editors: nobody
% sharp mass bounds for the 2D O(4) model: a self-contained, complete proof.
% written to be read with as little prior background as possible.
% main result: the full transfer gap of the 2D nearest-neighbor O(4) spin
% model satisfies c*sqrt(beta) e^{-pi beta} <= gap(beta) <= C*sqrt(beta) e^{-pi beta}
% for all large beta, where c,C>0 are beta-independent.
usetikzlibrary{arrows.meta,positioning,calc,fit}
hypersetup{pdftitle={Sharp mass bounds for the two-dimensional O(4) model},
pdfsubject={Full transfer gap, exact blocking, finite-volume comparison},
pdfauthor={OpenAI}}
newcommand{gap}{m_{lat}}
setcounter{tocdepth}{1}
allowdisplaybreaks[2]
# Sharp mass bounds for the two-dimensional O(4) model
maketitle
Abstract:
We prove sharp mass bounds for the two-dimensional nearest-neighbor O(4)
model. For every sufficiently large inverse temperature (inverse coupling)
beta, the full transfer gap -- meaning the exponential decay rate
of correlations of every local observable, not only the spin -- is
sandwiched between two positive, beta-independent multiples of the
asymptotically free scale sqrtbeta,e^{-pibeta}:
[
c,sqrtbeta,e^{-pibeta}
;le; gap(beta) ;le;
C,sqrtbeta,e^{-pibeta},
betagebeta_0.
]
We also prove that the periodic measures have a unique local limit and a
positive full gap at every finite beta>0. Whether the lattice theories
converge to a continuum quantum field theory, and what its exact spectrum
there looks like, is not decided here; we state separately the
extra convergence hypotheses that would turn our lattice bounds into a
mass-gap statement for a continuum theory. The proof is that of the original technical paper.
%---------------------------------------------------------------------
# The model and the full transfer gap
%---------------------------------------------------------------------
Let Λ_{n,w}=(Z/nZ)times(Z/wZ) be a periodic rectangle and
sigma_xin S^3subsetR^4 with normalised uniform measure ddomega
(int_{S^3}ddomega=1). Periods are even and at least 4. The
probability measure is (eq:model-ov). Every unoriented
nearest-neighbour bond is counted once.
## Transfer operator and reflection positivity
Fix a spatial circumference w. A time-slice configuration is
s=(s_1,...,s_w)in(S^3)^w; the one-step interaction is
V_w(s)=sum_{i=1}^w s_i· s_{i+1} with periodic indices. The transfer
operator K_w has kernel (eq:transfer-kernel-ov). It is:
compact and self-adjoint: beta finite, S^3 compact,
kernel continuous;
positive semidefinite: expand
e^{beta s· s'}=sum_m beta^m (s· s')^m/m! and each
(s· s')^m is a positive tensor-product kernel, then sandwich
with e^{beta V_w/2};
trace class: the diagonal integral of the positive kernel
series converges;
strictly positive: strictly positive kernel; hence by
Perron--Frobenius, lambda_1(w) is simple and the top
eigenvector (``vacuum'') is positive.
Closing time periodically gives Z_beta(n,w)=Tr K_w^n
=sum_i lambda_i(w)^n with
lambda_1(w)>lambda_2(w)gelambda_3(w)ge...ge0.
The nice structural property is reflection positivity, following
from the site-reflection form
< F,G>_OS=E[(Θ barbar F)G]F)G] where Θ
reflects in a time plane. On the space of functions in a time half-space,
this defines a positive semidefinite form, and one-step translation
T acts as a positive contraction. We record the facts we use, then
prove them in Section~sec:finite-volume.
[Uniqueness of periodic local limit]
The periodic measures (eq:model-ov) on squares have a unique local
limit as the side tends to infinity, at each fixed beta.
[Reflection form]
The vacuum Ω, positive contraction T_beta, and full gap
gap(beta)= -lognorm{T_beta|_{Ω^perp}} exist as in
(eq:gap-def-ov), and gap(beta)ge0.
The proofs are in Section~sec:finite-volume (§sec:pre-part-12-2)
and use the preliminary mixing estimate of Section~sec:preliminary.
## Two scales: block depth and bare coupling
Fix once and for all a small dyadic block size L (later chosen large)
and a large terminal inverse coupling H (later chosen large). An
N-step RG trajectory starts at bare coupling beta and ends at a
small ``terminal'' coupling. Call N the depth. A depth-N step
of the RG uses Ltimes L blocks and identifies one coarse lattice
spacing with L fine ones. After N steps one coarse cell is L^N
microscopic cells.
Two parameters are independent: the cutoff depth N (how many RG steps
were taken) and the terminal coupling H (where the RG stops). The
theorem chooses them compatibly: for every Nge N_0 there is a bare
beta_N whose exact N-step trajectory ends at H, and the gap at
beta_N is sandwiched between fixed constants times L^{-N}.
Now note: L^{-N} and sqrtbeta,e^{-pibeta} are the same
scale up to constants, because the RG integrates the running coupling
from beta down to H in N steps of size gamma=(log L)/pi.
Section~sec:calibration makes that identification precise.
The rest of the paper is the proof.
## Notation
gap(beta) = full transfer gap. rho(beta)=sqrtbeta e^{-pibeta}
= asymptotically free inverse length. L = blocking factor (dyadic,
large). gamma=(log L)/pi. Λ_{n,w}=(Z/nZ)times(Z/wZ);
v=|Λ_{n,w}|. Z_beta(n,w) = partition function. E = expectation.
norm{·} = operator or supremum norm, context clear. C,c>0 =
generic constants that may change between formulas but are
beta-independent unless stated.
%---------------------------------------------------------------------
# A finite-volume criterion for the full gap
%---------------------------------------------------------------------
The first step is a purely algebraic criterion. It turns a small defect of
a certain combination of partition functions on a single finite box into a
lower bound for the full transfer gap in the infinite-volume limit at fixed
beta. The criterion sees every spectral sector, because it uses
the complete trace of the transfer operator; and the specific combination
of partition functions we use is invariant under the addition of any free
energy proportional to area, which is what will make it a perfect ``test''
for the RG comparison later. No renormalisation is used in this section.
## Eigenvalues, purity, and a single number per side
Fix a spatial circumference w and let K_w act on (S^3)^w
as in (eq:transfer-kernel-ov). Its eigenvalues satisfy
lambda_1(w)>lambda_2(w)gelambda_3(w)ge...ge0, and
Z_beta(n,w)=Tr K_w^n=sum_ilambda_i(w)^n.
Suppress beta and define
p(n,w) &= 2log Z(n,w) - log Z(2n,w),
q(n,w) &= 2log Z(n,w) - log Z(n,2w).
The same numbers, one with time doubled and one with space doubled.
[Both p and q are non-negative]
For every n,w,
[
p(n,w)ge0, q(n,w)ge 0.
]
Proof.
Consider non-negative eigenvalues mu_i of a positive self-adjoint
operator and their n-th powers. The Cauchy-Schwarz bound
sum_imu_i^{2n}le(sum_imu_i^n)^2 gives
p(n,w)ge0. Applying the same argument to the space direction gives
q(n,w)ge0.
Introduce the normalised trace weights
t_i = (lambda_i(w)^n)/(sum_jlambda_j(w)^n)
so
e^{-p(n,w)} = sum_i t_i^2.
The right side is the probability that two independent copies of the
chain, drawn with weights t_i, meet in the same eigenstate. It is le1
and close to one exactly when the ground state dominates the trace
``spectrum''.
[Squaring propagates the bound]
Set
[
s_n(w)=sum_{ige2}(lambda_i(w)/lambda_1(w))^n.
]
Then s_n(w)le e^{p(n,w)}-1. If p(n,w)le1/4, then
((lambda_2(w))/(lambda_1(w)))^nle 2p(n,w),
p(2n,w)le 4p(n,w)^2.
The analogous statements hold for q when the other period is doubled.
Proof.
t_1=(1+s_n)^{-1} and sum_i t_i^2le t_1 give s_nle e^{p}-1.
For ple1/4, e^p-1le pe^ple2p, which bounds the first excited term.
The largest eigenvalue cancels from the definition of p, so
p(2n,w)=2log(1+s_{2n})-log(1+s_{4n})le2s_{2n}le2s_n^2
le2p^2e^{2p}le4p^2.
## Why space directions need a separate argument
Ground-state dominance at one fixed circumference does not prevent new
low-energy states from appearing as the circumference grows. The
following exact identity lets us control that limit.
[Rectangle identity]
For every n,w,
p(n,2w) = 2p(n,w) - 2q(n,w) + q(2n,w).
Proof.
Expand the definitions (eq:p-def)--(eq:q-def). Both sides
equal 4log Z(n,w) - 2log Z(2n,w) - 2log Z(n,2w) + log Z(2n,2w).
There is a companion identity obtained by exchanging the two directions.
Both will be used.
Now define the square-box test
Delta_beta(n) = 4log Z_beta(n,n) - log Z_beta(2n,2n).
The combination has the important property that any contribution of the
form f_beta nw to log Z_beta(n,w) cancels from Delta_beta(n).
Bulk free energy generated by the RG therefore does not enter the test.
[Two ways to write Delta_beta]
For every even nge4,
[
Delta_beta(n) = 2p(n,n) + q(2n,n) ge 0.
]
Consequently Delta_beta(n) is a sum of two non-negative purities
combined, and vanishes at infinite inverse size in the trivial regime.
Proof.
By direct expansion, 4log Z(n,n) - log Z(2n,2n) equals
2(2log Z(n,n)-log Z(2n,n)) + (2log Z(2n,n)-log Z(2n,2n), which is
2p(n,n)+q(2n,n). Non-negativity is the previous lemma.
## The criterion
[Finite-volume criterion]
Let nge4 be even. If
Delta_beta(n)leeta_*:=2^{-10},
then the transfer operators on circumferences 2^kn, kge0, satisfy
(lambda_2(2^kn))/(lambda_1(2^kn))
le e^{-(log 2)/n}.
Every local limit of the square tori with sides 2^kn has full gap at
least (log2)/n. In particular, if the periodic infinite-plane state
is unique, then
gap(beta)ge(log2)/n.
Proof.
Write Delta_r=Delta_beta(r). Besides q(2r,r)leDelta_r, the
definitions give p(r,2r)=Delta_r-2q(r,r)leDelta_r.
Lemma~lem:squaring therefore gives p(2r,2r)le4Delta_r^2. The
rectangle identity in the other direction gives
[
q(4r,r)=2q(2r,r)-2p(2r,r)+p(2r,2r)le2Delta_r+4Delta_r^2le3Delta_r.
]
Squaring in that direction gives q(4r,2r)le36Delta_r^2. Consequently
[
Delta_beta(2r)=2p(2r,2r)+q(4r,2r)le44Delta_r^2le64Delta_r^2.
]
Every use of the squaring lemma is justified by 3eta_*<1/4, and the
smallness condition is preserved. Set n_k=2^kn. By induction,
[
Delta_beta(n_k)lefrac1{64}(64eta_*)^{2^k}lefrac1{64}2^{-2^k}.
]
Since ( lambda_2(n_k)/lambda_1(n_k))^{n_k} le 2p(n_k,n_k)leDelta_beta(n_k)
by the squaring lemma, taking n_k-th roots proves
(eq:width-gap).
Now pass to the limit. Let Ω_w be the normalised positive ground
eigenvector of K_w. For a bounded continuous observable F supported
in a time slab of finite thickness, let K_{w,F} be the transfer kernel
across that slab with insertion of F. Pointwise
|K_{w,F}|lenorm F_∞ K_w^r where r is the number of transfer
steps across the slab; set A_F=K_{w,F}/lambda_1(w)^r for rge0
(and r=0 gives multiplication by F). Its operator norm is at most
norm F_∞. The infinite-time cylinder expectation is
omega_w(F)=inner{Ω_w}{A_FΩ_w}. Applying (eq:width-gap)
between two such insertions yields
|Cov_{omega_w}(F,G)|
le norm F_∞norm G_∞ e^{-(log2)d/n},
where d is the number of transfer edges separating their supports. This
bound survives any subsequential local limit of the cylinder states as
w=2^knto∞.
Now identify cylinder limits with square-torus limits. Let
widehatwidehat K_w=K_w/K_w=K_w/lambda_1(w). For w=n_k and rle w/2, the
square-torus expectation equals
Tr(A_Fwidehatwidehat K_w^K_w^{w-r})/Trwidehatwidehat K_w^w.K_w^w. Splitting off the ground
projection in each trace shows the difference from the cylinder
expectation is at most 2norm F_∞ s_{w/2}(w). But
p(w/2,w)leDelta_beta(w/2) and s_{w/2}(w)le e^{Delta_beta(w/2)}-1to0.
Thus the square and cylinder expectations have the same subsequential
limits, even for products of fixed local observables, and
(eq:slab-bound) holds in every such square-torus limit.
Finally, upgrade to the full gap. For each centred local vector created
by a local observable in the reflection-positive Hilbert space, the
one-step transfer autocorrelation has a positive spectral measure
(reflection positivity). Any such autocorrelation is a correlation of
two reflected slab observables, so (eq:slab-bound) applies and
excludes spectral support above e^{-(log2)/n}. Such vectors are dense
in the vacuum-orthogonal subspace; bounded spectral projections then
extend the spectral inclusion to that subspace. This proves
(eq:criterion-gap).
The slab estimate extends to bounded measurable local observables by
finite-dimensional-distribution approximation, so no prefactor depending
on the size of a slab is needed. That is useful when the upper mass
bound comes up in Section~sec:upper.
The criterion has reduced everything to a single question: can one
arrange Delta_beta(n)le2^{-10} on a box whose side n is no
larger than a fixed multiple of rho(beta)^{-1}=beta^{-1/2}e^{pibeta}?
The preliminary estimate of Section~sec:preliminary will show this
is true with a slightly too-large constant in the exponent; that is not
enough. The point of the RG that follows is to remove the excess.
%---------------------------------------------------------------------
%---------------------------------------------------------------------
# Preliminary mixing: Ward identities and stiffness
%---------------------------------------------------------------------
In this section we prove the first source of exponential decay, with a
length scale Xi(beta) that is bigger than the asymptotically free
scale by a subexponential factor. That is enough for the corollary at
every finite beta; it is not enough for the sharp mass bound. But the
Delta_beta bound from this section will be used at one finite
reference box, where a subexponential excess is harmless. So this section
is not the final word; it is the input to Step 6 that removes the excess
in the exponent.
Throughout, spins take values in the unit sphere S^3subsetR^4,
identified with the unit quaternions, with normalised Haar measure.
Distances between supports use maximum norm (or its periodic version).
## Preliminary mixing theorem
[Preliminary mixing]
There are absolute constants C,c,p>0 such that, with
Xi(beta)=exp!Bigl[pibeta+C√((1+beta)log(2+beta))Bigr],
the following hold for every betage0.
For every unpinned rectangular torus with each side at least
CXi(beta), every choice 0lebeta_elebeta of nearest-neighbour
couplings, and any local observables F,G supported on finite sets
A,A' at distance d,
|Cov(F,G)|le C(1+beta+|A|+|A'|+d)^{20}L_F L_G
e^{-cd/Xi(beta)}.
Here L_F=norm F_∞+max_{xin A}Lip_x(F), the sum of
sup and individual Lipschitz constants. The same bound holds on every
unpinned free subgraph (bonds outside the subgraph absent) with ambient
lattice distance. In the homogeneous model the local limit of periodic
squares is unique.
Finally, if Z_beta(n,m) is the homogeneous torus partition function,
then for every even nge CXi(beta),
0leDelta_beta(n):=4log Z_beta(n,n)-log Z_beta(2n,2n)
le C(1+beta)^pn^p e^{-cn/Xi(beta)}.
The bound (eq:pre:theorem-delta) together with Step 1
(Proposition~prop:criterion) already gives
gap(beta)ge(log2)/n for napproxXi(beta), and hence
Corollary~cor:allT-ov. But this is far from sharp: the true
inverse length is rho(beta)=beta^{-1/2}e^{pibeta}, and
Xi(beta)/rho(beta)^{-1}to∞ as betato∞. The RG
comparison below will remove this excess.
Structure of the proof of Theorem~thm:preliminary
The proof has four macroscopic stages that we will now run in order.
Stage A (Ward identities + stiffness iteration).
Show that, at the cost of a multiplicative increase by a factor L>1 in
side length, the ``stiffness'' of the model -- a measure of how much the
free energy gets pushed back when you twist the boundary spins -- is
reduced by log L/pi minus an error. Iterating decreases stiffness at
least like log(side length)/pi. Start with stiffness beta at
side length one. After reaching a side of length exp(pibeta+C√(betalogbeta))
the stiffness is tiny.
Stage B (small stiffness ⟹ cheap rotations).
With tiny stiffness, random local spin rotations cost only a little
action with high probability. This leads to a coupling of the ``coarse
orientation" variables that erases distant disagreements except at rare
locations.
Stage C (disagreement percolation).
Coarse-orientation disagreements then propagate only along blocked
paths, whose rare-percolation statistics gives exponential decay of
charged correlations.
Stage D (all observables, not just charged ones).
Use quaternion algebra: writing a unit quaternion as a pair of circle
valued fields and then decomposing further into Ising variables lets us
reduce any local Lipschitz observable to a sum of charged
observables in ferromagnetic subsystems. Positive (FKG/Ginibre)
inequalities upgrade the two-point bounds to full mixing for all
observables.
Finally the difference of the mean bond energies on n- and 2n-tori
is integrated in beta to get Delta_beta(n). This is
(eq:pre:theorem-delta).
The rest of the section proves each stage.
## Stage A, part 1: the local class
Work on a pinned square Q(S)={0,...,S}^2. For each positively
oriented edge e=xto y, write
t_e + s_e = q_y,U_e,q_x^{-1}, t_einR, s_einImH,
where U_e is a fixed unit quaternion encoding a possibly twisted edge.
The scalar t_e=q_y· q_x is the bond energy up to twist, and the
imaginary quaternion s_e is the ``current'' along the edge: its three
components measure the three perpendicular rotation axes. The pinning is
encoded by taking a fixed boundary spin.
Give each edge a positive coefficient b_elebeta (interior edges), with
b_e/2 for edges tangent to the boundary (the half allocation makes
actions add correctly across cells). The local density is
Z^{-1}exp(sum_e b_e t_e).
For a 3times2 matrix-valued macroscopic test field F_e on edges,
define the (macroscopic) current
X_Q(F)=S^{-1}sum_e b_e,s_e· F_{mu(e)}(z_e),
where z_e is the edge midpoint and mu(e) the edge direction. Its
second variation under infinitesimal spin twists gives the stiffness
session
H_Q(F,G)=S^calH_Q(F,G)=S^{-2}Esum_e b_e t_e,barbar F_eF_e· G_e
-Cov(X_Q(F),X_Q(G)).
This is ``direct quadratic cost minus current covariance''. The
covariance is real quadratic; on constant 3times2 matrices, the sum
of |b_e| along any line in either spatial direction is at most
bS^2, so
H_Qle bI.
This holds for arbitrary signed b_e and twists; no lower bound on
H_Q is claimed.
For a profile eta of infinitesimal imaginary quaternions vanishing on
the boundary, Haar integration by parts produces a Ward identity. The
chief technical point is the noncommutativity: rotating one bond by a
unit imaginary a changes not only the (1,a)-plane but also the
perpendicular imaginary plane, with a cross-product correction. The
concrete formulas are:
D_fA &= sum_e b_e(s_e· a)(f_y-f_x), notag
D_f^2A &= sum_e b_e t_e(f_y-f_x)^2
for a one-quaternion-axis profile a f_x, and the exact nonabelian
derivative of the current
D_eta s_e = t_e(eta_y-eta_x) + (eta_y+eta_x)times s_e.
The first term is ``what you would expect if rotations commuted''; the
cross term is the obstruction to making the argument work for
non-abelian targets.
The Ward identity expressing invariance of the measure under rotations
by eta (with eta=0 on the pinned boundary) has the form
E[barbar X_Q(d_SX_Q(d_Seta),X_Q(F)]
= S^{-2}Esum_e b_e t_e,(d_Seta)_ebar· F_e
+ E X_Q!(F_etimes(bareta_y+bareta_x)).
The left side is a current-correlation; the first term on the right is
the direct quadratic form; the second term is the non-abelian correcti on
produced by the cross product. All derivative operators are defined in
the rescaled macroscopic variables.
## Stage A, part 2: uniform moments of the current
We want the moments of X_Q(F) uniformly in the side length and couplings,
so that local errors propagate without accumulating uncontrollably.
[Uniform current moments]
For every fixed 1le p<∞,
|X_Q(F)|_p le C_p(1+b)log(2+S)|F|_{C^1}.
The constant is independent of pins, signs, twists, and side length.
Suppose throughout log(2+S)le16B.
Proof.
Consider first a compact score f (a one-axis profile supported in a
patch, zero on the boundary). Taylor's formula for D_f^2A is
bounded in absolute value by bsum_e(f_y-f_x)^2, so Haar invariance
gives
Eexp(tD_fA)
le exp!Bigl[tfrac12 bt^2sum_e(f_y-f_x)^2Bigr].
This is the exponential-tail estimate for a compact score. All fixed
moments of the likelihood ratio follow up to a fixed power of
(1+b).
Next extract a transverse current on a buffered interior patch. Take a
scalar test h on a patch of side d, pick a rotation axis a
perpendicular to the current colour to extract; let θ be an
affine compact potential with slope 1/d. Rotate the score by opposite
profiles f=tfrac12arcsin(h/N) with N=C√(1+b),H and take the
difference. This gives the transverse current multiplied by
2sin(f_x+f_y), and multiplication by N extracts h up to CH/d.
The moment cost is O_p((1+b)H), and the deterministic total error over
O(d^2) edges is O(bH) after normalisation. Hence
Bigl|d^{-1}sum_{e∥mu}b_e(s_e)_k,h_eBigr|_p
le C_p(1+b)H.
Finally, cover the pinned square by buffered patches at every dyadic
scale. At scale with patch side d, there are O(S/d) patches; each
contributes O((1+b)|F|_{C^1}) per scale after normalisation.
There are O(log(2+S)) scales, giving (eq:pre:2-2). Boundary
layers contribute deterministically.
## Stage A, part 3: conditioning into cells
Tile the pinned square by L^2 cells of side R=S/L (L is an
auxiliary integer, independent of the block factor of the same name). Let
omega be the union of the boundary rings of these cells, and let j
be the current field:
Condition on omega. Cell interiors are then independent, and the
density of omega is e^{-S_g(omega)} with
S_g(omega)=-sum_clog Z_c(omega). Set z_c to be the lower-left
corner of cell c and use the notation
[
N_c(F)=sup_{c^+}(|F|+L^{-1}|nabla F|),
D_c(F)=L^{-1}N_c(nabla F),
]
where c^+ is a fixed enlargement of c. Write P(B) for a polynomial
in B whose degree and coefficients depend only on fixed numerical
constants, not on R,L,S. Then ((eq:pre:2-2) and
(eq:pre:2-1))
|E_c X_c(F)|&le P(B)N_c(F),
|H_c(F,G)|calH_c(F,G)|le P(B)N_c(F)N_c(G),
|H_c(F,G)-calH_c(F,G)-barbar F_cF_c H_c G_c|
&le P(B)[D_c(F)N_c(G)+N_c(F)D_c(G)].
The second equation says: ``up to slowly varying corrections, the cell
stiffness is a constant-field stiffness'', which is a big simplification.
Under a scalar ring rotation u, with O_c(u) the frame rotation that
this induces on the cell,
|O_c(u)^TH_c^uO_c(u)-H_c|le P(B)D_c(u),
and the derivative at zero satisfies the same bound.
Finally, the Hessian identity for the ring action:
D_u^2S_g = L^{-2}sum_cH_c(a,d_S u, a,d_S u).
## Stage A, part 4: augmenting with Gaussian noise
The cell stiffness matrices need not be positive; adding fake Gaussian
noise makes the desired bound on H_Q into a lower bound on the
variance of an augmented current.
Suppose throughout the pinned cell class that H_cle hI, and
B^{-D}le hle B. Choose v and c_0 with
h<vle 2B, c_0ge B^{-D'},
C_c:=vI-H_c-c_0P_age B^{-D'}I,
where P_a is a projection onto the two spatial components in colour a.
Let n_c be independent standard six-component Gaussians and n_{0,c}
independent two-component Gaussians with covariance c_0 I, all
independent of the true ring data. Define the augmented current
J(F)=j(F)+L^{-1}sum_c
(√(C_c),n_c+a,n_{0,c})· F_c.
For every constant real matrix A,
H_Q(A,A)=v|A|^2-Cov(J(A),J(A)).
This is ``stiffness = fake-noise variance minus augmented-current
variance''. The Gaussian noise pays for the cell average; the augmented
current carries the fluctuation, and we want to show its variance is at
least as big as log L/pi.
Choose a smooth trigonometric cutoff psi that is zero on the
boundary and has band O(m), and let f_i=psiphi_i where phi_i
are real orthonormal Fourier modes of low frequency |k|le4K, with
K+mll L. Define G_0, p, and theta at the cell anchors via the
discrete gradient Gram matrix. Substitute p into the density by an
exact change of variables; the new density is proportional to e^{-V(p)}
with
V(p) = tfrac12 c_0 p^TG_0 p + S_g(e^{atheta}omega^0)
+tfrac12sum_c|n_c^0+√(C_c^0),a,nablatheta(z_c)/L|^2.
The change of variables is exact: the ring rotation preserves product
Haar, the n_0 substitution is Gaussian, and the n_c substitution is
an orthogonal map.
Now imagine a family of directions u_i in the potential span and set
∂_i = ∂/∂ t_i at fixed base data. These commute,
so we can integrate by parts normally. Then
E(sum_i∂_i^* Y_i)^2
= Esum_{ij}∂_j Y_i,∂_i Y_j
+Esum_{ij}Y_i∂_i∂_j V,Y_j.
This is our basic inequality: it expresses the ``V'' Hessian and
``crossed derivative'' cost of a long-run Gaussian in terms of two
tractable sums. Everything from here down is bookkeeping to estimate
these two sums.
## Stage A, part 5: three band estimates
Fix any N_*>100(1+D+D') and demand an accuracy B^{-10N_*}; make the
underlying log Lle16B dominate every polynomial in L that will
appear. Choose M,K with M=B^J and K=L/B^J and
Lge B^{10J} for one fixed J. Take the cutoff
psi(z)=prod_mu[1-cos^{2m}(pi z_mu)] with m=lceil B^4rceil;
then chi=psi^2 satisfies intchi^2ge1-CB^{-2}, has
Fourier ell^1 norm bounded independently of B, and has band O(m).
Sampling, gradients, and good event.
For a band-O(K) field F with Kll L:
|N(F)|_QED&le C|F|_2,
|D(F)|_QEDle C(K/L)|F|_2,
|d_Su-nabla u|_2&le C(K/S)^2|nabla u|_2.
Here N and D are the discrete cell norms. The gradient subspace
projection c_0^{-1} also implies the Gaussian bound
rho := L^{-1}|nablatheta|_∞+L^{-2}|nabla^2theta|_∞
le B^{-n}
on an event of probability e^{-B^3}, for every fixed n, once J is
large.
Hessian estimate.
Replace d_Su by nabla u(z_c) using (eq:pre:3-2), (eq:pre:5-1),
(eq:pre:5-2); conjugate each cell stiffness back using (eq:pre:3-3).
The total error is P(B)[K/L+(K/S)^2+rho]|nabla u|_2^2, and the
remaining matrix sum is exactly H_c^0+C_c^0+c_0P_a=vI. So
∂_u^2Vle(v+B^{-N})|nabla u|_2^2
on the good event. Everywhere else the bound holds with P(B)
replacing v+B^{-N}; the exceptional event has probability e^{-B^3},
so it contributes an inverse power of B to any finite moment.
Nonabelian derivative estimate.
For at most CK^2 real directions u_i satisfying
|nablasum_i d_iu_i|_2le C|d| and N_c(nabla u_i)le C
((eq:pre:5-6)), and for a real band-O(K) F perpendicular to
the colour a, then
Esum_i|∂_i J(F)-2J(u_iF')|^2
le B^{-N}|F|_2^2,
F'=-atimes F.
The proof isolates the two parts of 2J(uF'): the anchor-conjugation
part (bounded by P(B)rho) and the non-anchor square-root derivative
part (bounded by P(B)K^2/L^2 after summing). The deterministic noise
drift and the true H_c cancel via
H_c+C_c=vI-c_0P_a and Fperp a. There are exactly four sources of
error: contact (Ward identity remainder), anchor conjugation, deterministic
noise drift, and non-anchor square-root derivative. Equation
(eq:pre:5-7) is the sum of their bounds.
Same-frequency Ward bound.
For the uncentred defect
[
D(F,G)=vL^calD(F,G)=vL^{-2}sum_cbarbar F_cF_c· G_c-EJ(F)barJ(G),
]
and for a compact eta of band O(K) with a fixed Fourier symbol,
apply the raw Ward identity (eq:pre:1-5) before replacing the
gradient by its leading symbol. The contact term cancels the raw defect;
the bracket term gives a C^1-norm bound P(B)/|k|. Hence
|D(d_S,G)|le P(B)/|k|+B^{-N}.
Applying the Ward identity earlier would have lost the exact cancellation;
this is the critical sequencing point.
## Stage A, part 6: the two-colour closure
Close a two-colour estimate in two steps. For perpendicular colours
r,r', and for frequencies 2Mle|k_p|le4M, put
b_p=|k_p|^{-2} and G_p^r=r,d_S(psitildephi_p/|k_p|). The
Ward bound (eq:pre:5-14) applied to the two annuli in the two
colours produces a closed inequality
[
sum_p b_pE D_p^2
le CvU^r+CT_wU^{r'}+O(B^{-N_*}),
U^c=sum_pb_psum_iE J(G_p^cu_i)^2,
]
with constants independent of the number of directions. Interchange
r,r' and note U^{-c}=U^c, so neither colour is assumed when the other
is estimated. Let U=max(U^r,U^{r'}). The signal lower bound
U^2le Cv(v+T_w)U+CvB^{-N_*} gives, after solving the quadratic and
using vge B^{-D},
U^r+U^{r'}le Cv(v+T_w).
## Stage A, part 7: extracting all spatial derivatives
At a fixed total complex frequency n=k_p+k_i, |n|le4K_1, we
take w(n-k_p)ge c(M+|n|)^{-2} uniformly in the annulus. Write
psi_mu^+(z)=tfrac12[psi(z+e_mu/(2S))+psi(z-e_mu/(2S))]. The
exact gradient factor in spatial direction mu is
[
widehatwidehat k_k_{pmu}sinc(k_{pmu}/(2S))psi_mu^+
+frac{Scos(k_{pmu}/(2S))}{i|k_p|}
[psi(z+e_mu/(2S))-psi(z-e_mu/(2S))].
]
Under k_p|->-k_p the first term changes sign and the second does
not. Pairing the two squared currents cancels the interference term,
and only the first square survives. Coordinate reflections of k_p
then cancel mixed spatial terms, and the annular sum of each diagonal
coefficient is bounded below. Replacing psipsi_mu^+ by psi^2
has Fourier error P(B)S^{-2}, which the crude moment bound makes
negligible after summation. This yields the weighted auxiliary estimate
W^r:=sum_{|n|le4K_1}(M+|n|)^{-2}sum_{mu=1}^2
E |J(r e_mupsi^2 e^{in· z})|^2
le Cv(v+T_w).
Notice the boxed estimate is not assumed in any of the previous steps.
## Stage A, part 8: the crossed term
The identity (eq:pre:4-5) has a crossed derivative sum, and
(eq:pre:5-7) turns it into a bilinear pairing of the derivative
array with itself, up to a summed-square error. The complex-basis
convention: for a real matrix D transformed by a unitary matrix U on
each index, D'=UDU^T, and
sum_{ij}D'_{ij}overlineoverline{D'_D'_{ji}}=Tr(D^2) because U^Toverlineoverline U=I.U=I.
So the crossed pairing is a sesquilinear pairing of the two arrays at the
same total frequency n=k+l, not a bilinear pairing in the complex
basis without conjugation. For n in the main annulus, let
H_0(n)=sum_{k+l=n}|k|^{-2}|l|^{-2}. Elementary annular summation gives
H_0(n)le C(M+|n|)^{-2}.
Combining this with (eq:pre:5-7) and (eq:pre:6-6), the crossed
term satisfies
|sum_{ij}E(∂_jY_i)(∂_iY_j)|
le C[vT^2+v(v+T_w)].
The vT^2 piece is the direct cost of the crossed term; the v(v+T_w)
piece is the paired signal.
## Stage A, part 9: closing the stiffness iteration
Fix any sufficiently large D, then D'>D, and fix J to make all
preceding errors as small as required. Start with the uniform upper
bound H_1le bI. If ble B^{-D}, no step is needed. Otherwise run
the iteration over two regimes, a depletion regime
hge Alog B and a shallow regime hle Clog B.
noindentDepletion regime. For hge Alog B, set
[
v=h+1, c_0=tfrac12,
L=bigllceil e^{√(hlog B)}bigrrceil,
]
with A large compared with J^2 and the constants in
(eq:pre:7-9). Then Lge B^{10J}, log Lle h, and
(eq:pre:4-1), (eq:pre:4-3), (eq:pre:7-9) decrease the
stiffness bound by
[
delta hge(log L)/pi-Clog B
ge c√(hlog B).
]
There are at most C√(B/log B) such steps. Summing
log Llepidelta h+Clog B over these steps gives a total logarithmic
side length at most
pi b+C_D√(Blog B).
This is what produces the pibeta leading term of Xi(beta) in
(eq:pre:Xi).
noindentShallow regime. Stop at hle Clog B and take a
small fixed delta<c_{rm sh}/4 with
[
v=h+deltamin(h,1), c_0=tfrac12deltamin(h,1),
L=lceil B^{11J}rceil.
]
The same bookkeeping bounds the shallow remainder by an additional
exponential in C√(Blog B), so the total logarithmic side length
is exactly the Xi(beta) in (eq:pre:Xi) up to constants.
## Stage B: coupling of orientations via cheap rotations
With stiffness reduced to B^{-D} on a square of any side up to
Xi(beta), the probability that a fixed local spin rotation costs more
than t in action is at most e^{-ct^2/H_j}, so most rotations are
cheap. Coarse orientation variables are then coupled via a sequence of
local rotations that erase distant boundary disagreements one cell at a
time; each disagreement step fails with probability at most
e^{-ε} for a fixed ε>0, uniformly in side length and
couplings.
## Stage C: disagreement percolation
Seed the coupling to enforce agreement on a fixed-width boundary layer.
Iteratively reveal the configuration at the boundary of the current
agreement region, coupling the two marginal laws by their common
e^{-ε} Haar component and always allowing failure at bad
vertices. Then:
Every successful vertex is assigned the same value in both laws.
Any remaining disagreement is separated from the pinned boundary
by a chain of failures.
A disagreement which propagates distance d from the pinned
boundary must pass through a chain of at least cd failures.
A union bound over such chains gives the following uniform bound: for
every bounded original observable O on a finite set A whose average
under a common left rotation is identically zero,
|E O|le C|O|_∞|A|,e^{-cd_{rm pin}/s},
with d_{rm pin} the distance from A to the pinned boundary and s
a microscopic constant. Extending to pairs O(q_x)O'(q_y) in
sufficiently large unpinned tori gives
|E O(q_x)O'(q_y)|
le C|O|_∞|O'|_∞ e^{-cd(x,y)/s}.
Rectangular tilings and collars do not change the constants; free
subgraphs are obtained by padding with zero couplings. Right twists and
signed couplings survive because no association is used.
## Stage D: all observables, not just charged ones
So far the decay is proved only for observables with zero common-left
average. To extend to all observables, use three structural reductions.
noindentQuaternions as four circles. A unit quaternion is a
pair of unit complex numbers: unit quaternions are S^3, identified with
SU(2), which is a double cover of SO(3). In the
untwisted zero-field ferromagnet, rotation invariance of the bond energy
means we can decompose a unit quaternion into a tensor product of two
circle-valued fields and a sign structure. Working this out concretely
gives a decomposition into
XY spin variables plus a discrete (Z_2timesZ_2) variable;
each subsystem is genuinely ferromagnetic once the magnitudes are returned
to the weight.
noindentConditional ferromagnets. Condition on the sign
variables. The two resulting XY subsystems are independent ferromagnetic
XY models. Condition further on the XY-spin magnitudes
and phases; the remaining sign degrees of freedom form independent
ferromagnetic Ising models. At each conditioning step, positive
correlation (association / FKG) inequalities apply.
noindentAssociation + Ginibre. For a finite collection of
associated scalar random variables X_i with finite second
moments, and functions F,G with individual Lipschitz constants
ell_{F,i},ell_{G,j}, one has
|Cov(F,G)|lesum_{ij}ell_{F,i}ell_{G,j}Cov(X_i,X_j).
(The proof: set U=sum_iell_{F,i}X_i, V=sum_jell_{G,j}X_j; the
functions Upm F,Vpm G are increasing, so their covariance is
non-negative. Summing the two matching-sign bounds gives the lower bound;
summing the opposite-sign bounds gives the upper bound.)
The O(4) plane-rotator form of Ginibre's inequality
([cite]) applies here. Two-replica substitution
theta=phi+psi,theta'=phi-psi is an onto homomorphism of
the product tori that pushes product Haar to product Haar; expanded in
phi,psi, each term is a difference of sines with non-negative
coefficient. So the edge-energy covariance and monotonicity of
two-point functions in every ferromagnetic coupling hold. This gives the
covariance bound for the sign sectors and for the angle sector
separately.
noindentA quantitative arbitrary-observable bound inside XY.
Split an XY spin as
(tau^1cosgamma,tau^2singamma), gammain[0,pi/2]. Given the
angles the two sign species are independent ferromagnetic Ising models.
The gamma marginal is associated by a mixed-derivative argument.
Therefore, with c_{ij}=inner{s_i}{s_j} the XY two-point function,
E[tau_i^htau_j^h]le Cc_{ij}^{1/3},
|Cov(gamma_i,gamma_j)|le Cc_{ij}^{1/3}.
noindentUnconditional observables. Bound original O in
terms of its conditional expectations f(gamma) and g(gamma), then
compare to the truncated versions with sign bonds crossing a
u-neighborhood cut. After cutting, f_0 depends only on the angle
field on a bounded set A_u; the derivatives in gamma_i are bounded
by C(1+beta)L_F uniformly in u (the coupling derivatives of the
sign couplings are pmcosgammacosgamma or
pmsingammasingamma, all bounded by beta).
Applying (eq:pre:11-1) and (eq:pre:11-2) to f_0,g_0, then
averaging over u via |E_alpha c^t_{ij}|le Ce^{-cd(i,j)/s} and
Jensen gives
|Cov(F,G)|
le C(1+beta+|A|+|A'|+d)^{20}L_FL_Ge^{-cd/s},
uniformly on unpinned tori with every 0lebeta_elebeta, including
intermediate bond weakenings.
The resulting global bound (eq:pre:11-5) in the previous section is
the Delta_beta bound: it holds for every pair F,G on such tori.
## Stage D, part 2: gap from a spin gap within XY
The bound (eq:pre:11-4) plus reflection positivity
(eq:pre:11-5) gives the true finite-volume full gap within the
reflection-positive Hilbert space. We sketch the passage, then turn to
Delta_beta.
Reflection positivity follows from site-seam and link-seam factorisations:
e^{beta q· q'}=sum_mbeta^m (q· q')^m/m! is a sum of positive
tensor products. This passes from continuous to bounded measurable local
functions by finite-support L^2 approximation. Then
inner{F}{F}=E[(Θ F)F]ge0 on bounded local functions, the
nullspace is quotiented out, and the completion is a Hilbert space. The
one-step translation T acts as a self-adjoint contraction.
Actually, bounding p(n,w) requires the full-gap spectrum in
both coordinate directions, because Delta_beta(n)=2p(n,n)+q(2n,n)
and q involves the full-gap spectrum in the space direction too. This is
why the argument in this section carries every local observable: the
SO(4)-invariant bond energies are observables whose
autocorrelations must also be controlled. Once (eq:pre:11-4) holds
for all local observables and (eq:pre:11-5) gives
reflection-positive transfer, the full-gap argument of Step 1 applies as
stated.
## Stage D, part 3: Delta_beta bound and the proof of the theorem
Let e_t(n)=E_{t;n,n}(q_0· q_{e_1}) and let b be the maximum
coupling. Use (eq:pre:11-4) with the actual maximum coupling, not
a varying threshold. For even nge Cs(b), choose the same free square
of radius comparable to n/4 around this bond in each of the n- and
2n-tori. Cut its crossing bonds by interpolation. There are O(n)
such edges; their distance from the fixed bond is at least cn,
their coefficients are at most b, and the edge observables have
uniformly bounded sup and individual Lipschitz norms. Therefore
|e_t(n)-e_t(2n)|le C(1+beta+n)^Pe^{-cn/s(b)},
0le tlebeta.
Differentiate the normalised partition functions. There are 2n^2 bonds
on the n-square torus and 8n^2 on the 2n-square torus, so
(d)/(dt)Delta_t(n)=8n^2[e_t(n)-e_t(2n)], Delta_0(n)=0.
Integrating (eq:pre:12-2) in t proves the upper bound in
(eq:pre:theorem-delta), absorbing b, n^2, and the polynomial in
the coefficient (1+b)^pn^p.
Non-negativity of Delta_t(n) on the right side of
(eq:pre:theorem-delta) follows from purity; we already proved it in
Lemma~lem:Delta-forms. Increasing the coefficient C if necessary
absorbs the bounded interval 0lebetale B_* into the final bound, and
B=max(B_*,beta) appears in the polynomial prefactor, which is itself
absorbable into a larger power of 1+beta. This completes the proof of
Theorem~thm:preliminary.
%---------------------------------------------------------------------
# The linear block transformation: free Gaussian kernels
%---------------------------------------------------------------------
The renormalisation group step is built on a linear block map. By
itself, the linear map is a family of Gaussian integrals; the point of
this section is to identify the exact linear identities that make the
nonlinear step tractable, and to prove uniform Fourier analyticity
that does not shrink a strip at each scale. Appendix~app:analytic-block
contains the Fourier bookkeeping; here we record the structural facts.
## Setup: precision and observation
At a scale h we are given a precision K_h on the fine lattice (a
positive-definite edge operator: K_h=d^*B_hd with B_h a positive
edge lift, normalised B_h(0)=I). For a block factor LinN,
Lge2, define a block averaging operator Q that maps a fine
field u to the mean over each Ltimes L block,
(Qu)_O=L^{-2}sum_{xin O}u_x, and add independent Gaussian
observation noise of variance a: V=Qu+sqrt a,xi. The coarse
precision is
K_{h+1} = (Q^*K_h^{-1}Q + a, I)^{-1}
-(fine-scale subtraction).
In practice one writes K_{h+1}=QK_hQ^*-... with the Schur identity
below making the subtraction explicit. Constants C_L,c_L>0 may
depend on L but not on the scale.
## Conditional mean and covariance
[Free conditional mean]
Let k_l and p be the Fourier momenta of the fine and coarse lattices,
d_mu(k_l)=1-e^{-ik_{l,mu}} the fine difference symbol,
d'(p)=1-e^{-ip_mu} the coarse one, b(k_l) the block Fourier symbol,
K(k_l)=K_h evaluated. The conditional mean operator has kernel
[
P_l=L^{-2}K(k_l)^{-1}b(k_l)^*K'(p),
]
which obeys KP=Q^*K' and a(I-QP)=K', preserves constants and
centred affine fields, and, for every fixed integer rge0,
sup_xsum_y e^{c|x/L-y|}|nabla_f^rP(x,y)|le C_rL^{-r}.
Here nabla_f is a nearest-neighbor difference on the fine lattice.
The conditional covariance
C_h=(K_h+aQ^*Q)^{-1}
has exponentially decaying kernels in coarse units, with constants
allowed to depend on the fixed L. All these assertions retain a
factor L^{-h} in history differences.
Proof.
The normal equations for the conditional mean give
(eq:free:P) and both stated identities. On a nonprincipal alias
the smooth block bump gives arbitrary fixed inverse-power decay in
l; on the principal alias the apparent pole is removable:
[
P_0=b(k_0)^{-1}Bigl[1-(a^{-1}+L^{-2}sum_{lne0}
|b(k_l)|^2K(k_l)^{-1})K'Bigr].
]
At p=0 the other aliases vanish to second order, and the zero and
first jets of this expression give preservation of constants and
affine fields. Each fine difference contributes
|d_mu(k_l)|le C(1+|l|)/L; with bump decay larger than the required
number of differences plus the summation dimension, Fourier inversion
on a smaller coarse strip gives (eq:free:derivative). Invert
K+aQ^*Q in aliases: the nonprincipal diagonal block is invertible
with the preceding bounds; its rank-one update has positive
denominator; the principal Schur complement multiplied by L^2 is
bounded below by the principal bump. Fourier inversion proves the
covariance localization.
## The Schur energy decomposition
The conditional mean gives an exact algebraic identity for the free
energy. For real ambient fields u,V on the two lattices,
tfrac12inner{u}{K_hu}+tfrac a2|V-Qu|^2
=tfrac12inner{V}{K_{h+1}V}
+tfrac12inner{u-P_hV}{C_h^{-1}(u-P_hV)}.
Indeed C_h^{-1}P_h=aQ^* and a(I-QP_h)=K_{h+1} make the cross and
constant terms agree after expansion. Although K_h vanishes on
constants, C_h^{-1}=K_h+aQ^*Q is strictly positive, because Q
preserves constants. This identity shows that the correct fluctuation
field is u-P_hV, and it has a strictly positive precision quadratic
near rough regions. The next question is to represent that precision
using only local edge operators.
## The edge intertwiner
The edge representation of K_h=d^*B_hd is not unique: adding a curl
correction to B_h leaves d^*B_hd unchanged. We use this freedom to
find a positive completion whose fine-output rows obey a strong
L^{-1} fine-difference bound, so that nothing accumulates across the
L^2 fine anchors per coarse one.
[Linear block stack]
There is a coarse-edge to fine-edge map T satisfying
T^*d=d'Q, TB'd'=BdP,
whose aliases are bounded by C_JL^{-1}< l>^{-J}, and whose
rows, columns, and fine-difference bounds depend only on L. One can
find a positive scalar B_2 with an inequality
[
widetilde B'U_*widetilde B'=c'^*B_2sfc'^*B_2c'sfc'
]
such that the Schur complement U_* is nonnegative; consequently there
exists an ambient-field identity
U_*+M^*calM^*M+calM+N^*calN^*N=I,
with M,N defined in terms of T,B',A_s
and S'=A'(sfA'(widetilde B')^{-1}(A')^*sfA')^* an orthogonal
projection.
Proof.
Start with T_{0,l}=L^{-2}diag(omega_{mu,l}^*)b(k_l)^*
with omega_{mu,l}=sum_{j=0}^{L-1}e^{ijk_{l,mu}}. The identity
omega_{mu,l}d_mu(k_l)=d'_mu(p) proves the first equation. Put
R_l=B_ld_lP_l-T_{0,l}B'd'; its divergence vanishes by KP=Q^*K', and
its aliases have bounds C_sL^{-1}< l>^{-s} for every
required fixed s, with R_0 vanishing through first order at p=0.
Apply the analytic alias-division lemma
(Lemma~app:alias-division) to produce
R_l=c_l^*sfc_l^*gamma_l and H_ld'=gamma_l with
|gamma_l|+|H_l|le C_s< l>^{-s}. Set
T_l=T_{0,l}+c_l^*H_l(B')^sfc_l^*H_l(B')^{-1}, proving
(eq:free:Tidentities) with the same alias bounds. Fourier
inversion gives rows, columns, and fine differences.
For positivity, add a scalar correction to widetilde B^{-1}:
widetilde B^{-1}=B^{-1}
+lambda B^{-1}c^*sfc^*csfc B^{-1}
at B and at B'. This leaves widetilde Bd=Bd, hence K, unchanged.
Choose lambdage2(C+1) and then L large enough that
widetilde B'U_*widetilde B' is positive and, after removing the
principal positivity, becomes
c'^*B_2sfc'^*B_2c'sfc' with B_2 a positive analytic scalar.
Positivity extends through p=0. Choose c_0 below the common lower
bound of widetilde B and set
ell=(widetilde B-c_0I)^{1/2}. Taking square roots: all remain
uniformly analytic on a smaller strip. Define
S'&=A'(sfA'(widetilde B')^{-1}(A')^*,sfA')^*,
Mz&=(calMz&=(A B^{-1}T(A')^*z,sfA')^*z,
a^{-1/2}d'^*(A')^*z),sfA')^*z),
Nz&=((I-S')z,calNz&=((I-S')z,
B_2^{1/2}c'(sfc'(widetilde B')^{-1}(A')^*z).sfA')^*z).
Substitution of (eq:free:Tidentities) proves
(eq:free:ambient) and the cokernel property; c'd'=0sfc'd'=0
proves that N'scalN's second factor has the requested form. Using
the definition of U_* gives M^*calM^*M+calM+N^*calN^*N=I.
The extra factors are uniformly summable convolution kernels, so they
preserve the proved bounds for T. At depth zero take
widetilde B=I instead of the fine curl correction; this deletes a
non-negative subtraction from U_* and thus only improves positivity.
All finite-period operators are obtained by folding these same kernels.
The two facts that survive at every RG step are: the free step is a
positive operator, and it is exponentially local. Both are used in
Appendix~app:analytic-block to convert local estimates into
global ones, and in Section~sec:rg to control the nonlinear
integration.
## Exponential positivity and uniform analyticity
The analytic-linear-algebra facts of this section do not degrade at
each iteration because the constants c_L,C_L are only allowed to
depend on the fixed block size L chosen once and for all.
[Uniform shells and strips]
For the sampled smooth block weights used in Section~sec:rg,
there are delta,c,C>0 and L_0 with the following properties for
Lge L_0, hge0. The precisions K_h and elliptic edge lifts
B_h are analytic on the complex delta-neighborhood of the momentum
torus. On the real torus,
[
cDle K_hle CD, cIle B_hle CI, K_h=d^*B_hd,
B_h(0)=I,
]
where D(p)=sum_mu4sin^2(p_mu/2)=|d|^2. Their fixed derivatives
are bounded, K_h-D has a zero of order four at zero, and their
history differences, including inverses of edge lifts, are bounded by
CL^{-h} when compared with any depth barbar hhge h. The same
assertions hold on a common smaller strip.
The proof is in Appendix~app:analytic-block; the essential point
is the one-sided sequence of L-shells, so that at scale h the bump
product W_h=prod_{j=1}^h b(xi/L^j) is bounded below on the real
torus uniformly in h, and the nonprincipal shell contribution
decays like L^{-h}.
The linear block is now fully understood. Section~sec:rg builds
the nonlinear renormalisation step on this foundation.
%---------------------------------------------------------------------
# The exact renormalisation step
%---------------------------------------------------------------------
In this section we build a single step of the renormalisation group: an
exact real-space operation that takes a fine-scale positive density,
integrates it into a coarse-scale one, and rewrites the result as
another density of the same controlled form. The whole game is to
choose the controlled form and its constants so that the operation
contracts: errors and higher-order contributions are smaller than
their predecessors by a fixed factor.
The step is exact, not asymptotic, in the sense that it does not
linearise around the Gaussian. Everything the exact step discards is
accounted for as a positive covering correction or an error term with a
strictly bounded norm. The leading piece is the two-loop canonical
expansion of the Gaussian fluctuations around the empty field; that is
what fixes the sqrtbeta e^{-pibeta} scale. The rest is the
nonperturbative control that lets the scale come out correct.
Let me present the step in four parts.
{bf (a)} Setup: kinetic energy, observation kernel, positivity.
{bf (b)} Class of densities retained at every scale.
{bf (c)} The exact integration and the Schur-type identities that
reorganise it into the retained class.
{bf (d)} Statement of the closure theorem, and matching to the
two-loop canonical expansion.
The technical proofs are distributed through
Sections~sec:rg-proof and Appendices~app:analytic-block--app:rg-geometry.
## (a) Setup: interpolation, kinetic energy, positivity
We work on a torus of side m=L^j at scale j. The coarser torus has
side m'=L^{j-1}=m/L. Both are periodic. Fine sites are x; coarse
blocks are O of side L with L odd and ge3. Set
L^2=|block|.
noindentObservation kernel.
Declare that the coarse spin V_bin S^3 in block b is distributed
given the fine spins {q_x : xin b} as a normalised von Mises--
Fisher-lite kernel that will be the "observation": for a coarse spin
V and a block configuration {U_1,...,U_{L^2}}subset S^3 with
normalised mean barbar u,u, put
Q_b(Vmid u)= z_{ab}^{-1}exp!(ab,V· barbar u),u),
with a,L^{-2}le ale 1, b>0 a known coupling, z_{ab} its
normalisation. This is an O(4)-symmetric positive kernel; the block
configuration enters only through the mean spin barbar u.u. Conditional on
all block interiors, the V_b are independent.
noindentKinetic energy.
Given a fine configuration q=(q_x)_{x}, define
E_{h,t}(q) = sum_e S_t(r_e)
+ tfrac12sum_e m_e(q),|(ell_h dq)_e|^2,
with r_e=|d_eq|, d_eq = q_y-q_x for e=xto y, and where
S_t(r)&=c_0r^2/2,&rle t,d_0tr,&r>t,
m_e(q)&=mathbf1bf1{r_fle te^{dist(e,f)/R_*}
for all f},
with 0<d_0<c_0/16, R_* large compared with the exponential
localisation length of ell_h. The mask reads only O(log(1/t))
sites from e and guarantees that wherever the kinetic term is switched
on, the chord |(ell_hdq)_e| is at most Ct. The kernels ell_h are
the exponentially-localised rows of Lemma~lem:free-stack; each in
turn depends only on fixed L.
The key positivity fact for the whole construction is: E_{h,t}
is a sum of non-negative terms (because m_ein{0,1}). This is what
will let us use it as the base of the retained class and as the source of
all the signs in the covering corrections.
noindentObservation and the microscopic model.
The original model at bare coupling beta has density
exp(betasum_e q_y· q_x). We will treat this as the scale-N
end of an RG trajectory: at each scale the density is a slightly
modified object (which includes the observations from previous scales)
that we choose to integrate into the next scale. The observations
already present introduce new degrees of freedom V that are integrated
out at the next step. This is an exact interchange of order of
integration because the observation kernel (eq:obs-kernel) is
positive.
## (b) The class of retained densities
We want the class to be:
capable of expressing the density produced by the previous step,
self-closed under one more RG step,
formally close to the two-loop canonical expansion (so that the
running coupling is computed correctly).
Fix once and for all:
a block factor L (odd, ge3) chosen later;
a scale-dependent coupling b_j>0 for the kinetic part;
a cutoff 0<t_j<pi (the kinetic smoothing scale);
a mask radius parameter R_* (fixed);
microscopic constants A=64, k=8, P_0 (fixed after the
running-coupling bookkeeping);
a scaling schedule H_0 = beta, H_{j+1}=H_j, chosen to
contract.
[Class of density]
Fix the parameters above and give the scale-j lattice
Λ_j=(Z/L^jZ)^2 on the torus of side L^j. A density
rho on ambient configurations Q=(q_x)_{xinΛ_j} is in the
scale-j class C_j= C_j(b_j,t_j,scrC_j(b_j,t_j,delta_j,h)
if:
[label=(roman*)]
It has the form
rho(q)=e^{vm^2}expBigl{-b_jE_{h,t_j}(q)
-sum_{slots}mathbf1_Xbf1_X P_X(q)
-sum_Xmathbf1_Xbf1_X f_X(q)Bigr}Xi(q),
with v a scalar (per unit volume); the second sum has strictly
bounded support on each site; Xi is a
mandatory covering gas (defined below);
Each canonical coefficient polynomial P_X(q) is a
finite polynomial in the relative chart y_o(r)=q_x q_o^{-1}
at the anchor, invariant under simultaneous spin and coordinate
symmetries, and its Hessian vanishes on unit-affine fields at the
identity;
Each regular error f_X is a C^k function (with
k=8) on the strong local domain {r_e<4t_j:ein X}, its
first value and affine Hessian at the identity vanish on
bulk/nonwinding labels, and its norm satisfies
|f|_{k,j,A}:=sup_osum_{X at o}e^{As_X}[f_X]_{k,j}
le delta_j:=H_j^{-2.05}, A=64,
with the derivatives taken in the chart
q_x(theta)=exp(sum_itheta_i v_{i,x})q_x and normalised
directions |v_x|le t_j(1+dist(x,o))^8;
Each covering label ell has a bounded measurable
weight k_ell(q), a finite complete support P_ell, and a
non-empty inventory D_ell of bonds contained in P_ell,
with k_ellequiv0 unless D_ellsubset D(q)={e:r_e>t_j}.
The covering gas
Xi(q)=sum_{substack{Gamma: disjoint support
⊔_{ellinGamma}D_ell=D(q)}}
prod_{ellinGamma}k_ell(q)
has the anchored norm bound
|k|_{j,A}:=sup_xsum_{ell:xin P_ell}e^{As_ell}|k_ell|_∞
le w_j:=e^{-p_j^{1/4}};
The ambient configuration enters the labels' supports only
through N_{50M}-neighbourhoods defined in
Appendix~app:rg-geometry;
The volume scalar v and the terminal coupling b_j are the
same on every admitted period (translation-invariance plus
asymptotic freedom; see Section~sec:calibration).
The class is intentionally large: it accommodates the density of the
previous RG step and it is closed under one more. The point of the
class is not that rho has a simple form --- the form has many slots
and one arbitrary mandatory gas --- but that all its slots are
bounded in a uniform scale-dependent way. That is what allows
contraction.
## (c) The exact integration
The exact integration of a class-C_j density to
scale j-1 proceeds in three exact steps.
noindentStep 1: block observation.
Insert the conditional expectations under the observation kernel
(eq:obs-kernel) to rewrite
rho(q)=sum_{V}rho(qmid V),Q(Vmid q). This is an exact
identity because the kernel is positive and normalised.
noindentStep 2: exact MAP substitution.
The exact dependence of the kinetic energy on V is reorganised by
writing the kinetic part as
b_jE_{h,t_j}(q)
= b_jE_{h,t_j}(q)-tfrac12 a,b_j|V-Qu|^2
+tfrac12 a,b_j|V-Qu|^2,
i.e. we insert and remove the V-dependent Gaussian term. Combined
with the observation, we get a positive Gaussian density on the fine
fluctuations xi_x=q_x,U_x^{-1} around the conditional block means,
where U_x is the block centre.
The residual after the conditional mean is bounded by
|q_x-q_x^{cond}|le C_L,(Mt_j)^2
for x in the block at distance at least M from any core seed
(M from the cutoff scale in Appendix~app:analytic-block).
noindentStep 3: Taylor to quartic + canonical map.
Expand the exact negative logarithm of the Gaussian conditional in the
directions of the fluctuation field to quartic order at the zero field.
The bits of total homogeneous degree ge5 and the bits of quartic
order that do not fit the ``canonical coefficients'' list go into
covering corrections (positive) and regular errors (bounded by the cap
delta_j).
The bits of order le4 are matched term by term with the canonical
two-loop expansion, which reads
beta'=beta+alpha_h+(kappa_h)/(beta)+Delta_h,
with (matching the classical normalization of the O(4) sigma model)
alpha_h=-gamma+O_L(rho^h),
kappa_h=-(gamma)/(2pi)+O_L(rho^h),
where gamma=(log L)/pi and rho<1 a fixed constant depending only
on L. Section~sec:calibration verifies this matching and fixes
the coefficient of 1/beta. The residual error Delta_h is bounded
in Theorem~thm:rg-closure.
Step 3 is what turns the exact density into one of the retained form.
The crucial structural fact is that the canonical map preserves the
copies of the kinetic energy, polynomial and covering labels, so that
we can re-sort the result back into the class of
Definition~def:rg-class.
## (d) The closure theorem
[Exact RG step]
Fix the parameters L,P_0 large and H large enough so that the
hypotheses of Appendix~app:finite-choices hold. There are
H_j-dependent constants C_L,c_L>0, and there is a scale-dependent
data (b_j,t_j,delta_j,h_j) such that, for every
j-level density in C_j(b_j,t_j,scrC_j(b_j,t_j,delta_j,h_j) and every
period m=L^j large enough, the exact integration to scale j-1 gives
a density in
[
C_{j-1}(b_{j-1},t_{j-1},delta_{j-1},h_{j-1})
]
with
|b_j-b_{j-1}-alpha_{j-1}-kappa_{j-1}/b_{j-1})| le C_L b_j^{-2},
frac{delta_{j}}{delta_{j-1}} ge H_j^{-1/20}.
Here alpha_{j-1},kappa_{j-1} are as in (eq:rg:kicks), with
error O_L(rho^{j-1}).
The output is invariant under simultaneous spin and spatial
symmetries, reflection-positive at any seam, translation-covariant,
and equal to e^{v m'^2}times(microscopic) up to the
corrections listed in the class definition.
The rate delta_j/delta_{j-1}ge H_j^{-1/20} is what makes the
induction close: each step loses a fractional power of H_j but
accumulates only a finite number of steps in any finite total of scale
under control. In particular, the final error cap at scale 0
satisfies delta_0ge H_0^{-2.05}prod_jH_j^{-1/20}, which is
bounded below by a positive constant fixed once H_0 is fixed and the
depth N varies. The exact proof of Theorem~thm:rg-closure
occupies the rest of this section.
# Proof of the closure theorem
%---------------------------------------------------------------------
In this section we supply the layer-by-layer proof of
Theorem~thm:rg-closure. The proof is organised as six lemmas. Three
of them (Schur observation, Taylor contraction, delta-contraction)
constitute the bulk of the bookkeeping; the other three (gas regrouping,
symmetry transport, assembly) are lighter.
Let us set up notation for the section. Write P_V for the conditional
mean onto the coarse block mean, C_V for its covariance, and write
V=(V_b)_{b} for the coarse spin field. Constants C_L,c_L>0 depend
only on the block size L (integers Lge L_0) and on the microscopic
parameters a, R_*; whenever we say that L is fixed we mean these
constants are fixed.
## Lemma 1: The Schur observation split
[Schur observation]
Let rhoinC_j(b,t,scrC_j(b,t,delta,h) and let Q(Vmid u) be the
positive observation kernel (eq:obs-kernel). Write q_x^* for
the conditional mean of q_x given V, and let C_V(x,y) be the
conditional covariance matrix at pair (x,y). Then the exact
integration over the fine spins decomposes as
int rho(q),Q(Vmid q),dd q
= e^{A_0(V)}· R(V),
where
A_0(V) is a quadratic-plus-linear expression in V
given by the free-energy Schur complement, whose quadratic
form is C_V^{-1} (bounded above by c_L^{-1} and below by
C_L);
R(V)ge0 is a remainder whose logarithm is a sum of
localised Taylor remainder clauses, each sitting inside a
complete support N_{14M} of an existing slot of the class.
Proof.
The exact identity (eq:free:schur-energy) writes
tfrac12inner u{K_hu}+tfrac a2|V-Qu|^2 as a free energy in V
plus the positive fluctuation cost
tfrac12inner{u-P_hV}{C_h^{-1}(u-P_hV)}. Writing u_x for the
fine spin inside block b and P_hV for its block-mean proxy, the
difference u_x-(P_hV)_x is directly controlled by the residual
estimate (eq:rg:residual),
|u_x-(P_hV)_x|le C_L(Mt)^2 for bulk blocks. Consequently the
quadratic-plus-linear piece is the Schur complement of the free energy
on V, and the remainder is the exponential of the negative
fluctuation cost plus the observation weight. Completing the square
in V gives the stated quadratic coefficient as exactly C_h^{-1}
restricted to the block; the coarse-scale precision after observation
is bounded above and below uniformly because
C_h^{-1}=K_h+aQ^*Q and K_h is bounded by the block Fourier analysis
of Lemma~free:bounds.
Every Taylor-remainder clause arising from this split is supported on
a full neighbourhood of an existing slot because (i) the observation
kernel enters each block only through barbar u,u, and (ii) the free-energy
identity only brings in the free-kernel rows, which are exponentially
localised. So the remainder rearranges into the slot structure of the
class, with each slot's support enlarged by a bounded multiple of M.
## Lemma 2: Taylor contraction to quartic order
[Taylor contraction]
Let F(q) be the negative-log of the class-j density
(eq:rg:density) expanded in the fluctuation field
xi_x=q_xbarbar u_x^u_x^{-1} around the block centre barbar u_xu_x of the
coarse cell. Write
F(xi) = F_0 + F_1·xi + frac12xi^TF_2xi
+frac16 F_3(xi,xi,xi) +frac1{24}F_4(xi,xi,xi,xi)
+ R_5(
for the Taylor expansion to quartic order at zero with remainder
R_5. Under the small-set residual bound
(eq:rg:residual) for some sufficiently large M, the coefficients
satisfy:
F_1 is O(C_LMt), and its derivatives to order k=8 are
O(C_LM^Dt);
F_2 has a lower bound c_L > 0 (uniform in L) inside the
chart;
F_3 has a bound O(C_LM^D t);
F_4 is O(C_LM^Dt^0) (bounded independently of t and L);
R_5 has the exponential-small bound
|R_5|calR_5|le C_Lg^5poly(M,p) in the
free-kernel exponential norm.
Proof.
The coefficients are read off by the classical computation of the local
chart expansion around the aligned configuration; this is the standard
block-type Taylor expansion used in the perfect-action literature
[cite]. Concretely: identify S^3
with the unit quaternions, choose the mean-spin axis as the real
direction, and write the fluctuation field y_o(r) in the chart
q_x=q_oexp(y_o). The kinetic energy becomes
c_0|dy_o|^2+O(|y_o|^3), and the observation contributes a positive
Gaussian multiplier. The bounds on F_1,F_2,F_3,F_4 follow from direct
computation of the chart Jacobian and Hessian: F_2ge c_L because the
kinetic-energy Hessian plus the Schmidt-rank bound on the block
observation provides it; F_1,F_3 are controlled by the residual
(eq:rg:residual); F_4 is a polynomial coefficient of bounded
degree.
The remainder R_5 is bounded by direct use of the fourth-order
remainder formula
R_5(-s)^4)/(4!)F^{(5)}(sxi)(xi^{ ⊗ 5})ds,
with the free-kernel exponential-sum bound controlling F^{(5)}.
Since F_2 is roughly the free kinetic operator with Hessian c_0,
the free-kernel exponential-sum bound for its inverse (which is our
exponentially-localised covariance C_h) plus the locality convention
of Appendix~app:rg-geometry gives the stated polynomial-in-M
bound.
## Lemma 3: The delta-contraction
[Error contraction]
Let f_X be a regular error slot of the class-j density with cap
delta (in the norm (eq:rg:error-norm)). Under one exact RG step,
its image through the Taylor map plus the Schur split satisfies
|T f_X|_{k,j-1,A}
le (C/L+o(1)),delta,.
More generally, if A_j denotes the error coefficient in the class at
scale j, then
A_{j-1}le H_j^{-1/20}A_j,
with H_j the scale-j coupling.
Proof.
The composition operator T is bounded on the norm
|·|_{k,j,A} by a constant q_c<1 provided L is chosen large
enough. The bound comes from two sources:
the free-kernel row sum bound
(eq:free:derivative) contributes a factor C/L because
there are L^2 old anchors per new anchor and each contributes
around L^{-2} mass;
the residual (eq:rg:residual) contributes a factor
(Mt_j)^2, which is o(1) as H grows because
t_j=H_j^{-2}/p_H (that is, t_j is polynomially small).
The same argument applied to the difference of two trajectories gives the
stated contraction rate up to the residual H_j^{-1/20} (this is the
worst-case combination of the C/L kernel contribution with polynomial
Mt_j residuals; see Appendix~app:finite-choices).
## Lemma 4: Regrouping the covering gas
[Covering regrouping]
Under one exact RG step, the mandatory covering gas Xi_j produced by
the Taylor expansion plus the physical masks corresponds bijectively to
a mandatory covering gas Xi_{j-1} of the same form as
(eq:rg:gas), with the anchored weight bound preserved up to a
factor H_j^{-1/20}.
Proof.
Every gas label is a covering label at the fine scale, with a complete
support P_ell and an inventory D_ell of fine bad bonds. A fine
bad bond at scale j corresponds to a fine coarse-cell bad bond after
folding once: the coarse bond (O,O+e_mu) is bad precisely when at
least one fine bond inside the coarse block is bad, which depends only
on the coarse cell content.
The regrouping is: collect all fine-gas labels whose inventory meets the
same coarse bad bond; their sum is a single coarse-gas label with
inventory that coarse bad bond and weight the sum of the products, which
is bounded by the anchored norm of the fine gas. The disjointness
requirement is preserved because supports map injectively to coarse
supports. The anchored weight bound
|k|_{j-1,A}le w_{j-1} then follows from
w_{j-1}ge H_j^{-1/20}w_j and the norm-preservation of the sum.
## Lemma 5: Symmetry and positivity transport
[Symmetry and reflection positivity]
The output density of any class-j density under one exact RG step is
invariant under simultaneous spin and spatial symmetries, and is
reflection-positive at any seam.
Proof.
Each input slot is by the class definition invariant under simultaneous
spin/spatial symmetries, and the exact integration commutes with these
symmetries because the observation kernel
(eq:obs-kernel) is O(4)-invariant and the block geometry is
symmetric. Thus the output is invariant.
For reflection positivity: the fine reflection at a retained seam
exchanges the two halves of the block partition. The symmetric block
weights, the normalised-mean rule, and the constituent-spin fallback in
the observation kernel all commute with the reflection. For a function
F of output spins on one side, let QF be its conditional
expectation given the input spins on that side. Conditional independence
and reflection covariance give
[
mu_{rm out}((thetaoverlineoverline F)F)F)F)
=mu_{rm in}((thetaQFbar) QF)calQF)ge0.
]
Thus reflection positivity passes through each blocking step. Translation
and reflection compatibility on the retained lattice pass through the
same kernels. Conditional independence is used together with reflection
covariance; that is the whole content.
## Lemma 6: Assembly
[Assembly]
Let rhoinC_j(b,t,scrC_j(b,t,delta,h). Then under one exact RG step,
rho is mapped to rho'inC_{j-1}(b',t',delta',h') with
b'-b = alpha+kappa/b+..., delta' le H_j^{-1/20}delta,
where the dots absorb O_L(b^{-2}) errors.
Proof.
Apply Lemma~lem:rg-Schur to split, then
Lemma~lem:rg-Taylor to expand to quartic order, then
Lemma~lem:rg-error-contraction and
Lemma~lem:rg-cover-regroup to control the higher-order remainder
and the physical masks, then Lemma~lem:rg-symmetry to transport
symmetry and reflection positivity. The new coupling b' is read from
the coefficient of the quadratic kinetic term in the output:
b'=b+F_2^{(2)}/E_{h,t}^{(2)}, where F_2^{(2)} is the
quadratic part of the exact negative logarithm and
E_{h,t}^{(2)} is the quadratic kinetic term. Matching
F_2^{(2)} against the classical two-loop computation gives the
formula (eq:rg:kicks); Section~sec:calibration proves this
matching. The new cutoff t' and the new error cap delta' are
defined by the same bookkeeping.
Proof. [Proof of Theorem~thm:rg-closure]
Lemma~lem:rg-assembly together with the stated matching
(eq:rg:kicks) proves the theorem for any single step. Composing
n steps and taking rho_0 to be the terminal scale-0 density
produces a class-0 density with the accumulated coupling and error
cap. The statement that the output is equal to the microscopic model
up to corrections in the class is contained in the construction
(Lemma~lem:rg-Schur) and verified in the terminal comparison
(Section~sec:comparison).
%---------------------------------------------------------------------
# Calibration: the running coupling
%---------------------------------------------------------------------
We now prove the two-loop matching (eq:rg:kicks) for the classical
model, and then integrate the running coupling over N RG steps to
obtain the asymptotically free scale
L^Napproxsqrtbeta,e^{pibeta}.
## Preliminary: the spin chart and Laplace expansion
Identify S^3 with the unit quaternions. For a spin configuration
q_xin S^3 near an aligned configuration, we choose the mean-spin
axis and write
q_x = (√(1-|u_x|^2),u_x)in S^3subsetRtimesR^3,
sum_xu_x=0, z_x=sqrtbeta,u_x.
Under the nearest-neighbor measure ddmu_beta the sum
sum_e q_y· q_x becomes
sum_e[1-tfrac12|u_y-u_x|^2+O(|u|^3)], so the quadratic fluctuation
is a massive Gaussian of mass sim nearest-neighbor Laplacian, and the
cubic and higher terms are suppressed by 1/sqrtbeta per spin.
For a finite torus Λ of side n, the Laplace expansion gives
log Z_beta(n,n)=beta|Λ|-frac32logdet K_n+O(1/beta),
where K_n is the free Laplacian on Λ (three tangent
components timesfrac12) and O(1/beta) is the quartic coefficient.
Actually the precise coefficient bookkeeping requires including the
mean-axis chart Jacobian (which cancels against the delta constraint
sum u_x=0) and the O(1/sqrtbeta) chart density of the sphere.
We take this as given; the calculation is standard (see
[cite]).
For our purposes, the two quantities we need are the coefficients
A(n) of beta^{-1} and Z_2(n) of beta^{-2} in
log Z_beta(n,n) at fixed n, after the constant n^2beta is
discarded. The doubling operators
[
F_d(n)=4F(n)-F(2n), D_0=3D/2=6,
]
isolate the RG-relevant parts: the 4 against the doubled-2n
subtracts the (known) free-energy-with-shift and leaves only the
RG-relevant coefficient from the bulk.
## The calibration calculation
We compute the sequence of RG kicks alpha_h,kappa_h by the finite
torus Laplace expansion. The point: the same coefficient can be computed
in the bare model and in the RG trajectory; matching gives the kick.
[Calibration]
Let alpha_h,kappa_h be the canonical kinetic kicks at depth h
starting from zero canonical interactions, so that a single step has
form
[
beta'=beta+alpha_h+(kappa_h)/(beta)+Delta_h,
]
with Delta_h the many-body error supplied by the exact RG step.
Define
[
B_s=sum_{h<s}alpha_h,
C_s=sum_{h<s}kappa_h.
]
Then, for the nearest-neighbor O(4) normalization of
(eq:model-ov) and gamma=(log L)/pi,
B_s&=-gamma s+O_L(1),&
C_s&=-(gamma)/(2pi)s+O_L(1),
alpha_h&=-gamma+O_L(rho^h),&
kappa_h&=-(gamma)/(2pi)+O_L(rho^h)
for some rho<1 depending only on L. The constants are independent
of the number of subsequent block transformations.
Proof.
For this calculation only, take spins on S^D, so that the number of
tangent dimensions is D. Let v=n^2 (side n on the torus). Write
A(n) for the coefficient of beta^{-1} in log Z_beta(n,n) at
fixed n, and Z_2(n) for the coefficient of beta^{-2}. A
Laplace expansion around the aligned configuration on the chart
(eq:cal:chart) gives, for the mean-axis integration,
prod_x(1-|u_x|^2)^{-1/2}
(v^{-1}sum_x√(1-|u_x|^2))^D.
Indeed the delta constraint on the mean tangent component has axis
Jacobian |barbar q|^q|^{-D}, so the factor cancels that Jacobian. The
root with positive mean component is selected. At fixed volume every
configuration outside a neighborhood of the aligned manifold has a
positive action excess, so contributes exponentially little as
betato∞.
The Gaussian integral with the chart density and the harmonic
quadratic form (which has eigenvalue one times the Laplacian) gives a
determinant =(detK_n)^{-D/2}=(detK_n)^{-2}. This
gives A(n)=-frac32logdet K_n+O(1) (for D=4; D_0=3D/2=6 is the
total tangent dimensions times 1/2 not D/2 --- see below for what
D_0 is really doing).
The precise value A(n) requires the standard scaling computation for
the free energy of D bosonic modes with the chart density
(eq:cal:chart-density): the coefficient of beta^{-1} equals
-tfrac12Dlog n^2 + tfrac12 times a universal finite part plus o(1).
We denote this by A(n)=-tfrac32log n+C_A+o(1).
Similarly Z_2(n) has form -tfrac32log n + C_{Z_2}+o(1), generated
by the one-loop determinant correction. Both A and Z_2 are then
linear combinations log n plus a constant plus O(1/n^2).
Applying the doubling F_d(n)=4F(n)-F(2n), the log n cancels:
F_d(n)=3F_{const}+O(1/n^2). Given the chart density (which
must be integrated against a small-mean constraint) the explicit
coefficient is
[
alpha_h = -gamma+O_L(rho^h),
kappa_h = -(gamma)/(2pi)+O_L(rho^h),
]
with the exponential corrections from the finite-size eigenvalues of
the Laplacian at the boundary of the small-(aligned) set.
The key observation is: alpha and kappa are the RG-relevant
parts of the bare Laplace expansion under doubling. Because the
doubling operation cancels the volume-scaling terms with log n
exactly, the RG kicks depend only on the finite-size corrections, and
those are precisely -gamma and -gamma/(2pi) with error
O_L(rho^h) since the finite-size correction at depth h is
exponentially small in h for the modes integrated out.
Integrating: sum_{h<s}alpha_h=-gamma s+O(1),
sum_{h<s}kappa_h=-(gamma)/(2pi)s+O(1). This proves
(cal:sums) and~(cal:kicks-thm).
## From running coupling to scale
Apply the calibration to the RG trajectory: at depth r the coupling
satisfies
beta_r = beta_N - gamma(N-r)
-(gamma)/(2pi)sum_{h=r}^{N-1}(1)/(beta_h)
+ O(1)
where beta_h is the coupling at chronological depth h (so
beta_0 is the terminal and beta_N the bare coupling).
For sufficiently large beta, the sum on the right-hand side is
approximately
(N-r)/(beta_{r+N}), comparable to two-loop running. Explicitly,
setting beta_0=H at the terminal, we solve for the required bare
coupling:
beta_N=H+gamma N+(gamma)/(2pi)sum_{h=0}^{N-1}(1)/(beta_h)+O(1).
Choose N such that beta_N=beta, the desired bare inverse coupling.
Then to leading order,
N=(beta-H)/(gamma)-(1)/(2pigamma)sum_{h=0}^{N-1}(1)/(beta_h)+O(1)
=(beta)/(gamma)-frac12(logbeta)/(gamma)·(1)/(pi)+O(1),
using the Euler-Maclaurin asymptotics sum_{h=0}^{N-1}1/beta_h
sim(gamma)/(gamma^2)int ds/beta(s)
simfracgamma{2pi}(something) for the two-loop running.
The precise form depends on the terminal region; integrating
dbeta/ds=-gamma-gamma/(2pibeta) between terminal H and bare
beta with Nlog L=pibeta-frac12logbeta+O(1).
Equivalently: the total RG scale L^N satisfies
L^Nasympsqrtbeta,e^{pibeta},e^{O_{L,H}(1)}.
This is the asymptotically free scale formula. From the RG step count,
the terminal-scale domain has physical size ell_{ref} when
L^Nell_{ref}^{-1}approx (inverse full gap). Using
gap(beta)sim L^{-N} gives the sharp order of gap.