Cosmology That ClicksBonus 6 / Standing on the "mover's" side (Trilogy, Part 2)

"α changes from 1/137 to 1/128" — this "change" is a different axis from the "moving over time" of Bonus 5

"1/137 Becomes 1/128" —
Which Motion Is It? There are two axes along which α moves — moving with cosmic time, and moving with the fineness (energy) at which you look.
One of them carries a gauge freedom; the other does not. Mix them up and you crash.

Tools you'll need: the "running α" of Episode 6, Part 1; Bonus 5 The axis of time and the axis of energy

"The fine-structure constant changes from 1/137 to 1/128" — some people really do say this. But it is a change along a completely different axis from the "\(\alpha\) drifting with the ages" story we handled in Bonus 5. This one is the running we did in Episode 6, Part 1 — the value changes not with time, but with the energy you slam things together at (the fineness at which you look). Mix the two up, and you get an accident: you mistake "an accelerator result" for "the universe having changed." The second installment of the trilogy sorts out the two ways \(\alpha\) moves, cleanly.

01"128" isn't a story about time — it's a story about energy

First, what's actually happening. Recall the picture from Episode 6, Part 1. Around the electron clings a thin coat of \(e^+e^-\) pairs welling up out of the vacuum, hiding a bit of its charge (screening). Look coarsely (at low energy) and you're outside the coat, so \(\alpha\approx 1/137\); look finely (at high energy) and you've slipped inside the coat, where the unhidden, stronger charge shows through and \(\alpha\approx 1/128\). The rough boundary is around the mass of the \(Z\) particle (about 91 GeV).

What "128" really is

The same electron, in the same era, viewed by changing only the measuring energy.
The everyday world (low energy) → \(\alpha\approx 1/137\) / the \(Z\)-particle scale (~91 GeV) → \(\alpha\approx 1/128\).
The era hasn't changed, and this isn't about the distant universe — it's a laboratory fact you can reproduce in an accelerator right now.

So when you hear "\(\alpha\) becomes 128" and brace yourself thinking "has the universe changed since long ago?!", that's mixing up the axes. What's moving here isn't time \(t\), it's the fineness of your look = energy \(\mu\). Same phrase, "\(\alpha\) moves," but the axis it runs along is entirely different.

02Line up the two ways α moves

The "\(\alpha\) moving with time" we handled in Bonus 5, and the "\(\alpha\) moving with energy" of right now. The same-named quantity can move along two independent axes. Let's compare them head-on in a table.

 α moving with time (Bonus 5)α moving with energy (this piece; Episode 6, Part 1)
Axis it moves alongthe universe's time tthe fineness of your look = energy μ
Example valuesα may differ between now and 13.8 billion years ago1/137 (low E) → 1/128 (~91 GeV)
Is it physics?real physics (shows up in observations)real physics (shows up in observations)
Which constant do you blame?gauge = free (e, or ε₀, or ħ — your choice)no choice. Physics uniquely fixes it: "the coupling (charge) runs"
What about c and ħ?fixing them is a gauge choicethey don't run at all (they aren't couplings)
How to check itcosmology (quasar absorption lines, Oklo, atomic clocks)accelerators (LEP, etc.) — reproducible right now
How certainevidence for variation is unsettled and contestedan established fact

In the figure below, watch how differently the two knobs bite. Turn the energy knob and \(\alpha\) runs hard (1/137→1/128). Turn the time knob, on the other hand, and \(\alpha\) stays almost flat — because observations pin it down tightly.

Figure: for the same "amount of knob-turning," α runs along the energy axis (amber) but stays nearly flat along the time axis (green). Vertical axis is 1/α (higher = larger α)
Energy knob: α runs Time knob: α stays nearly flat

03Why running has no "freedom to choose the bookkeeper"

Here is the deepest point of this piece, and the very core of the contrast with Bonus 5. In Bonus 5, "when \(\alpha\) moves, whether you make \(e\), \(\varepsilon_0\), or \(\hbar\) the one that moves is a gauge (bookkeeping) freedom." But running has no such freedom. Physics (vacuum polarization) uniquely fixes that what runs is "the coupling constant = the charge \(e\)."

The reason is that \(c\) and \(\hbar\) don't run in the first place. These two aren't "couplings (strengths of a force)"; they are the kinematic conversion factors that link energy to frequency, and momentum to wavelength. Raise the energy, and there's no reason for \(c\) and \(\hbar\) — the conversion rates — to change what they convert. What runs, i.e. depends on energy, is only the coupling that expresses the strength of the interaction. So "blaming \(\alpha\)'s running on \(\hbar\)," that bookkeeping reassignment, simply doesn't hold up here.

The decisive difference between the two "moves"

α moving with time: you can choose which constant to blame (a gauge freedom remains).
α moving with energy: the mover is fixed to e (the coupling) — no choice. α(μ) is a uniquely determined, definite observable at each energy.

A connecting voice — "what's deep is how it runs," from Episode 6, Part 1 In Episode 6, Part 1 we said "the rule for how it runs is deeper than the value (1/137)." How it runs (at what speed it moves from 137 to 128) is calculable from theory, from which charged particles well up in the vacuum. Running has "no bookkeeping freedom" precisely because this way-of-running is uniquely fixed by theory. The reason freedom does remain on the time-variation side is, conversely, that no one has yet been able to nail down the theory that decides "what it is that moves with time."
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04So seeing "128" does not mean the universe has changed

The conclusion. The people who say "\(\alpha\) becomes 1/128" are turning only the "fineness of your look" knob, while holding time, c, ħ, and every other constant fixed. They are doing none of the gauge reassignment — "which constant to blame" — of Bonus 5. That the moving factor is fixed to \(e\) (the coupling) is likewise not a choice but a consequence of the physics of vacuum polarization. So "128" is textbook quantum field theory (QED), and it lives on a different shelf from the varying-constants claim that "the universe has changed since long ago."

An honest line — the two aren't unrelated

The axes are different, but there is a place where the two meet. Build a theory in which "\(\alpha\) really does move with time," and that motion feeds back into the way-of-running rule (the β function) and the contents of the vacuum. So varying-α theorists discuss time variation on top of the running framework. A different axis, but standing on the same stage (quantum field theory) — that's the precise picture.

Note that "nearly flat on the time axis" in the figure is a schematic expression. In reality atomic clocks pin it to \(|\dot\alpha/\alpha|\lesssim 10^{-17}\)/year, and even quasar observations claiming variation come out, order-of-magnitude, at around \(10^{-6}\) over the age-of-the-universe scale — nothing like the 7% of the energy axis. That's why we draw it "nearly flat."

Practice problems
  1. In "α changes from 1/137 to 1/128," what is moving — time, or energy?
    See the answer
    Energy (the fineness of your look). Stay in the same era and raise the measuring energy, and α grows = running. It is not a change in time.
  2. In running, you cannot "blame α's change on ħ." Why?
    See the answer
    Because ħ (and c) aren't couplings but kinematic conversion factors, and don't run with energy in the first place. What runs is only the strength of the interaction = the coupling (the charge e). So there's no freedom to reassign the bookkeeping.
  3. α moving with time versus α moving with energy — in one line, how do they differ in certainty?
    See the answer
    Moving with energy (running) is an established fact reproducible in accelerators. Moving with time is still unsettled and contested — the evidence isn't in.

SUMMARYThe same "α moves," but there are two axes

"1/137 becomes 1/128" is running that moves with energy (the fineness of your look), not time. Through screening by vacuum polarization, the finer you look the stronger the charge appears and the more α grows — a fact already checked in accelerators. It is a different axis from the "α moving with time" of Bonus 5, and moreover running has no gauge freedom of "which constant to blame" — physics uniquely fixes that what runs is the coupling (charge), and c and ħ don't run in the first place.

So seeing "128" and thinking "the universe has changed" is mixing up the axes. α moving with time is unsettled and contested; α moving with energy is an established fact. The same-named quantity can move along two independent axes — the first thing to do is tell which one you're talking about. That was the second installment of the trilogy.

This document is Bonus 6 of the "Cosmology That Clicks" series, a piece for physics-loving high-schoolers and undergraduates. The "running" of the fine-structure constant is established physics due to vacuum polarization, and the change from \(\alpha^{-1}\approx137.0\) (low-energy limit) to \(\alpha^{-1}\approx128\) (\(Z\)-boson mass, ~91 GeV) has been measured in accelerator experiments. This is an energy-scale dependence, a separate axis from time variation. Observational constraints on time variation are about \(|\dot\alpha/\alpha|\lesssim 10^{-17}\)/year from atomic clocks; claims of variation in distant quasars (the reports by Webb et al.) are of order \(10^{-6}\) over the age-of-the-universe scale, but independent verification remains unsettled. What runs in running is a dimensionless coupling; \(c\) and \(\hbar\), as kinematic conversion factors, do not run. The flatness of the time axis in the figure is a schematic expression. — To print, use your browser's "Print" and "Save as PDF" (in the print version the slider and answers are frozen and hidden).

Print / make a PDF: ⌘+P (Ctrl+P on Windows). On screen, the slider lets you see how differently the energy axis and time axis bite. "See the answer" opens each solution.