The answer to step 1 is in ── and the reason is that the supertranslation weight was "a half"
A reader made a fair point about the previous article ── "the usual loop of swapping one problem for another?" Half right. Episode 12 merely arrived at Episode 11's wall from another direction; it was not progress.
There are only two ways out. Compute, or go and get the negative. This episode does both. We actually ran step 0 (the positive control) and step 1 (the branch point) from the procedure table placed at the end of last time.
The result first. Step 0 failed once and spat out a bug in my own formula. And the answer to step 1 is NO.
This is not a rephrasing. One door has closed.
Episode 11 wrote down the template for the proof ── asymptotic symmetry → central charge → Cardy. If we intend to use it in four dimensions, we must first see that the tool works correctly in the three-dimensional case where the answer is known. Step 0.
Doing it for real, it failed. The BMS-Cardy formula written in Episode 11 was mixing conventions ── the algebra was written with \(\frac{c}{12}m^3\) while the formula used the form from another convention that writes the central term bare. The entropy was overestimated by \(\sqrt{12}=2\sqrt3\approx3.46\).
Corrected and re-run, it agrees with the geometry side to a relative deviation of \(2.2\times10^{-16}\) across six orders of magnitude in \(GM\). The details and the corrected formula are in Episode 11, §03.
The tool passed. Having earned the right to proceed to step 1, we proceed.
The question was this ── can a central term enter the bracket of BMS₄ that straddles superrotations and supertranslations?
"I looked and did not find it" is no answer. Write down every form it could take and solve the equations. The central term is a number (the coefficient of the central element \(Z\)), so there are infinitely many unknowns rather than finitely many, but cut off by mode it is a system of simultaneous linear equations.
First, write the algebra in a form covering both three and four dimensions. With superrotations \(L_m\) and supertranslations \(T_r\) ──
Here \(a\) is the weight the supertranslations carry under the superrotations. This single number distinguishes three dimensions from four.
| \([L_m,T_r]\) | \(a\) | \(b\) | |
|---|---|---|---|
| bms₃ | \((m-r)T_{m+r}\) | \(1\) | \(0\) |
| bms₄ (one chirality) | \(\left(\frac{m-1}{2}-r\right)T_{m+r}\) | \(\mathbf{1/2}\) | \(-1/2\) |
The \(1/2\) in four dimensions comes from the supertranslations carrying weight \((-\tfrac12,-\tfrac12)\) on the celestial sphere ── an established fact, to the point that some write \(\mathfrak{bms}_4\) as \(W(-\tfrac12,-\tfrac12,-\tfrac12,-\tfrac12)\). That awkward number becomes the protagonist of this episode.
Now, \(C(m,r)\) is the coefficient of a central element, so it can only be non-zero when the modes sum to zero (otherwise \(Z\) would carry a mode). So the unknowns line up in a single row ──
$$C(m,r)=c_m\,\delta_{m+r,0}$$The unknowns are \(\{c_m\}\). The stage is set.
You may not put in arbitrary \(c_m\). A Lie algebra must satisfy the Jacobi identity. Written with the three elements \(L_m,\,L_n,\,T_r\) ──
$$[[L_m,L_n],T_r]-[L_m,[L_n,T_r]]+[L_n,[L_m,T_r]]=0$$The central element commutes with everything, so we can pick out just the central part. Only \(r=-(m+n)\) survives ──
Completely linear in \(c_m\). Which is to say, this is just a system of simultaneous linear equations. All we have to do is count the dimension of the solution space.
But one subtraction is needed, because there are merely apparent solutions. Redefine a generator as \(T_0\to T_0+\beta Z\) and a central term appears although nothing was done ──
$$c_m^{\text{trivial}}=\bigl((a+1)m+b\bigr)\beta$$This is nothing but a change of coordinates, so it is not a physical central charge. Mathematics calls it a coboundary. What we want is
$$\dim H^2\;=\;\dim(\text{cocycle space})\;-\;\dim(\text{coboundary space})$$If this is \(0\), "there is no central charge"; if \(1\) or more, "there is." The answer is an integer, and binary.
The same discipline again. Try it first where the answer is known. Three dimensions really has \(c_M=3/G\), so if putting in \(a=1,\,b=0\) does not give \(\dim H^2=1\), this computation cannot be trusted.
Cutting the modes at \(|m|\le8\) gives 17 unknowns and 217 equations. Solved exactly over the rationals (with floating point, judging the rank becomes a question of thresholds).
# [L_m, T_r] = (m - r) T_{m+r} + c_m delta_{m+r,0} # 17 unknowns (|m| <= 8), 217 equations from Jacobi, exactly over the rationals cocycle space dim = 2 coboundary dim = 1 c_m = 2m ------------------------------------------ dim H^2 = 1 identifying the extra solution as a polynomial: c_m = m^3 satisfies Jacobi : YES c_m = m^3 - m satisfies Jacobi : YES c_m = m satisfies Jacobi : YES (← coboundary. trivial) → there it is. this is what c_M = 3/G really is. matches the form of the literature's central term (c_M/12)(m^3 - m).
There it is. \(m^3-m\) satisfies Jacobi, and it is not a coboundary. This is the \(c_M\) that carried the entire entropy in Episode 11. The three-dimensional success has been reproduced inside my own computation.
The tool works. On to the real run.
Put \(a=1/2,\,b=-1/2\) into the same code.
# [L_m, T_r] = ((m-1)/2 - r) T_{m+r} + c_m delta_{m+r,0} cocycle space dim = 1 coboundary dim = 1 c_m = (3m - 1)/2 ------------------------------------------ dim H^2 = 0 looking at the unique cocycle (|m| <= 12, m = -3..3): -2/7 -1/5 -4/35 -1/35 2/35 1/7 8/35 = (3m - 1) / 35 ← the coboundary itself trying the form that worked in three dimensions: c_m = m^3 - m satisfies Jacobi : NO (violated at 388 places) unchanged when the mode cutoff is varied: |m| <= 4 dim H^2 = 0 |m| <= 6 dim H^2 = 0 |m| <= 8 dim H^2 = 0 |m| <= 12 dim H^2 = 0 the sign convention is written both (m+1)/2 and (m-1)/2 in the literature, so both: a=1/2, b=+1/2 dim H^2 = 0 a=1/2, b=-1/2 dim H^2 = 0
All that survived in the solution space is one coboundary. And that is merely apparent, produced by shifting a generator's definition. Subtract it and you get zero.
No central charge can enter the superrotation–supertranslation bracket of BMS₄.
It is not "not yet found." The Jacobi identity does not permit it, so searching will not find it. The \(m^3-m\) that made \(c_M=3/G\) work in three dimensions violates the identity at 388 places in four.
Therefore route A' (a 4d version of BMS-Cardy) is structurally closed. The proof that Episode 10 described as "already done in three dimensions" does not lift as it stands.
Stop here and it ends at "four dimensions failed." Sweep \(a\) with the same code and the condition itself should become visible. Moving the weight continuously, I counted \(\dim H^2\).
Move the slider and the bar stays low almost everywhere. And it jumps only at the integers. Tabulating the sweep ──
| weight \(a\) | \(b\) | \(\dim H^2\) | genuine cocycle |
|---|---|---|---|
| \(-1\) | \(0\) | 2 | \(c_m=1,\;c_m=m\) |
| \(0\) | \(0\) | 1 | \(c_m=m^2\) |
| \(1\) bms₃ | \(0\) | 1 | \(c_m=m^3\) ← \(c_M=3/G\) |
| \(1/2\) bms₄ | \(-1/2\) | 0 | none |
| All 64 combinations of \(a\in\{-1,-\tfrac12,0,\tfrac12,1,\tfrac32,2,3\}\) and \(b\in\{-1,-\tfrac12,0,\tfrac12,1,\tfrac32,2,3\}\) were run. Only three points gave \(H^2\ne0\): \(b=0\) with \(a\in\{-1,0,1\}\) | |||
A central charge stands in the superrotation–supertranslation bracket only when the weight \(a\) is an integer.
bms₃ has \(a=1\) ── on the target. bms₄ has \(a=1/2\) ── off by exactly a half.
This is a shape the series has stepped on many times. Anomaly cancellation in Episode 2, the closing of the algebra in Episode 6, the twistorial lift in Episode 8, the central charge in Episode 11 ── a binary target that cannot be tuned continuously. This time it wore the face of integrality.
And four dimensions missed. Not narrowly, not by a whisker ── by exactly \(1/2\).
Here I write with inference included. The numerical fact (\(H^2=0\) at \(a=1/2\)) is as computed above, but the reading of why only four dimensions is awkward is mine.
A supertranslation was "the freedom to shift the time." How the shift function \(T\) transforms under coordinate changes on the boundary ── that weight is \(a\).
| spatial section of the boundary | supertranslation weight | \(a\) | |
|---|---|---|---|
| 3d gravity | the celestial "sphere" is a circle \(S^1\) | \(-1\) (one whole direction) | \(1\) |
| 4d gravity | the celestial sphere \(S^2\) | \((-\tfrac12,-\tfrac12)\) (halved across two directions) | \(1/2\) |
The total is \(-1\) in both cases. What differs is that four dimensions has two chiralities, so the two of them share that \(-1\). Shared, it becomes \(1/2\), and falls off the integer target.
Put differently ── the weight split because the four-dimensional celestial sphere is two-dimensional. In three dimensions the boundary is one-dimensional, so there was nobody to split with and it stayed an integer.
Saying "there is none" from my own computation alone would be risky, so I checked. Three independent lines give the same answer.
| line | what it says |
|---|---|
| algebra (cohomology) Safari–Sheikh-Jabbari 2019 arXiv:1902.03260 | "The second real cohomology \(H^2(\mathfrak{bms}_4;\mathbb{R})\) admits no central extension other than \(C_{\mathcal L},\,C_{\bar{\mathcal L}}\)" ── a classification citing Barnich–Troessaert. That is, only the two Witt sides; none in the mixed bracket. Consistent with the computation above |
| charge algebra (field-dependent) Barnich–Troessaert 2011 / Barnich 2017 arXiv:1106.0213, 1703.08704 | What appears in four dimensions is a field-dependent 2-cocycle. Not a constant central charge, and it vanishes if one uses globally defined BMS. Hence it is treated as a Lie algebroid rather than a Lie algebra (as touched on in Episode 11, §01) |
| charge algebra (latest) Rignon-Bret–Speziale 2024 PRD 110, 044050 | Using the Wald–Zoupas prescription, the BMS algebra is realized with no 2-cocycle and no central extension on any cut of null infinity. The paper's title is literally "Centerless BMS charge algebra" |
Zero from the algebra side and zero from the charge side. This \(1/2\) is not the kind of wall that merely happens to be beyond present technique.
Let us refill the procedure table placed at the end of Episode 11.
| step | content | status |
|---|---|---|
| 0 | Positive control. Reproduce the 3d BMS-Cardy in the original papers' convention | passed (failed once, recovering one bug in the formula) |
| 1 | Does the supertranslation sector of BMS₄ have a \(c_M\) analogue? | the answer is NO. \(\dim H^2=0\) |
| 2a | if yes → route A' (a 4d version of BMS-Cardy) | closed |
| 2b | if no → look for a different template | the only survivor |
Episode 11 wrote that "the question is well posed, including the possibility that the answer is 'no'." We have now drawn that "no."
It looks like a loss, but not quite. A door that has closed is a door you never have to knock on again. We treat it the same way Episode 1 treated \(p=0.67\) as a result ── a negative is information.
What remains is 2b. Route B from Episode 11, §05 ── the road that uses no modular invariance and builds a Cardy-type formula by dimensional reduction in the limit of a small thermal circle (the line Di Pietro–Komargodski followed in \(d=4,6\)). That route does not require \(c_M\) in the first place. The absence of a central charge is no blow to it.
If we intend to get the four-dimensional area law out of Cardy, the template must not route through a central charge.
Until now we were waiting to see "whether a central charge would be found." We no longer have to wait.
Step 0 (the positive control) failed once. Episode 11's BMS-Cardy formula mixed conventions and was off by \(\sqrt{12}=2\sqrt3\). After correction it agrees with the geometry side to a relative deviation of \(2.2\times10^{-16}\) across six orders in \(GM\). Without the positive control I would have carried that bug into four dimensions.
The answer to step 1 is NO. Putting the central term in as unknowns and solving the Jacobi identity exactly over the rationals as a linear system gives \(\dim H^2=0\) for the superrotation–supertranslation bracket of bms₄. All that remains in the solution space is one coboundary. Unchanged for mode cutoffs \(|m|\le4,6,8,12\), and unchanged for the sign convention \(b=\pm\tfrac12\).
It is a negative with a positive control. Feed the same code bms₃ (\(a=1,b=0\)) and \(\dim H^2=1\) comes out, with central term \(m^3-m\) ── matching the form of the literature's \(c_M=3/G\). The tool can detect "there is one." And still nothing came out in four dimensions.
And the reason came out ── the target was the integers. Sweeping the weight \(a\) over 64 combinations, \(H^2\ne0\) only at three points: \(b=0\) with \(a\in\{-1,0,1\}\). bms₃ is on target at \(a=1\); bms₄ is off by exactly a half at \(a=1/2\). The result of the weight \(-1\) being halved across two chiralities, because the four-dimensional celestial sphere is two-dimensional.
Route A' is closed. Episode 10's three-dimensional proof does not lift as it stands. What survives is route B from Episode 11, §05 ── a dimensional-reduction Cardy that does not route through a central charge. There is no longer any need to wait for one.
This was not a rephrasing. Up to Episode 12 the series kept moving the question around. What we did this time was not a move but closing a door. In the same sense that Episode 1 treated \(p=0.67\) as a result, a negative is information.
This document is Episode 13 of the "Lattice We Build" series, a reading piece for high-school and university students who love physics. Where the sister series "That Clicks" explains known physics, this series shows the work itself ── including the failures and their corrections.
Established material: the commutators of the BMS₃ / BMS₄ algebras and the supertranslation weights; the horizon entropy of 3d flat cosmology and its reproduction by BMS-Cardy (Barnich arXiv:1208.4371, Bagchi–Detournay–Fareghbal–Simón arXiv:1208.4372); that \(H^2(\mathfrak{bms}_4;\mathbb{R})\) admits no central extension beyond the two Witt central charges (Safari–Sheikh-Jabbari arXiv:1902.03260, citing Barnich–Troessaert arXiv:1106.0213); the field-dependent 2-cocycle and Lie algebroid of the 4d charge algebra (Barnich arXiv:1703.08704); and the centerless charge algebra in the Wald–Zoupas prescription (Rignon-Bret–Speziale, PRD 110, 044050 (2024)).
The cohomology computation in §02–06 of this article is an independent rederivation of the conclusions of those papers, carried out as finite-dimensional linear algebra with modes cut off ── so strictly it is a claim "within the truncation" (verified invariant for \(|m|\le4,6,8,12\)).
On the other hand, §07's reading that "the weight is awkward because the 4d celestial sphere is two-dimensional and the \(-1\) is halved across two chiralities" is this series' author's interpretation. The weight \((-\tfrac12,-\tfrac12)\) itself is an established fact, but describing it as "missing the integer target" is this article's phrasing. The Weyl-BMS loophole at the end of §08 is presented only as a report of the literature and has not been checked. That the horizon's Carrollian theory itself is unconstructed is as stated in Episodes 8, 11 and 12.
Main series: Episode 1|Episode 2|Episode 3|Episode 4|Episode 5|Episode 6|Episode 7|Episode 8|Episode 9|Episode 10|Episode 11|Episode 12 | bonus: ①/②/③ ── to print, use your browser's "Print" → "Save as PDF."
Print / PDF: ⌘+P (Ctrl+P on Windows). The figure lets you confirm that shifting the weight off an integer makes the central charge vanish.