Maria Goeppert Mayer Sticker
A Full Floor Is Magic. | Physics
Some nuclei are unusually stable, at numbers that looked like magic. In 1949 Goeppert Mayer, and independently Jensen, Haxel and Suess, explained the magic numbers (2, 8, 20, 28, 50, 82, 126) with spin–orbit coupling. A pixel-art portrait on a 3" × 3" sticker; the physics panel below has the equation, every symbol and the sources.
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Details
Size3″ × 3″
3″ × 3″ kiss-cut sticker.
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The physics
Protons and neutrons fill energy shells in the nucleus, much like electrons in an atom. Adding strong spin-orbit coupling moves the shell gaps to the observed magic numbers 2, 8, 20, 28, 50, 82 and 126, where nuclei are unusually stable.
Equations
| Symbol | Meaning | Unit |
|---|---|---|
| \(E_N\) | energy of oscillator shell N | \(\mathrm{J}\) |
| \(N\) | oscillator shell number | \(\mathrm{1}\) |
| \(\hbar\omega\) | oscillator level spacing | \(\mathrm{J}\) |
| \(g_N\) | states in shell N per nucleon species (spin included) | \(\mathrm{1}\) |
| \(V_{\ell s}\) | spin–orbit potential | \(\mathrm{J}\) |
| \(C(r)\) | radial strength of the spin–orbit term (with orbital and spin angular momentum measured in units of ħ) | \(\mathrm{J}\) |
| \(\vec\ell, \vec s\) | orbital and spin angular momentum, in units of ħ | \(\mathrm{1}\) |
| \(\ell\) | orbital angular momentum quantum number | \(\mathrm{1}\) |
| \(j\) | total angular momentum quantum number | \(\mathrm{1}\) |
Sources
- Goeppert Mayer (1949) On Closed Shells in Nuclei. II, Phys. Rev. 75, 1969 (opens in a new tab)
- Haxel, Jensen & Suess (1949) On the "Magic Numbers" in Nuclear Structure, Phys. Rev. 75, 1766 (opens in a new tab)
- Goeppert Mayer, Nobel Lecture (1963) The shell model (opens in a new tab)
- NobelPrize.org — The Nobel Prize in Physics 1963 (summary) (opens in a new tab)
- Scientific American — The last woman to win a physics Nobel (waltz analogy) (opens in a new tab)
- Wikipedia — Nuclear shell model (opens in a new tab)
Source Mayer, M. G. (1949). On Closed Shells in Nuclei. II. Physical Review 75, 1969–1970.doi.org/10.1103/PhysRev.75.1969 (opens in a new tab)