The Lattice We BuildEpisode 13 / There is no central charge

The answer to step 1 is in ── and the reason is that the supertranslation weight was "a half"

There is no central charge Up to now we have narrowed the question to one ── does the supertranslation sector of BMS₄ have an analogue of \(c_M\)?
Here is the answer. No. Not "not yet found," but structurally unable to enter.
Put the central term in as unknowns and solve the Jacobi identity as a linear system, and the solution vanishes.
And the reason came out too ── because the four-dimensional supertranslation weight is the awkward number \(1/2\).

Tools needed: Episode 11 (\(c_L\), \(c_M\), BMS-Cardy), simultaneous linear equations The core of this episode: \(\dim H^2=0\). The target was the integers

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.

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01First, confirm the tool is not broken

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.

WHY YOU MUST NOT SKIP THIS \(\sqrt{12}\) is not a size you spot by staring at a formula. Had I gone to four dimensions without the positive control, I would have kept blaming the disagreement on physics. A bug in the tool and a fact about nature show up with the same face: the answer does not match. Without killing the tool's bugs first, you cannot tell them apart.

The tool passed. Having earned the right to proceed to step 1, we proceed.

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02Make the central term an unknown

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 \(T_r\) ──

THE COMMON FORM
$$[L_m,L_n]=(m-n)L_{m+n}+\cdots,\qquad [T_r,T_s]=0$$ $$[L_m,T_r]=\underbrace{(a\,m-r+b)}_{f(m,r)}\,T_{m+r}\;+\;C(m,r)\,Z$$

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.

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03The Jacobi identity becomes the equations

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 ──

THE COCYCLE CONDITION
$$(m-n)\,c_{m+n}\;-\;(a n+m+n+b)\,c_m\;+\;(a m+m+n+b)\,c_n\;=\;0$$

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.

WHAT WE ARE ACTUALLY DOING This is the procedure of computing the second Lie-algebra cohomology \(H^2\) by cutting off modes and reducing it to finite-dimensional linear algebra. Almost the same toolkit as finding the integer kernel of the dimension matrix in Episode 1 ── build a matrix and count its rank. The physics vocabulary disappears and only linear algebra remains.
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04Positive control ── does \(m^3-m\) come out for bms₃?

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).

POSITIVE CONTROL ── bms₃ (a = 1, b = 0)
# [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.

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05bms₄ ── nothing comes out

Put \(a=1/2,\,b=-1/2\) into the same code.

THE REAL RUN ── bms₄ (a = 1/2, b = −1/2)
# [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.

THE ANSWER TO STEP 1

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.

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06So what kind of algebra can have one?

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 \(\dim H^2\).

Figure: the dimension of the cocycle space as the supertranslation weight \(a\) is varied. For almost every \(a\) it is "coboundary only." A central charge stands only at a few isolated points, like the teeth of a comb
coboundary only (\(H^2=0\)) a genuine central charge exists (\(H^2\ge1\)) the \(a\) currently selected

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\(-1/2\)0none
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 \(a\in\{-1,0,1\}\)
THE CONDITION FOUND IN THIS EPISODE

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 \(1/2\).

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07Where does the four-dimensional "half" come from?

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 boundarysupertranslation weight\(a\)
3d gravitythe celestial "sphere" is a circle \(S^1\)\(-1\) (one whole direction)\(1\)
4d gravitythe 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.

A WARNING AGAINST TEMPTATION One wants to say "then split it some other way." You cannot. The weight \((-\tfrac12,-\tfrac12)\) is fixed by the requirement that the supertranslations contain the translations of four-dimensional spacetime ── move it arbitrarily and it is no longer BMS₄ but a different algebra. This \(1/2\) is not a coefficient you get to choose; it is a consequence of being in four dimensions.
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08Checking against the literature

Saying "there is none" from my own computation alone would be risky, so I checked. Three independent lines give the same answer.

linewhat 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.

THERE IS ONE REPORTED LOOPHOLE Widen the algebra and the story changes. There are reports that Weyl-BMS (\(\lambda\)-BMS), with a Weyl generator added, has a family of central extensions. But that is not \(\mathfrak{bms}_4\) itself; it is a different algebra with an extra generator ── and I have not checked that line here. Read the condition above, "it closes because the weight is not an integer," as something that added generators may evade.
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09The door that closed, and the door that remains

Let us refill the procedure table placed at the end of Episode 11.

stepcontentstatus
0Positive control. Reproduce the 3d BMS-Cardy in the original papers' conventionpassed (failed once, recovering one bug in the formula)
1Does the supertranslation sector of BMS₄ have a \(c_M\) analogue?the answer is NO. \(\dim H^2=0\)
2aif yes → route A' (a 4d version of BMS-Cardy)closed
2bif no → look for a different templatethe 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.

THE ONE LINE FROM THIS EPISODE THAT WILL MATTER NEXT

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.

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WORK IT BY HAND
  1. Put \(a=1,\,b=0,\,c_m=m^3\) into the cocycle condition \((m-n)c_{m+n}-(an+m+n+b)c_m+(am+m+n+b)c_n=0\) and check it holds at \((m,n)=(2,1)\).
    show the answer
    With \(a=1,b=0\) the condition is \((m-n)c_{m+n}-(m+2n)c_m+(2m+n)c_n=0\). At \((m,n)=(2,1)\), putting \(c_3=27,\,c_2=8,\,c_1=1\) gives \((2-1)\cdot27-(2+2)\cdot8+(4+1)\cdot1=27-32+5=0\). It holds. This is the identity supporting the three-dimensional \(c_M\).
  2. At the same \((m,n)=(2,1)\), what happens if you put \(c_m=m^3\) into \(a=1/2,\,b=-1/2\) (bms₄)?
    show the answer
    The coefficients are \(an+m+n+b=\tfrac12+3-\tfrac12=3\) and \(am+m+n+b=1+3-\tfrac12=\tfrac72\). So \((2-1)\cdot27-3\cdot8+\tfrac72\cdot1=27-24+3.5=\mathbf{6.5}\neq0\). It is violated. One line of hand calculation shows that \(m^3\) is unusable in four dimensions ── the first of the text's "388 places."
  3. Why is the coboundary \(c_m=((a+1)m+b)\beta\) "not physical"?
    show the answer
    Because it appears from merely redefining a generator as \(T_0\to T_0+\beta Z\). Physics does not depend on how generators are named, so a central term that can be removed by renaming carries no physical information. That is why \(H^2\) quotients it out. Conversely, a central charge with \(H^2\ne0\) cannot be removed by any renaming ── which is why it can be a physical quantity.

What we learned in this episode

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 1Episode 2Episode 3Episode 4Episode 5Episode 6Episode 7Episode 8Episode 9Episode 10Episode 11Episode 12 | bonus: ── 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.