In Episode 2 we said "the coefficient 1/4 is the one thing that ratios can't give you" ── so let's see how far we can get by hand
In Episode 2 I wrote that the skeleton of black-hole entropy \(S=A/(4\ell_P^2)\) (the area law) comes out from ratios alone, but that the coefficient 1/4 alone requires a quantum-gravity calculation. The 137.036 of α was a mystery nobody can derive, but this 1/4 is within reach ── actually doing that is what this bonus episode is about. To give away the ending first ── the 1/4 gets built up almost entirely from your "ratios." ① the radius of the horizon, ② the surface gravity, ④ the first law, ⑤ the area ── all of these are just lining up quantities that carry units and dividing. There is exactly one place where the hand calculation stops: ③ the 2π in the relation "accelerate, and you see a temperature." And the true identity of that 2π is exactly what your "Understanding Cosmology" Episode 9 was about ──〈rotate i onto the imaginary axis and a temperature is born〉── that very thing. The only thing you import is this single 2π. Everything else is in your own hands.
If you push with dimensions alone, the only length unit entropy can carry is the Planck length \(\ell_P\), so you get to \(S\propto A/\ell_P^2\) (the area law) right away. But the pure number ── "is it \(1/4\), or \(1\), or \(1/2\)?" ── can never come out of dimensional analysis. Here you need exactly one drop of genuine physics (mechanics). What that one drop is, we'll pin down by moving our hands.
Here is the first seed of the 1/4 ── squaring the "2" in the Schwarzschild radius put a \(4\) in the denominator. Nothing has been imported yet; this is pure hand calculation. (Amusingly, \(g=c^4/4GM\) ── just Newton's gravity evaluated at \(R_s\) ── coincides exactly with the general-relativistic "surface gravity." A relative of Episode 1's "Newton somehow gets it right.")
This is the single drop that ratios cannot give you. Stand somewhere strongly accelerating (=right next to the horizon) and the vacuum looks like a "hot thing with a temperature" (the Unruh effect). That temperature is tied to the acceleration (surface gravity) \(g\) like this ──
The 2π in the denominator is the whole of this bonus episode's "magic." Plug in \(g=c^4/4GM\) from ② and \(8\pi=2\pi\times4\). The form of the Hawking temperature from Episodes 2 and 3 lands here in your hands.
Where does this 2π come from? It's a basic theorem of statistical mechanics ── a world at temperature \(T\) is the same as a world where, once you rotate time to imaginary values (\(t\to i\tau\)), imaginary time is rolled up into a circle of period \(\hbar/k_BT\) ("Understanding Cosmology" Episode 9, "rotate i onto the imaginary axis and get temperature"). Rotate the spacetime near the horizon into imaginary time, and the period that avoids making a cusp (a conical singularity) is fixed at exactly 2π/(surface gravity) ── an angle story, "one full turn is 2π," fixes the temperature. So what you actually imported is just the one point "imaginary time is periodic = that is temperature." From here on, we're back in the world of ratios.
There it is. The identity of the 1/4 is \(\dfrac{4\pi}{16\pi}\) ── the \(4\pi\) that came from integrating on the temperature side (④), divided by the \(16\pi\) on the area side (=the sphere's \(4\pi\) × the \(2^2\) from \(R_s\)). The π of the temperature and the π of the area get divided, and out comes 1/4.
①②④⑤⑥ are all your "ratios." The only thing you imported is the 2π of ③. Unlike α's 137.036, the 1/4 was a number you can derive by hand.
The figure below steps through ①→⑥ one at a time, showing how the \(1/4\) gets built up. Advance with "Next step." At each stage you can follow with your eyes which equation is added, where the "4" and "16" are born, and how it finally lands on \(4\pi/16\pi=1/4\). Only at ③ does an "import: 2π" tag appear ── that's the single drop that ratios can't give you.
Let's chew the 2π imported at ③ one stage finer. The story is in two parts: (A) temperature, at its root, is an "imaginary-time loop," and (B) at the horizon, one turn of that loop has to be exactly 2π or it forms a cusp. Put these two together and the 2π turns into temperature.
(A) Temperature is the "length" of the imaginary-time loop. Quantum time evolution is \(e^{-iHt/\hbar}\), and the Boltzmann factor of statistical mechanics is \(e^{-H/k_BT}\). Set these two side by side ──
In other words, "to exist at temperature \(T\)" = "to advance a length \(\hbar/k_BT\) in the direction of imaginary time \(\tau=it\)." And because the statistical average is a full sum around (a trace), the two ends of imaginary time join up ── imaginary time rolls up into a "loop (circle)" of period \(\hbar/k_BT\). A short loop = hot, a long loop = cold. Temperature turns out to be the inverse of the length of the imaginary-time loop (the KMS condition; the substance of "Understanding Cosmology" Episode 9's "rotate i onto the imaginary axis and get temperature").
(B) The region near the horizon is "a plane in polar coordinates" ── so one full turn is 2π. Rotate the spacetime near a black hole into imaginary time, and the two dimensions (imaginary time, distance from the horizon) take exactly the form of the plane in polar coordinates \(ds^2=d\rho^2+\rho^2 d\varphi^2\) (\(\rho\)=distance from the horizon, \(\varphi\)=the "angle" built from imaginary time). What matters here is ──
When you view a plane in polar coordinates, for the center (\(\rho=0\)=the horizon) to be smooth (not a cusp), the angle \(\varphi\) has to go around in exactly 2π. Shorter than 2π and you get a conical cusp; longer and you get a fold, and spacetime breaks there. It's the same as folding paper into a cone: it becomes pointed by exactly the angle you cut away (the deficit) ── "a clean plane = one turn of 2π."
Since this "angle \(\varphi\) is built from the surface gravity \(\kappa\) and imaginary time as \(\varphi\propto\kappa\tau\)," \(\varphi\) going around in 2π = the period of imaginary time \(\tau\) is \(2\pi/\kappa\) (×c). Set this equal to (A)'s "period of imaginary time = \(\hbar/k_BT\)" ──
The Hawking temperature of ③ came out purely from the smoothness of geometry: "the length of the imaginary-time loop (temperature)" = "the one turn that keeps the horizon from cusping (2π)." The true identity of the imported "seed" is ── "one full turn is 360°=2π," that and nothing more. The 2π of the circle circumference is, as is, the 2π of the black hole's temperature.
To sum up, the 2π of ③ is no magic at all ── it's a combination of two obvious things: "temperature = the length of the imaginary-time loop" + "the turn that keeps the horizon from cusping = 2π." It's a drop that dimensional analysis (ratios) can't give you, but the identity of that drop is the 2π of a circle's circumference. Accept that much, and the 1/4 is entirely yours to derive by hand.
The derivation shown here (② \(g=c^4/4GM\), ③ the Hawking temperature, ④⑤⑥ the thermodynamics, and 1/4=4π/16π) all agrees with the standard semiclassical results. The derivation of the 1/4 via the conical-deficit / Gibbons–Hawking Euclidean path integral is also well established. "The only import is a single 2π" is an accurate summary within this semiclassical framework.
That said. ① The reason the Newtonian surface gravity \(g=GM/R_s^2=c^4/4GM\) of ② agrees with the general-relativistic surface gravity is close to a "happy coincidence"; the legitimate derivation is general relativity (surface gravity \(\kappa\)) (same kind of thing as Episode 1's "Newton somehow gets it right"). ② This 1/4 is a semiclassical (thermodynamic / geometric) derivation; explaining "why the horizon has \(A/4\ell_P^2\) microscopic states" by counting is a separate task ── that's carried out by string theory (Strominger–Vafa 1996, counting states to reproduce the 1/4) and loop quantum gravity (fixing the Immirzi parameter to get the 1/4), the story of Episodes 2 and 6. ③ The 2π of "acceleration → temperature" is a genuine quantum effect (Unruh effect / KMS) that dimensional analysis can't give you ── so you can't get to "zero imports." ④ \(A/4\) is the leading term; there are logarithmic corrections and, if the gravitational action is non-Einstein, a generalization to Wald entropy.
The 1/4 in Bekenstein–Hawking's \(S=A/(4\ell_P^2)\) gets built up almost entirely from "ratios." ① \(R_s=2GM/c^2\), ② surface gravity \(g=GM/R_s^2=c^4/4GM\) (the 2²=4 seed here), ④ the first law gives \(S=4\pi GM^2/\hbar c\), ⑤ the area \(A=16\pi G^2M^2/c^4\), ⑥ combine to \(S=k_B A/4\ell_P^2\). The identity of the 1/4 is 4π/16π (the temperature's π ÷ the geometry's π). The only place the hand calculation stalls is ③ ── the 2π of "accelerate, and you see a temperature" (Unruh / KMS, the imaginary-time-=-temperature of "Understanding Cosmology" Episode 9).
So to be honest ── the 1/4 can be completely derived by hand. Except that a single 2π ── "imaginary time is periodic = temperature" ── has to be accepted as physics. That is the drop ratios can't give you, the genuine one where quantum and geometry meet. But it feels good that the import can be pared down to a single 2π. Whereas α's 137.036 was a "mystery you can't derive," this 1/4 is a success story within reach ── and string theory and LQG independently reproduce the same 1/4 (Episodes 2 and 6). "Ratios for the skeleton, 2π for the import, and the rest is entirely in your hands."
Print / save as PDF: ⌘+P (Ctrl+P on Windows). On screen, "Next step" builds up the 1/4. "Show answer" opens each solution.