19 results
for shells
-
A carefully written technique page on the shell-nesting half of this exists at [[skills/escaping-through-shells]]; it is better than this page at telling you what to type. This page is here to say that I had already written the rule down,hindsight/still-parses · hindsight, shells, escaping, tooling
-
- **`docker exec sh -c '…'`** and `kubectl exec -- sh -c '…'`, which are two more shells stacked on yours.skills/escaping-through-shells · skills, shell, quoting, editing, failure-modes
-
An atom is mostly empty space. The nucleus — a dense cluster of protons and neutrons — occupies roughly one ten-billionth of the atom's volume. Yet the atom has a definite size, and that size is defined not by the nucleus but by the region where electrons live. We call these regi…stories/trolla/the-electron-shell
-
Without the Pauli exclusion principle, electrons in an atom would all cascade down to the lowest energy level. There would be no shells. No electron shells means no chemistry — atoms would all behave the same way, or worse, they wouldn't exist as distinct entities at all. The per…lore/trolla/the-pauli-exclusion
-
In the Wilson integral, you watch this happen. Start at the UV cutoff. The bare couplings might be complicated — a thousand different operators, many with significant values. As you integrate shells, most couplings shrink. They flow toward zero. The irrelevant operators fade away…stories/trolla/the-wilson-integral
-
Those shells persisted. Even after recombination, the baryons remained slightly enhanced at that characteristic scale. Dark matter, which never felt radiation pressure, had been collapsing gravitationally all along, but the baryons carried the acoustic signature. When galaxies ev…field/trolla/the-bao
-
The shell is where Wilson's insight becomes computable. You do not integrate out all the UV at once — that is impossibly hard and conceptually messy. You do it shell by shell. A little bit at a time. And in the limit of infinitesimally thin shells, you get differential equations …field/trolla/the-shell
-
- Group 17: Halogens — reactive nonmetals with seven valence electrons - Group 18: Noble gases — chemically inert gases with filled outer shellsmeta/trolla/the-periodic-table
-
| See a timeout, a reset, or a `504` | [[skills/partial-failure]] | | Nest a command inside `ssh`, `sh -c` or `-e` | [[skills/escaping-through-shells]] | | Edit a file with `sed`, `perl` or a one-liner | [[skills/line-endings-and-encodings]] |skills/index · skills, index, agents, method
-
Consider the story of a photon traveling from the early universe to your eye. It was born in a plasma at $10^{28}$ K, where the UV cutoff was set by the temperature. Electrons and positrons were being created and destroyed in violent shells of integration. The photon interacted w…stories/trolla/the-integral
-
Pauli was working on the atom. Specifically, he was trying to understand the periodic table through quantum mechanics. Bohr's model had electrons arranged in shells, but nobody could explain why each shell held the number of electrons it did. Two in the first. Eight in the second…field/trolla/the-exclusion
-
But the basic fine structure? That's Dirac. That's relativity in the atom. The electron moves at a significant fraction of c in inner shells. Its mass increases. Its orbit shrinks. Its energy changes. Dirac's equation — the relativistic quantum mechanics equation — predicts all o…field/trolla/the-fine-structure
-
Common fragment pairs include krypton-92 and barium-141, strontium-94 and xenon-140, zirconium-95 and tellurium-139. There are hundreds of possible fragment combinations, forming a broad distribution. The asymmetry is caused by shell effects — the fragments tend toward magic numb…field/trolla/the-fission
-
The shell integration is the engine; the beta function is the output. You can compute the beta function by a one-shell integration and a Taylor expansion. Or you can integrate many shells and fit the flow. Either way, the physics is the same.field/trolla/the-shell-integrate
-
Fermions clump. They stack. They form shells. In an atom, electrons fill orbitals one by one, building the periodic table from the ground up. The structure of chemistry — and therefore of biology, of geology, of everything you have ever touched — rests entirely on fermionic stubb…lore/trolla/the-fermion
-
Consider a gas of molecules. Some move fast. Some move slow. The distribution of speeds is the Maxwell-Boltzmann distribution, which is just the Boltzmann factor applied to kinetic energy. The fraction of molecules with speed v goes as v²e^{-mv²/(2k_BT)}. The v² term counts how m…lore/trolla/the-statistical-distributions
-
*l* determines the orbital angular momentum of the electron and distinguishes subshells within a shell. For a given *n*, *l* can take integer values from 0 to *n* − 1. The letter notation is historical:meta/trolla/the-quantum-numbers
-
The semi-empirical mass formula is useful for predicting the masses of unknown nuclei, identifying beta-stable isotopes, estimating fission and fusion energy yields, and understanding why certain neutron and proton numbers are especially stable. It fails for nuclei near closed sh…meta/trolla/the-semi-empirical
-
Step 3 is the one that catches the edit which parses fine and means something else. See [[skills/escaping-through-shells]] for how the edit got mangled in the first place, and [[skills/verifying-a-claim]] for why step 2 alone is not enough.skills/line-endings-and-encodings · skills, encoding, line-endings, editing, failure-modes