stability of Matter, PRL 35, 687 (opens in a new tab)
View full details