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Symmetric Volume Descent from U4 and a Four-Dimensional Lower Bound

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Abstract

We explain a symmetric deformation that decreases the volume of the four-dimensional constant-width body U4U_4. The emphasis is on why the deformation works, rather than the size of the decrease. Oddness preserves width; convexity requires control of the curvature radii. A positive cap on one support branch is coupled to a negative correction on the adjacent branch. Their first-order volume contributions have different orders in the localization parameter, so the favorable contribution dominates. A small motion towards the ball makes the direction feasible for positive time. In a separate part we give a spectral lower bound for all four-dimensional bodies of constant width one, including an explicit positive refinement. A short projection argument using a three-dimensional theorem of Jiang gives the stronger lower bound 0.178722030.17872203. A substantial gap between the lower and upper bounds remains.

The result and the geometric idea

The body U4U_4 has the symmetries of a regular four-simplex [1]; write U4(1)U_4^{(1)} for its width-one normalization. The companion preprint [5], Theorem 1.1 establishes that it has smaller volume than the other members of the finite collection studied there. Here we show that it can be deformed, while retaining those symmetries and constant width, to have smaller volume.

Theorem 1.1 (Symmetric local descent). There exist S5S_5-invariant bodies KtK_t of constant width one, converging to U4(1)U_4^{(1)} as t↓0t \downarrow0, such that

Vol⁡4(Kt)<Vol⁡4(U4(1))(t>0 sufficiently small).\operatorname{Vol}_4(K_t) < \operatorname{Vol}_4(U_4^{(1)}) \qquad(t > 0\ \text{sufficiently small}).

Width is a linear constraint. The support function h(u)h(u) gives the signed distance from the origin to the supporting hyperplane with outward unit normal uu. Width one means h(u)+h(−u)=1h(u) + h(-u) = 1. Thus moving one supporting plane by φ(u)\varphi(u) and its opposite by −φ(u)-\varphi(u) preserves width exactly. In support-function language, the perturbation must be odd.

Research development and supervision. The initial idea of a volume-decreasing deformation of U4U_4 was developed by the author and communicated to Professor Andriy Prymak on August 7, 2026. Professor Prymak subsequently examined the proposed approach and contributed further mathematical details and expanded, AI-assisted expositions of the argument. The present manuscript was developed through this exchange and the author’s subsequent investigations and verification.

Affiliations. China University of Geosciences (Wuhan), China; University of Manitoba, Canada (Mitacs Globalink Research Intern, 2026).

Acknowledgements. Most of this work was completed during the author’s 2026 Mitacs Globalink Research Internship at the University of Manitoba. The author gratefully acknowledges Mitacs for its support and thanks Professor Andriy Prymak for his supervision, mathematical contributions, and generous guidance in developing more effective research and learning methods.

AI assistance and manuscript preparation. The manuscript combines human-written material with AI-assisted drafting, organization, revision, and editorial refinement. OpenAI’s GPT-5.6 Sol, GPT-5.6 Sol, and Astra assisted with selected proof steps, auxiliary checks, code development, and manuscript preparation. Astra was used through Codex; Claude provided limited editorial assistance with the \LaTeX{} manuscript. The author takes responsibility for the mathematical content and conclusions.

Verification: all parts checked and understood. The author has checked and understood all parts of this manuscript, including the mathematical arguments and supporting calculations. This statement describes the author’s own review and does not assert formal verification or independent peer review.

Convexity is the constraint that matters. An odd function need not describe a convex body. The matrix Ah=∇2h+hIA_h=\nabla^2h+hI describes its curvature radii and must satisfy 0⪯Ah⪯I0\preceq A_h\preceq I. Here the spectral endpoints are the eigenvalues 00 and 11. At U4U_4 some radii are already at an endpoint. The perturbation must move these radii in the permissible direction. This is why an arbitrary asymmetric bump, or a bump on just one branch, does not settle the problem.

Why two coupled pieces succeed. We place a favorable cap on a region with two positive and three negative coordinates. Matching the opposite support branch forces a compensating piece on the region with three positive and two negative coordinates. There is more room for the favorable piece. For localization parameter δ\delta, its contribution has size at least cδ9/2c\delta^{9/2}, whereas the loss is at most Cδ13/2C\delta^{13/2}. The loss-to-gain ratio is therefore O(δ2)O(\delta^2) and tends to zero. The proof therefore needs no optimized numerical choice of parameters.

From a direction to a body. We finally add a motion of order δ5\delta^5 towards the ball. It supplies strict curvature margins while costing less than the favorable δ9/2\delta^{9/2} term. A compactness lemma then produces an actual support function for small positive time. This step certifies global convexity, not just the constant-width identity or convexity at sampled directions.

The lower-bound part is independent. § 5 starts again with an arbitrary width-one body, not a perturbation of U4U_4. It gives

Vol⁡4(K)≥11π2224(1−25),\operatorname{Vol}_4(K)\geq\frac{11\pi^2}{224}\left(1-\sqrt{\frac{2}{5}}\right),

and an independent spectral refinement above 0.17818404. Corollary 5.4 then applies Jiang’s three-dimensional bound [6] to all hyperplane projections and yields

Vol⁡4(K)≥4953π32000(1−25)>0.17872203.\operatorname{Vol}_4(K)\geq\frac{4953\pi}{32000}\left(1-\sqrt{\frac{2}{5}}\right)>0.17872203.

The latter improvement uses an external theorem; the four-dimensional spectral proof is independent of it. Neither argument identifies a minimizer. Detailed optimization of tiny volume reductions is omitted.

Support functions and convexity

Support functions, constant width, and curvature radii

A convex body is a compact convex subset of Rn\mathbb{R}^n with nonempty interior. Its support function is

hK(u)=max⁡x∈K⟨x,u⟩,u∈Sn−1,h_K(u)=\max_{x\in K}\langle x,u\rangle,\qquad u\in S^{n-1},

and its positively one-homogeneous extension is

HK(x)=max⁡y∈K⟨y,x⟩,HK(ru)=rhK(u)(r≥0).H_K(x)=\max_{y\in K}\langle y,x\rangle,\qquad H_K(ru)=rh_K(u)\quad(r\geq0).

The body can be recovered from its support function through

K=⋂u∈Sn−1{x∈Rn:⟨x,u⟩≤hK(u)}.(1)K=\bigcap_{u\in S^{n-1}}\{x\in\mathbb{R}^n:\langle x,u\rangle\leq h_K(u)\}. \tag*{(1)}

If a∈Rna\in\mathbb{R}^n, then hK+a(u)=hK(u)+⟨a,u⟩h_{K+a}(u)=h_K(u)+\langle a,u\rangle; thus first spherical harmonics represent translations. The width of KK in direction uu is

wK(u)=hK(u)+hK(−u).w_K(u)=h_K(u)+h_K(-u).

Accordingly, KK has constant width d>0d>0 if and only if

hK(u)+hK(−u)=d(u∈Sn−1),(2)h_K(u)+h_K(-u)=d\qquad(u\in S^{n-1}), \tag*{(2)}

or, equivalently,

HK(x)+HK(−x)=d∥x∥(x∈Rn).(3)H_K(x)+H_K(-x)=d\lVert x\rVert\qquad(x\in\mathbb{R}^n). \tag*{(3)}

The antipodal identity is the basic constraint used throughout the paper. It gives both the regularity of constant-width support functions and the relation between their curvature-radius operators at antipodal points.

Lemma 2.1 (Regularity of constant-width support functions). Let K⊂RnK \subset\mathbb{R}^n be a convex body of constant width dd, and write h=hKh=h_K. Then hK∈C1,1(Sn−1)h_K \in C^{1,1}(S^{n-1}). At almost every u∈Sn−1u \in S^{n-1} the operator

Ah(u):=∇Sn−12h(u)+h(u)ITuSn−1(4)A_h(u) := \nabla^2_{S^{n-1}}h(u) + h(u)I_{T_uS^{n-1}} \tag*{(4)}

is defined and satisfies

0⪯Ah(u)⪯dI,Ah(−u)=dI−Ah(u),(5)0 \preceq A_h(u) \preceq dI,\qquad A_h(-u)=dI-A_h(u), \tag*{(5)}

after identifying TuSn−1=T−uSn−1=u⊥T_uS^{n-1}=T_{-u}S^{n-1}=u^\perp.

Proof. The homogeneous support function H=HKH=H_K is convex. By (3), H(−x)=d∥x∥−H(x)H(-x)=d\lVert x\rVert-H(x), and H(−⋅)H(-\cdot) is also convex. Hence, in the sense of distributions,

0⪯D2H⪯dD2∥x∥.0 \preceq D^2H \preceq dD^2\lVert x\rVert.

On an annulus a≤∥x∥≤ba\leq\lVert x\rVert\leq b with a>0a>0,

D2∥x∥=1∥x∥(I−x⊗x∥x∥2)⪯1aI,D^2\lVert x\rVert=\frac{1}{\lVert x\rVert}\left(I-\frac{x\otimes x}{\lVert x\rVert^2}\right)\preceq\frac{1}{a}I,

so

0⪯D2H⪯daI.0\preceq D^2H\preceq\frac{d}{a}I.

Thus HH is locally semiconvex and semiconcave on Rn∖{0}\mathbb{R}^n\setminus\{0\}, whence H∈Cloc1,1H\in C^{1,1}_{\mathrm{loc}} there. Restricting to Sn−1S^{n-1} gives h∈C1,1(Sn−1)h\in C^{1,1}(S^{n-1}).

At a point of twice differentiability, the standard identity for a one-homogeneous extension gives

D2H(u)∣u⊥=∇Sn−12h(u)+h(u)I=Ah(u).D^2H(u)|_{u^\perp}=\nabla^2_{S^{n-1}}h(u)+h(u)I=A_h(u).

Restricting the distributional Hessian inequalities to u⊥u^\perp yields 0⪯Ah(u)⪯dI0\preceq A_h(u)\preceq dI. Differentiating (3) twice at uu and −u-u gives Ah(−u)=dI−Ah(u)A_h(-u)=dI-A_h(u) almost everywhere. □

For a smooth strictly convex body, the eigenvalues of AhA_h are the principal radii of curvature. Lemma 2.1 shows that the same terminology is meaningful almost everywhere for every body of constant width: the principal radii lie in [0,d][0,d], and antipodal radii add to dd.

We also need the support-function volume formula in precisely the nonsmooth regularity class that occurs for U4U_4. Let Sn−1(K,⋅)S_{n-1}(K,\cdot) denote the surface-area measure of KK on Sn−1S^{n-1}, and let σ\sigma denote ordinary, unnormalized spherical surface measure. The Minkowski integral formula [2 Section 5.1] is

Vol⁡n(K)=1n∫Sn−1hK(u) dSn−1(K,u).(6)\operatorname{Vol}_n(K)=\frac{1}{n}\int_{S^{n-1}}h_K(u)\,dS_{n-1}(K,u). \tag*{(6)}

For C1,1C^{1,1} support functions the measure has an almost-everywhere density.

Proposition 2.2 (C1,1C^{1,1} surface-area density). If hK∈C1,1(Sn−1)h_K\in C^{1,1}(S^{n-1}), then

dSn−1(K,u)=det⁡AhK(u) dσ(u),(7)dS_{n-1}(K,u)=\det A_{h_K}(u)\,d\sigma(u), \tag*{(7)}

where the Hessian is understood almost everywhere. Consequently,

Vol⁡n(K)=1n∫Sn−1hK(u)det⁡AhK(u) dσ(u).(8)\operatorname{Vol}_n(K)=\frac{1}{n}\int_{S^{n-1}}h_K(u)\det A_{h_K}(u)\,d\sigma(u). \tag*{(8)}

Proof. Because h=hKh=h_K is C1,1C^{1,1}, the reverse Gauss parametrization

Xh(u)=h(u)u+∇Sn−1h(u)(9)X_h(u)=h(u)u+\nabla_{S^{n-1}}h(u) \tag*{(9)}

is Lipschitz. Rademacher’s theorem gives differentiability almost everywhere, and Aleksandrov’s theorem gives twice differentiability of hh almost everywhere. If v∈TuSn−1v\in T_uS^{n-1} is a tangent vector, differentiation of (9), followed by cancellation of the normal terms, gives

DXh(u)v=(∇2h(u)+h(u)I)v=Ah(u)v.DX_h(u)v=\left(\nabla^2h(u)+h(u)I\right)v=A_h(u)v.

Since Ah(u)⪰0A_h(u) \succeq0 almost everywhere, the tangential Jacobian is

Jn−1Xh(u)=det⁡Ah(u).J_{n-1}X_h(u)=\det A_h(u).

Almost every boundary point of a convex body has a unique outer normal. Since differentiability of hh makes each support face a singleton, XhX_h has multiplicity one at these regular boundary points. The exceptional boundary set has zero (n−1)(n-1)-dimensional measure. The area formula [3] therefore accounts for collapsed normal regions as zero Jacobian and gives, for every Borel set ω⊂Sn−1\omega\subset S^{n-1},

Sn−1(K,ω)=∫ωdet⁡Ah(u) dσ(u).S_{n-1}(K,\omega)=\int_{\omega}\det A_h(u)\,d\sigma(u).

Substitution into (6) yields (8). This argument is the C1,1C^{1,1} realization of Schneider’s general measure-valued formula and does not require a globally C2C^2 boundary.

The support geometry of U4U_4

We recall the support formula and curvature spectrum from [5 Section 3 and Proposition 3.1], where the latter is proved. Only the notation and statements needed for the descent argument are retained here.

The support function on sign cells

3.1. The support function on sign cells. Identify H4=15⊥⊂R5H_4=1_5^{\perp}\subset\mathbb{R}^5 with R4\mathbb{R}^4 and let S(H4)≅S3S(H_4)\cong S^3. For a nonempty proper subset PP of {1,…,5}\{1,\ldots,5\}, the corresponding open sign cell is

CP={u∈S(H4):ui>0 (i∈P), uj<0 (j∉P)}.C_P=\{u\in S(H_4):u_i>0\ (i\in P),\ u_j<0\ (j\notin P)\}.

For u∈S(H4)u\in S(H_4) put

P(u)={i:ui>0},k(u)=∣P(u)∣,P(u)=\{i:u_i>0\},\qquad k(u)=|P(u)|,
r(u)2=∑i∈P(u)ui2,s(u)2=1−r(u)2,μ(u)=∑i∈P(u)ui.r(u)^2=\sum_{i\in P(u)}u_i^2,\qquad s(u)^2=1-r(u)^2,\qquad\mu(u)=\sum_{i\in P(u)}u_i.

The projection construction of Arman–Bondarenko–Prymak–Radchenko [1] gives the following width-two support function:

H(u)={2r(u),r(u)≥s(u),2−2s(u),r(u)≤s(u).(10)H(u)= \begin{cases} \sqrt{2}r(u), & r(u)\ge s(u),\\ 2-\sqrt{2}s(u), & r(u)\le s(u). \end{cases} \tag*{(10)}

Write

D={u∈S(H4):r(u)≥s(u)}.\mathcal{D}=\{u\in S(H_4):r(u)\ge s(u)\}.

The branch-switch set r=sr=s and the coordinate hyperplanes have spherical measure zero.

Proposition 3.1 (Curvature-radius spectrum, [5 Proposition 3.1]). On a sign cell in D\mathcal{D} with k=∣P∣≥2k=|P|\ge2, let

QH:=∇S32(2r)+2rI.Q_H:=\nabla^2_{S^3}(\sqrt{2}r)+\sqrt{2}rI.

Its eigenvalues on TuS(H4)T_uS(H_4) are

α,…,α⏟k−2,βk,0,…,0⏟4−k,\underbrace{\alpha,\ldots,\alpha}_{k-2},\quad\beta_k,\quad\underbrace{0,\ldots,0}_{4-k},

where

α=2r,βk=2((5−k)r2+μ2)5r3.(11)\alpha=\frac{\sqrt{2}}{r},\qquad\beta_k=\frac{\sqrt{2}\bigl((5-k)r^2+\mu^2\bigr)}{5r^3}. \tag*{(11)}

For k=1k=1, QH=0Q_H=0.

If u∈Du\in\mathcal{D} had four positive coordinates, the unique negative coordinate would have absolute value μ\mu, hence s=μ>rs=\mu>r in the interior of the cell. Therefore

k(u)∈{1,2,3}for almost every u∈D,(12)k(u)\in\{1,2,3\}\quad\text{for almost every }u\in\mathcal{D}, \tag*{(12)}

and consequently det⁡QH=0\det Q_H=0 almost everywhere on D\mathcal{D}.

For the rest of the descent argument we use width one, so h=H/2h=H/2 and Ah=QH/2A_h=Q_H/2 on the first branch. In particular det⁡Ah=0\det A_h=0 there. The zero eigenvalues describe the directions along which the initial body has no curvature margin; the construction below is adapted to these directions.

A volume-decreasing deformation of U4U_4

The initial idea of a volume-decreasing deformation of U4U_4 was proposed by the author and communicated to Prymak on August 7, 2026. The expanded exposition here draws on the subsequent research notes supplied by Prymak [4], specifically the coupled cap formulas and branch matching, the endpoint curvature checks, the comparison of the positive and negative first-variation contributions, and strictification towards the ball. The expanded notes also prove a dimension-independent endpoint tangent-cone criterion and an explicit symmetric descent theorem for all n≥4n \ge4; their Theorem 18 includes the four-dimensional nonminimality conclusion. Here we give a detailed four-dimensional exposition of the construction and feasibility proof, without invoking the higher-dimensional theorem as a black box.

This section proves Theorem 1.1. We first derive the endpoint curvature constraints and pair antipodal points in the volume variation. We then construct the two matching pieces, check their curvature signs, and compare their contributions. The last step adds a smaller motion towards the ball and applies compactness to obtain a globally feasible path. The geometric reasons for these steps were described in § 1.

Local minimizers, admissible paths, and endpoint constraints

Let W4,1\mathcal{W}_{4,1} be the class of four-dimensional convex bodies of constant width one. Since translations preserve width and volume, we work modulo translations.

Definition 4.1 (Local volume minimizer). A body K∈W4,1K \in\mathcal{W}_{4,1} is a local volume minimizer modulo translations if there exists ε>0\varepsilon> 0 such that

Vol⁡4(K)≤Vol⁡4(L)\operatorname{Vol}_4(K) \le\operatorname{Vol}_4(L)

whenever L∈W4,1L \in\mathcal{W}_{4,1} and

inf⁡a∈R4dH(K,L+a)<ε.\inf_{a \in\mathbb{R}^4} d_H(K,L+a) < \varepsilon.

Hausdorff convergence of convex bodies is equivalent to uniform convergence of their support functions. Let hh be the width-one support function of U4U_4. For the affine paths used here, a candidate support function has the form

ht=h+tφ(t↓0)(13)h_t=h+t\varphi\qquad(t \downarrow0) \tag*{(13)}

with h,φ∈C1,1h,\varphi\in C^{1,1} and continuous second derivatives on each closed smooth piece. The width condition forces φ\varphi to be odd.

Write

Ah=∇2h+hI,Bφ=∇2φ+φI.A_h=\nabla^2h+hI, \qquad B_\varphi=\nabla^2\varphi+\varphi I.

Here BφB_\varphi is the linearized curvature-radius operator: Aht=Ah+tBφA_{h_t}=A_h+tB_\varphi. If (4.1) is a path of width-one support functions, then 0⪯Aht⪯I0 \preceq A_{h_t} \preceq I. Let P0P_0 and P1P_1 be the orthogonal projections onto ker⁡Ah\ker A_h and ker⁡(I−Ah)\ker(I-A_h).

Lemma 4.2 (Necessary endpoint inequalities). Every feasible affine velocity in (4.1) satisfies almost everywhere

P0BφP0⪰0,P1BφP1⪯0.P_0B_\varphi P_0 \succeq0, \qquad P_1B_\varphi P_1 \preceq0.

Proof. If v∈ker⁡Ah(u)v \in\ker A_h(u), then

0≤⟨Aht(u)v,v⟩=t⟨Bφ(u)v,v⟩,0 \le\langle A_{h_t}(u)v,v\rangle=t\langle B_\varphi(u)v,v\rangle,

so dividing by t>0t>0 and letting t↓0t \downarrow0 gives ⟨Bφv,v⟩≥0\langle B_\varphi v,v\rangle\ge0. Similarly, for v∈ker⁡(I−Ah(u))v \in\ker(I-A_h(u)),

0≤⟨(I−Aht)v,v⟩=−t⟨Bφv,v⟩,0 \le\langle(I-A_{h_t})v,v\rangle=-t\langle B_\varphi v,v\rangle,

which yields the upper inequality. □\square

These pointwise inequalities are only necessary; gluing across sign and branch interfaces is part of the global construction below.

First variation of volume

The first mixed-volume functional, evaluated on a C1,1C^{1,1} velocity, is

δVh(φ):=∫S3φ dS3(U4(1))=∫S3φ(u)det⁡Ah(u) dσ(u).(14)\delta V_h(\varphi):=\int_{S^3}\varphi\,dS_3(U_4^{(1)})=\int_{S^3}\varphi(u)\det A_h(u)\,d\sigma(u). \tag*{(14)}

Here S3S^3 is the unit sphere in H4=15H_4=1_5. For a feasible affine path this equals the derivative of volume at zero, by Minkowski’s first-variation formula. Before feasibility is proved we use it only as the displayed linear functional.

Let

D={u∈S(H4):∥u+∥≥∥u−∥}D=\{u\in S(H_4):\|u_+\|\geq\|u_-\|\}

be the first support branch. The spectrum calculation in Proposition 3.1 shows that det⁡Ah=0\det A_h=0 almost everywhere on DD. Since width one gives Ah(−u)=I−Ah(u)A_h(-u)=I-A_h(u) and an admissible velocity is odd,

δVh(φ)=∫D[φ(u)det⁡Ah(u)+φ(−u)det⁡Ah(−u)] dσ(u)=−∫Dφ(u)det⁡(I−Ah(u)) dσ(u).\begin{aligned} \delta V_h(\varphi)=\int_D[\varphi(u)\det A_h(u)+\varphi(-u)\det A_h(-u)]\,d\sigma(u) \\ &=-\int_D\varphi(u)\det(I-A_h(u))\,d\sigma(u). \end{aligned}

Thus

δVh(φ)=−∫Dφdet⁡(I−Ah) dσ.(15)\delta V_h(\varphi)=-\int_D\varphi\det(I-A_h)\,d\sigma. \tag*{(15)}

A feasible direction with a positive integral on the right therefore gives negative first volume variation.

Leaf-adapted parametrization and a localized perturbation

On the first branch in H4=15H_4=1_5, the homogeneous width-one support function is

h^(x)=12∥x+∥.(16)\widehat h(x)=\frac{1}{\sqrt{2}}\|x_+\|. \tag*{(16)}

Fix a smooth sign cell with positive coordinate set PP and put r=∥x+∥r=\|x_+\|. Write

x=r(p−q),p=x+r,q=−x−r.(17)x=r(p-q),\qquad p=\frac{x_+}{r},\qquad q=\frac{-x_-}{r}. \tag*{(17)}

Then

p,q≥0,∥p∥=1,∑pi=∑qj=:m,∥q∥≤1.(18)p,q\geq0,\qquad\|p\|=1,\qquad\sum p_i=\sum q_j=:m,\qquad\|q\|\leq1. \tag*{(18)}

On the open cone over the interior of a first-branch sign cell, let LpL_p be a fiber of the map x↦p=x+/∥x+∥x\mapsto p=x_+/\|x_+\|. Its tangent space is

TxLp=ker⁡D2h^(x)={w∈H4:wP∈span⁡{p}},T_xL_p=\ker D^2\widehat h(x)=\{w\in H_4:w_P\in\operatorname{span}\{p\}\},

where the Hessian is restricted to H4H_4 and wPw_P is the component of ww on the positive coordinate indices. Thus these fibers are the integral leaves of the Hessian kernel. At fixed rr and pp, variations of qq satisfying ∑qj=m\sum q_j=m lie in a slice of one such leaf; the unperturbed homogeneous support function has vanishing second derivative in these directions. Here null refers to the support Hessian and, on the sphere, to the curvature-radius operator.

Here mm is normalized: on the unit sphere it equals μ(u)/r(u)\mu(u)/r(u), where μ\mu is the unnormalized coordinate sum from Section 3 (denoted by m(u)m(u) in [5 Section 3]). The symbol h^\widehat h denotes the homogeneous width-one support, whereas HH in (10) has width two. The branch-switch set is ∥q∥=1\|q\|=1. The first branch has one, two, or three positive coordinates. The interface used below has two positive and three negative coordinates, or the antipodal sign pattern.

The reason for choosing this interface is visible in the negative-coordinate sections. Put k=∣P∣k=|P| and ℓ=5−k\ell=5-k, and suppress the zero coordinates of qq. At fixed r,pr,p (hence fixed mm), write

q=mℓ1ℓ+z,z⊥1ℓ,∥q∥2=m2ℓ+∥z∥2≤1.q=\frac{m}{\ell}\mathbf{1}_{\ell}+z,\qquad z\perp\mathbf{1}_{\ell},\qquad\|q\|^2=\frac{m^2}{\ell}+\|z\|^2\leq1.

Thus the section is given by ∥z∥2≤1−m2/ℓ\|z\|^2\leq1-m^2/\ell, with the coordinate conditions qj>0q_j>0 still imposed. For k=2k=2, its limiting radius as m↑2m\uparrow\sqrt{2} is 1/31/\sqrt{3}, and the section retains nonempty two-dimensional relative interior around (2/3)13(\sqrt{2}/3)_{13}. For k=3k = 3, the radius tends to zero and the section contracts to the single point (1,1)/2(1,1)/\sqrt{2}. This contrast motivates placing the positive perturbation on the two-positive cells and its compensating continuation on the three-positive cells near m=2m = \sqrt{2}; the weighted volume comparison is proved below.

Fix

c=45,0<δ<2−75,m0=2−δ,(19)c = \frac{4}{5}, \qquad0 < \delta< \sqrt{2} - \frac{7}{5}, \qquad m_0 = \sqrt{2} - \delta, \tag*{(19)}

and define

χδ(m)=(m−m0)+4,F(y)=∑i(yi−c)+4.(20)\chi_\delta(m) = (m-m_0)_+^4, \qquad F(y) = \sum_i (y_i-c)_+^4. \tag*{(20)}

The cutoff χδ\chi_\delta restricts the perturbation to m>2−δm > \sqrt{2}-\delta, near m=2m = \sqrt{2} on the active branches. We use cap as shorthand for this localized perturbation. The function FF is convex, permutation invariant, and

y⋅∇F(y)−F(y)=∑i(yi−c)+3(3yi+c)≥0.(21)y \cdot\nabla F(y) - F(y) = \sum_i (y_i-c)_+^3(3y_i+c) \ge0. \tag*{(21)}

The numerical-looking constant 4/54/5 is chosen for a simple exact geometric reason.

Lemma 4.3 (The cutoff is inactive near coordinate interfaces). On the support of χδ\chi_\delta, the functions FF and DFDF vanish in a neighborhood of every coordinate interface of the relevant two-coordinate leaves.

Proof. Let (a,b)(a,b) be a nonnegative unit two-vector with a+b=ma+b=m. Solving a2+b2=1a^2+b^2=1 and a+b=ma+b=m gives

amax⁡(m)=m+2−m22.a_{\max}(m) = \frac{m+\sqrt{2-m^2}}{2}.

For m>1m>1 this is strictly decreasing, and

amax⁡(7/5)=45.a_{\max}(7/5) = \frac{4}{5}.

On the support of χδ\chi_\delta we have m≥m0>7/5m \ge m_0 > 7/5, hence each coordinate is strictly below 4/54/5 when the configuration approaches the coordinate boundary that would change the sign pattern. The same upper bound applies to a nonnegative two-vector of norm at most one: at fixed sum mm, its largest coordinate is maximized when the norm is one. This covers the negative leaf when one of its three coordinates vanishes. On a positive three-vector boundary the norm is already one. The remaining one-positive boundary has m=1<m0m = 1 < m_0 and is excluded by χδ\chi_\delta itself. The strict gap m0>7/5m_0 > 7/5 makes these statements hold on neighborhoods of the interfaces. The remaining 3↔43 \leftrightarrow4 interface cannot meet the active first branch: there q→(m,0)q \to(m,0) up to permutation, contradicting ∥q∥≤1\lVert q\rVert\le1 and m≥m0>1m \ge m_0 > 1. Therefore every positive-part factor (yi−4/5)+(y_i-4/5)_+ is identically zero on a neighborhood of that interface; the same holds for its first derivative. □\square

On a two-positive first-branch cell define

G2,δ(r(p−q))=rχδ(m)F(q)≥0.(22)G_{2,\delta}(r(p-q)) = r\chi_\delta(m)F(q) \ge0. \tag*{(22)}

For a positive unit three-vector pp define

Γδ(p)=12[mχδ′(m)F(p)+χδ(m)(p⋅∇F(p)−F(p))]≥0,(23)\Gamma_\delta(p) = \frac{1}{2}\left[m\chi_\delta'(m)F(p) + \chi_\delta(m)(p\cdot\nabla F(p)-F(p))\right] \ge0, \tag*{(23)}

and on a three-positive cell set

G3,δ(r(p−q))=r[−χδ(m)F(p)+Γδ(p)(∥q∥2−1)]≤0.(24)G_{3,\delta}(r(p-q)) = r\left[-\chi_\delta(m)F(p)+\Gamma_\delta(p)(\lVert q\rVert^2-1)\right] \le0. \tag*{(24)}

On one-positive cells set Gδ=0G_\delta=0, and define the second support branch by oddness, Gδ(−x)=−Gδ(x)G_\delta(-x)=-G_\delta(x).

Finally put

φδ=Gδ∣S(H4).(25)\varphi_\delta= G_\delta|_{S(H_4)}. \tag*{(25)}

Matching across the mixed branch

The correction Γδ(∥q∥2−1)\Gamma_\delta(\lVert q\rVert^2-1) in (24) is designed exactly so that the two branch formulas match to first order.

Lemma 4.4 (Exact C1C^1 matching). Across every active mixed 2+32+3 branch-switch interface, the two formulas for GδG_\delta have the same value and differential.

Proof. At a mixed branch point write the positive two-vector as yy, the absolute negative three-vector as zz, and set

r=∥y∥,R=∥z∥,S=∑yi=∑zj.r=\lVert y\rVert,\qquad R=\lVert z\rVert,\qquad S=\sum y_i=\sum z_j.

The branch equation is r=Rr=R. Define

Ψ(ρ)=ρχδ(S/ρ)F(z/ρ).(26)\Psi(\rho)=\rho\chi_\delta(S/\rho)F(z/\rho). \tag*{(26)}

The two-positive formula is Ψ(r)\Psi(r). On the opposite branch, oddness of (24) gives

Gopp=Ψ(R)−Γδ(z/R)(r2R−R).(27)G_{\mathrm{opp}}=\Psi(R)-\Gamma_\delta(z/R)\left(\frac{r^2}{R}-R\right). \tag*{(27)}

At r=Rr=R the correction factor vanishes, so the values agree. Differentiate (26). Writing p=z/ρp=z/\rho and m=S/ρm=S/\rho, Euler differentiation gives

Ψ′(ρ)=χδ(m)F(p)−mχδ′(m)F(p)−χδ(m)p⋅∇F(p)=−2Γδ(p).\Psi'(\rho)=\chi_\delta(m)F(p)-m\chi_\delta'(m)F(p)-\chi_\delta(m)p\cdot\nabla F(p)=-2\Gamma_\delta(p).

At r=Rr=R,

d(r2R−R)=2(dr−dR).d\left(\frac{r^2}{R}-R\right)=2(dr-dR).

Here Ψ′\Psi' is the derivative in ρ\rho with S,zS,z fixed. When the point varies, the S,zS,z differential terms of Ψ(r)\Psi(r) and Ψ(R)\Psi(R) agree on r=Rr=R and cancel in their difference. Thus

d(Ψ(r)−Ψ(R))=−2Γδ(z/R)(dr−dR).d(\Psi(r)-\Psi(R))=-2\Gamma_\delta(z/R)(dr-dR).

The differential of the correction term in (27) has exactly this value; derivatives of Γδ\Gamma_\delta are multiplied by the vanishing factor r2/R−Rr^2/R-R. Hence dGopp=dΨ(r)dG_{\mathrm{opp}}=d\Psi(r), as required. □

Proposition 4.5 (Regularity and symmetry). The piecewise function GδG_\delta is positively one-homogeneous, odd, S5S_5-invariant, and belongs to Cloc1,1(H4∖{0})C^{1,1}_{\mathrm{loc}}(H_4\setminus\{0\}). Consequently φδ∈C1(S(H4))\varphi_\delta\in C^1(S(H_4)).

Proof. Each formula is one-homogeneous because p,q,mp,q,m are scale invariant and the only dimensional factor is rr. Permutation invariance follows from the symmetric definitions of FF and mm, and oddness is imposed by definition. Lemma 4.4 gives C1C^1 matching across the active branch interface, while Lemma 4.3 makes the perturbation identically zero near coordinate interfaces. On each remaining compact piece the displayed formulas have bounded second derivatives. A finite piecewise C1C^1 function with uniformly bounded piecewise Hessian is C1,1C^{1,1}. □

Verification of the endpoint curvature inequalities

We now verify Lemma 4.2 for the constructed velocity. The calculation is most transparent in homogeneous leaf coordinates.

Lemma 4.6 (Endpoint feasibility of the cap). Let

Bφδ:=∇2φδ+φδI.B_{\varphi_\delta}:=\nabla^2\varphi_\delta+\varphi_\delta I.

Then almost everywhere

P0BφδP0⪰0,P1BφδP1⪯0.P_0B_{\varphi_\delta}P_0\succeq0,\qquad P_1B_{\varphi_\delta}P_1\preceq0.

Proof. For lower-endpoint directions, the null directions of the homogeneous support Hessian are the radial direction together with the zero-sum directions supported on the negative coordinates. Indeed the Hessian of ∥x+∥\lVert x_+\rVert vanishes precisely when the positive part of a vector is parallel to x+x_+. Subtracting a radial vector leaves such a negative zero-sum vector. The Hessian of every one-homogeneous perturbation annihilates the radial vector, so its quadratic form on a spherical null direction is the same as on the corresponding leaf direction. On a two-positive cell, the $q

dependence of (22) is through the convex function F(q)F(q), so the corresponding homogeneous Hessian is positive semidefinite. On a three-positive cell the qq-dependent correcting term is

rΓδ(p)∥q∥2,r\Gamma_\delta(p)\lVert q\rVert^2,

whose qq Hessian is 2rΓδ(p)I⪰02r\Gamma_\delta(p)I \succeq0 by (4.12). This proves the lower endpoint inequality.

For the upper endpoint we use the explicit principal radii. On a width-one two-positive cell the unique nonzero radius, denoted by λ2\lambda_2, is nonsaturated in the interior and equals

λ2=(3+m2)1+∥q∥252.(28)\lambda_2=\frac{(3+m^2)\sqrt{1+\lVert q\rVert^2}}{5\sqrt{2}}. \tag*{(28)}

It reaches 11 only at the mixed branch endpoint m=2m=\sqrt{2}, ∥q∥=1\lVert q\rVert=1. Here the positive unit vector is p=(1,1)/2p=(1,1)/\sqrt{2}, and the saturated vector ww is supported on its two coordinates with zero sum. Along x+twx+tw the negative coordinates and their sum are fixed, while r′(0)=0r'(0)=0 and r′′(0)=∥w∥2/rr''(0)=\lVert w\rVert^2/r. Thus G2,δ=Ψ(r)G_{2,\delta}=\Psi(r), and Ψ′=−2Γδ\Psi'=-2\Gamma_\delta from the matching calculation yields

D2Gδ[w,w]=−2Γδ(q)r∥w∥2≤0.(29)D^2G_\delta[w,w]=-\frac{2\Gamma_\delta(q)}{r}\lVert w\rVert^2\leq0. \tag*{(29)}

On a three-positive cell the two positive radii are

λ3,1=1+∥q∥22,λ3,2=(2+m2)1+∥q∥252.(30)\lambda_{3,1}=\frac{\sqrt{1+\lVert q\rVert^2}}{\sqrt{2}},\qquad \lambda_{3,2}=\frac{(2+m^2)\sqrt{1+\lVert q\rVert^2}}{5\sqrt{2}}. \tag*{(30)}

The second is at most 4/54/5, so only λ3,1\lambda_{3,1} can saturate at 11, and it does so exactly on ∥q∥=1\lVert q\rVert=1. Its saturated vector ww is supported on the three positive coordinates and satisfies ∑wi=0\sum w_i=0 and p⋅w=0p\cdot w=0. To display the cancellation, put L(p)=χδ(m)F(p)L(p)=\chi_\delta(m)F(p), where m=∑pim=\sum p_i, so that p⋅∇L−L=2Γδ(p)p\cdot\nabla L-L=2\Gamma_\delta(p). Along x+twx+tw at the interface,

r′(0)=0,r′′(0)=∥w∥2r,p′(0)=wr,p′′(0)=−p∥w∥2r2,(∥q∥2)′′(0)=−2∥w∥2r2.r'(0)=0,\qquad r''(0)=\frac{\lVert w\rVert^2}{r},\qquad p'(0)=\frac{w}{r},\qquad p''(0)=-\frac{p\lVert w\rVert^2}{r^2},\qquad(\lVert q\rVert^2)''(0)=-\frac{2\lVert w\rVert^2}{r^2}.

Consequently the two terms in (24) have second derivatives

(−rL(p))′′=2Γδ(p)∥w∥2−χδ(m)D2F(p)[w,w]r,(rΓδ(p)(∥q∥2−1))′′=−2Γδ(p)∥w∥2r.(-rL(p))''=\frac{2\Gamma_\delta(p)\lVert w\rVert^2-\chi_\delta(m)D^2F(p)[w,w]}{r}, \qquad \left(r\Gamma_\delta(p)(\lVert q\rVert^2-1)\right)''=-\frac{2\Gamma_\delta(p)\lVert w\rVert^2}{r}.

Here D2L(p)[w,w]=χδ(m)D2F(p)[w,w]D^2L(p)[w,w]=\chi_\delta(m)D^2F(p)[w,w] because ∑wi=0\sum w_i=0. Adding gives

D2Gδ[w,w]=−χδ(m)rD2F(p)[w,w]=−12χδ(m)r∑i(pi−45)2wi2≤0.(31)D^2G_\delta[w,w]=-\frac{\chi_\delta(m)}{r}D^2F(p)[w,w] =-\frac{12\chi_\delta(m)}{r}\sum_i\left(p_i-\frac{4}{5}\right)^2w_i^2\leq0. \tag*{(31)}

The endpoint inequalities hold for the continuous one-sided Hessian extensions on the closures of the smooth pieces. On first-branch mixed closures, the positive radii stay bounded away from zero, so no new lower kernel appears; the lower quadratic forms retain their signs. The only newly saturated upper directions are those checked in (29) and (31). Near coordinate-sign interfaces the cap vanishes identically, so rank changes there impose no further condition. At the cutoff m=m0m=m_0 and hinge thresholds yi=cy_i=c, the newly activated terms, including their corrections, have vanishing derivatives through order two. On one-positive cells the cap is zero. These observations also cover intersections of the interfaces. The antipodal cases follow from oddness and Ah(−u)=I−Ah(u)A_h(-u)=I-A_h(u). □

The sign of the first variation

Define

Iδ=∫Dφδ(u)det⁡(I−Ah(u)) dσ(u)=I2,δ+I3,δ.(32)I_\delta=\int_D\varphi_\delta(u)\det(I-A_h(u))\,d\sigma(u)=I_{2,\delta}+I_{3,\delta}. \tag*{(32)}

where the two terms come from the two-positive and three-positive cells. By construction I2,δ≥0I_{2,\delta}\geq0 and I3,δ≤0I_{3,\delta}\leq0.

Proposition 4.7 (Asymptotic dominance of the two-positive cap). There are constants C2,C3>0C_2,C_3>0 such that, for all sufficiently small δ>0\delta>0,

I2,δ≥C2δ9/2,∣I3,δ∣≤C3δ13/2.(33)I_{2,\delta}\geq C_2\delta^{9/2},\qquad|I_{3,\delta}|\leq C_3\delta^{13/2}. \tag*{(33)}

Hence Iδ>0I_\delta>0 for all sufficiently small δ\delta.

Proof. On a two-positive unit vector write

p(θ)=(cos⁡θ,sin⁡θ)p(\theta) = (\cos\theta,\sin\theta), m(θ)=cos⁡θ+sin⁡θ=2cos⁡(θ−π/4)m(\theta) = \cos\theta+ \sin\theta= \sqrt{2}\cos(\theta-\pi/4).

Use q1,q2q_1,q_2 as independent leaf coordinates and set q3=m−q1−q2q_3=m-q_1-q_2. The parametrization

u=(p,−q)/1+∥q∥2u=(p,-q)/\sqrt{1+\lVert q\rVert^2}

has spherical measure

dσ(u)=5(1+∥q∥2)2 dθ dq1 dq2.d\sigma(u)=\frac{\sqrt{5}}{(1+\lVert q\rVert^2)^2}\,d\theta\,dq_1\,dq_2.

For clarity, in a cell with ℓ\ell negative coordinates write q=(m/ℓ)1ℓ+zq=(m/\ell)\mathbf{1}_{\ell}+z, ∑zi=0\sum z_i=0. On the slice ∥p∥=1\lVert p\rVert=1 the Gram determinant relative to dσ(p) dzd\sigma(p)\,dz is (5−m2)/ℓ(5-m^2)/\ell. Radial projection to the sphere multiplies its area element by (1−m2/5)−1/2(1+∥q∥2)−2(1-m^2/5)^{-1/2}(1+\lVert q\rVert^2)^{-2}. Thus the resulting density is 5/ℓ(1+∥q∥2)−2dσ(p) dz\sqrt{5/\ell}(1+\lVert q\rVert^2)^{-2}d\sigma(p)\,dz; the displayed formula uses dz=3 dq1dq2dz=\sqrt{3}\,dq_1dq_2. Taylor expansion at π/4\pi/4 gives

2−m(θ)=22(θ−π/4)2+O((θ−π/4)4).\sqrt{2}-m(\theta)=\frac{\sqrt{2}}{2}(\theta-\pi/4)^2+O((\theta-\pi/4)^4).

Thus the angular set on which m≥2−δ/2m\ge\sqrt{2}-\delta/2 has length comparable to δ\sqrt{\delta}. There

χδ(m)=(m−2+δ)4≥(δ/2)4.\chi_\delta(m)=(m-\sqrt{2}+\delta)^4\ge(\delta/2)^4.

Such a negative-leaf patch exists explicitly: at m=2m=\sqrt{2} take

q=(1720,2−17/202,2−17/202).q=\left(\frac{17}{20},\frac{\sqrt{2}-17/20}{2},\frac{\sqrt{2}-17/20}{2}\right).

All coordinates are positive, ∥q∥<1\lVert q\rVert<1, and F(q)>0F(q)>0. A small patch around it varies continuously for nearby mm. Choose such a compact interior patch of the negative leaf for which F(q)>0F(q)>0 and which stays away from all coordinate and branch boundaries. On this fixed patch the spherical Jacobian and det⁡(I−Ah)\det(I-A_h) have positive lower bounds independent of δ\delta. Integrating over the angular cap and this fixed leaf patch therefore yields

I2,δ≥c2δ4δ=c2δ9/2.I_{2,\delta}\ge c_2\delta^4\sqrt{\delta}=c_2\delta^{9/2}.

For the three-positive contribution, the negative leaf has two coordinates. Write

q1=m2+d,q2=m2−d,∣d∣≤η(m):=122−m2.q_1=\frac{m}{2}+d,\qquad q_2=\frac{m}{2}-d,\qquad|d|\le\eta(m):=\frac{1}{2}\sqrt{2-m^2}.

Let α\alpha be the angular coordinate on the circle {p∈S2:∑pi=m}\{p\in S^2:\sum p_i=m\}. Then dσS2(p)=dm dα/3d\sigma_{S^2}(p)=dm\,d\alpha/\sqrt{3} and dz=2 dddz=\sqrt{2}\,dd, so the same radial calculation gives

dσ(u)=5/3(1+∥q∥2)2 dm dα dd.d\sigma(u)=\frac{\sqrt{5/3}}{(1+\lVert q\rVert^2)^2}\,dm\,d\alpha\,dd.

This density is bounded uniformly for m0≤m≤2m_0\le m\le\sqrt{2}; the range of α\alpha has length at most 2π2\pi. A direct calculation gives

1−∥q∥2=2(η(m)2−d2).(34)1-\lVert q\rVert^2=2(\eta(m)^2-d^2). \tag*{(34)}

Let

x=m−m0,y=2−m,x+y=δ.x=m-m_0,\qquad y=\sqrt{2}-m,\qquad x+y=\delta.

On the active cap, 0≤x≤δ0\le x\le\delta. From (20) and (23),

χδ=O(x4),Γδ=O(x3).\chi_\delta=O(x^4),\qquad\Gamma_\delta=O(x^3).

Writing η=η(m)\eta=\eta(m), we have η2=y(2+m)/4=O(y)\eta^2=y(\sqrt{2}+m)/4=O(y). By (30), λ3,2≤4/5\lambda_{3,2}\le4/5 and

1−λ3,1=2(η2−d2)2(2+1+∥q∥2).1-\lambda_{3,1}=\frac{2(\eta^2-d^2)}{\sqrt{2}(\sqrt{2}+\sqrt{1+\lVert q\rVert^2})}.

Thus det⁡(I−Ah)\det(I-A_h) is bounded above by a constant times η2−d2\eta^2-d^2. The bounded density just computed and the identities

∫−ηη(η2−d2) dd=43η3,∫−ηη(η2−d2)2 dd=1615η5\int_{-\eta}^{\eta}(\eta^2-d^2)\,dd=\frac{4}{3}\eta^3,\qquad \int_{-\eta}^{\eta}(\eta^2-d^2)^2\,dd=\frac{16}{15}\eta^5

give, with constants independent of small δ\delta,

∣I3,δ∣≤C∫0δ[x4(δ−x)3/2+x3(δ−x)5/2] dx.|I_{3,\delta}| \le C\int_{0}^{\delta}\left[x^4(\delta-x)^{3/2}+x^3(\delta-x)^{5/2}\right]\,dx.

Rescaling x=δsx=\delta s gives

∣I3,δ∣≤C3δ13/2,|I_{3,\delta}|\le C_3\delta^{13/2},

because both beta-type integrals in s∈[0,1]s\in[0,1] are finite. Since 13/2>9/213/2>9/2, the positive two-cell contribution dominates for sufficiently small δ\delta.

By (15),

δVh(φδ)=−Iδ<0(35)\delta V_h(\varphi_\delta)=-I_\delta<0 \tag*{(35)}

for all sufficiently small δ\delta.

Strict curvature margins and construction of an admissible support path

Endpoint feasibility is non-strict, so it is not by itself a uniform finite-tt convexity certificate. We create a small spectral margin by moving slightly toward the width-one ball. Let

b(u)=12−h(u).(36)b(u)=\frac{1}{2}-h(u). \tag*{(36)}

This function is odd, and

Bb=∇2b+bI=12I−Ah.B_b=\nabla^2b+bI=\frac{1}{2}I-A_h.

Define the modified perturbation direction

φ~δ=φδ+δ5(12−h).(37)\widetilde{\varphi}_\delta=\varphi_\delta+\delta^5\left(\frac{1}{2}-h\right). \tag*{(37)}

The tilde denotes the modified perturbation direction, now with a strict spectral margin. On the two saturated subspaces,

Bφ~δ∣ker⁡Ah⪰δ52I,Bφ~δ∣ker⁡(I−Ah)⪯−δ52I.(38)B_{\widetilde{\varphi}_\delta}\big|_{\ker A_h}\succeq\frac{\delta^5}{2}I,\qquad B_{\widetilde{\varphi}_\delta}\big|_{\ker(I-A_h)}\preceq-\frac{\delta^5}{2}I. \tag*{(38)}

Since ∣δVh(b)∣≤2π2∥b∥∞|\delta V_h(b)|\le2\pi^2\|b\|_\infty, the added term changes the first variation by O(δ5)O(\delta^5) with a constant independent of δ\delta, whereas the negative contribution in (35) has magnitude at least a constant multiple of δ9/2\delta^{9/2}. Since 5>9/25>9/2,

δVh(φ~δ)<0(39)\delta V_h(\widetilde{\varphi}_\delta)<0 \tag*{(39)}

for all sufficiently small δ\delta.

We use one elementary compactness lemma to pass from the infinitesimal spectral inequalities to a genuine path.

Lemma 4.8 (Uniform matrix strictification). Let A(x),C(x)A(x),C(x) be continuous symmetric matrices on a compact set, with 0⪯A(x)⪯I0\preceq A(x)\preceq I. Assume that for some η>0\eta>0,

C∣ker⁡A⪰ηI,C∣ker⁡(I−A)⪯−ηIC\big|_{\ker A}\succeq\eta I,\qquad C\big|_{\ker(I-A)}\preceq-\eta I

at every point. Then there is t0>0t_0>0 such that

0⪯A+tC⪯I(0≤t≤t0)0\preceq A+tC\preceq I\qquad(0\le t\le t_0)

uniformly on the compact set.

Proof. Suppose the lower inequality failed for a sequence tj↓0t_j\downarrow0. Then there are points xjx_j and unit vectors vjv_j with

⟨(A(xj)+tjC(xj))vj,vj⟩<0.\left\langle\left(A(x_j)+t_jC(x_j)\right)v_j,v_j\right\rangle<0.

By compactness, after passing to a subsequence, xj→xx_j\to x and vj→vv_j\to v. Boundedness of CC and A⪰0A\succeq0 give

0≤⟨A(xj)vj,vj⟩<tj∥C(xj)∥,⟨C(xj)vj,vj⟩<0.0\le\langle A(x_j)v_j,v_j\rangle<t_j\|C(x_j)\|,\qquad \langle C(x_j)v_j,v_j\rangle<0.

Taking limits yields v∈ker⁡A(x)v\in\ker A(x) and ⟨C(x)v,v⟩≤0\langle C(x)v,v\rangle\le0, contradicting the strict positive bound. Apply the same argument to I−AI-A and −C-C for the upper inequality. ∎

For fixed δ\delta, partition the sphere by coordinate signs, support branches, and cutoff and hinge thresholds, and take the finitely many piece closures. On each closure, AhA_h and BφδB_{\varphi_\delta} have continuous one-sided extensions: on the first branch r=∥u+∥≥1/2r=\lVert u_+\rVert\ge1/\sqrt{2}, and the positive-part formulas are smooth on their respective pieces; the opposite branch follows by antipodality. Lemma 4.6 covers these extensions, including newly saturated boundary directions. Thus C=Bφδ+δ5(12I−Ah)C=B_{\varphi_\delta}+\delta^5(\frac{1}{2}I-A_h) satisfies the strict endpoint conditions with η=δ5/2\eta=\delta^5/2 on every closed piece. Using finitely many compact patches with local orthonormal tangent frames, apply Lemma 4.8 and take the minimum of the resulting positive times to obtain a common tδ>0t_\delta>0.

Theorem 4.9 (A feasible symmetric descent family). There exists δ∗>0\delta_* > 0 such that, for every 0<δ<δ∗0<\delta<\delta_*, there is tδ>0t_\delta>0 for which

hδ,t=h+tφ~δ,0≤t<tδ,(40)h_{\delta,t}=h+t\widetilde{\varphi}_\delta,\qquad0\le t<t_\delta, \tag*{(40)}

is the support function of an S5S_5-invariant convex body Kδ,tK_{\delta,t} of constant width one. For all sufficiently small t>0t>0,

Vol⁡4(Kδ,t)<Vol⁡4(U4(1)).(41)\operatorname{Vol}_4(K_{\delta,t})<\operatorname{Vol}_4(U_4^{(1)}). \tag*{(41)}

Consequently U4(1)U_4^{(1)} is not a local volume minimizer in W4,1W_{4,1}.

Proof. Proposition 4.5 shows that φδ\varphi_\delta is odd, S5S_5-invariant and C1,1C^{1,1}. The ball direction b=12−hb=\frac{1}{2}-h has the same properties, so (37) implies that φ~δ\widetilde{\varphi}_\delta does as well. Hence

hδ,t(u)+hδ,t(−u)=1.h_{\delta,t}(u)+h_{\delta,t}(-u)=1.

The compactness argument above gives

0⪯Ah+tBφ~δ⪯I0\preceq A_h+tB_{\widetilde{\varphi}_\delta}\preceq I

on every smooth piece for 0≤t<tδ0\le t<t_\delta. Since hδ,t∈C1,1h_{\delta,t}\in C^{1,1}, nonnegativity of the homogeneous curvature-radius operator is the support-function convexity criterion. More explicitly, the homogeneous extension has positive semidefinite Hessian almost everywhere away from the origin. Its Cloc1,1C_{\mathrm{loc}}^{1,1} regularity rules out negative singular Hessian terms at the interfaces, so its restriction to every segment avoiding the origin is convex. On a line through the origin, for a unit vector uu, the extension equals τhδ,t(u)\tau h_{\delta,t}(u) for τ≥0\tau\ge0 and −τhδ,t(−u)-\tau h_{\delta,t}(-u) for τ≤0\tau\le0. The right derivative minus the left derivative is hδ,t(u)+hδ,t(−u)=1h_{\delta,t}(u)+h_{\delta,t}(-u)=1. Thus the restriction to these lines is also convex. Hence hδ,th_{\delta,t} is the support function of a convex body. The antipodal identity gives width one, and the construction is S5S_5-invariant. Finally,

Vol⁡4(Kδ,t)=Vol⁡4(U4(1))+t δVh(φ~δ)+o(t),\operatorname{Vol}_4(K_{\delta,t})=\operatorname{Vol}_4(U_4^{(1)})+t\,\delta V_h(\widetilde{\varphi}_\delta)+o(t),

and the coefficient is strictly negative by (39). Therefore the volume is smaller for all sufficiently small positive tt. □

Equivalently, the deformed body can be written directly as

Kδ,t=⋂u∈S(H4){x∈H4:⟨x,u⟩≤hδ,t(u)}.K_{\delta,t}=\bigcap_{u\in S(H_4)}\{x\in H_4:\langle x,u\rangle\le h_{\delta,t}(u)\}.

Thus the result is not merely an abstract existence theorem: the formulas (22), (24), and (37) define an explicit nearby family. The choices “δ\delta sufficiently small” and “tt sufficiently small” have been justified analytically, without assigning numerical endpoints to the allowable ranges. Thus the theorem proves strict descent and global feasibility; it supplies no six-decimal volume for a specified optimized member of this family.

Remark 4.10 (One-sided and two-sided questions). The path only uses positive tt. A two-sided Minkowski decomposition asks for feasibility in both directions, which is a stronger requirement. Restrictions on two-sided perturbations therefore do not rule out the one-sided descent just constructed.

A lower bound for all four-dimensional constant-width bodies

In this independent section, pp denotes the support function of an arbitrary body KK of constant width one, and S3(K)S_3(K) denotes its surface area. We first obtain a surface-area lower bound from the curvature constraint, then convert it to volume using an inscribed ball.

A spectral surface-area estimate

5.1. A spectral surface-area estimate. First suppose pp is smooth and write p=1/2+fp=1/2+f. Constant width makes ff odd. A translation removes its degree-one spherical harmonic without changing ∇2f+fI\nabla^2f+fI. Set

A=∇2f+fI,E(f)=∫S3(∣∇f∣2−3f2) dσ.A=\nabla^2f+fI,\qquad\mathcal{E}(f)=\int_{S^3}\left(\lvert\nabla f\rvert^2-3f^2\right)\,d\sigma.

The eigenvalues of AA lie in [−1/2,1/2][-1/2,1/2]. Here AA is the centered curvature matrix: the support curvature matrix from the preceding sections is Ap=12I+AA_p=\frac{1}{2}I+A. Throughout this section, dσd\sigma is unnormalized spherical surface measure, so σ(S3)=2π2\sigma(S^3)=2\pi^2. Our norm conventions are

∥f∥22:=∫S3∣f(u)∣2 dσ(u),∥A∥22:=∫S3∥A(u)∥F2 dσ(u),\lVert f\rVert_2^2:=\int_{S^3}\lvert f(u)\rvert^2\,d\sigma(u),\qquad \lVert A\rVert_2^2:=\int_{S^3}\lVert A(u)\rVert_F^2\,d\sigma(u),

where ∥A(u)∥F\lVert A(u)\rVert_F is the pointwise Frobenius (Hilbert–Schmidt) norm. Thus ∥A∥22\lVert A\rVert_2^2 is a spherical L2L^2 norm of a matrix field.

Lemma 5.1 (Spectral identities). Let fℓf_\ell be the degree-ℓ\ell spherical harmonic component of ff, and λℓ=ℓ(ℓ+2)\lambda_\ell=\ell(\ell+2). Then

S3(K)=π24−12E(f),S_3(K)=\frac{\pi^2}{4}-\frac{1}{2}\mathcal{E}(f),
E(f)=∑ℓ=3,5,…(λℓ−3)∥fℓ∥22,\mathcal{E}(f)=\sum_{\ell=3,5,\ldots}(\lambda_\ell-3)\lVert f_\ell\rVert_2^2,
∥A∥22=∑ℓ=3,5,…(λℓ−1)(λℓ−3)∥fℓ∥22.\lVert A\rVert_2^2=\sum_{\ell=3,5,\ldots}(\lambda_\ell-1)(\lambda_\ell-3)\lVert f_\ell\rVert_2^2.

Proof. Oddness gives A(−u)=−A(u)A(-u)=-A(u) after identifying antipodal tangent spaces. In the expansion of det⁡(12I+A)\det(\frac{1}{2}I+A), the linear and cubic terms therefore integrate to zero. If σ2(A)\sigma_2(A) is the second elementary symmetric function of its eigenvalues, then

S3(K)=∣S3∣8+12∫S3σ2(A) dσ.S_3(K)=\frac{\lvert S^3\rvert}{8}+\frac{1}{2}\int_{S^3}\sigma_2(A)\,d\sigma.

The identity 2σ2(A)=(tr⁡A)2−∥A∥F22\sigma_2(A)=(\operatorname{tr}A)^2-\lVert A\rVert_F^2, integration by parts, and the integrated Bochner formula on S3S^3 give

∫∣∇2f∣2=∫(Δf)2−2∫∣∇f∣2,∫S3σ2(A)=3∫f2−∫∣∇f∣2.\int\lvert\nabla^2f\rvert^2=\int(\Delta f)^2-2\int\lvert\nabla f\rvert^2,\qquad \int_{S^3}\sigma_2(A)=3\int f^2-\int\lvert\nabla f\rvert^2.

This proves the area identity since ∣S3∣=2π2\lvert S^3\rvert=2\pi^2. On a degree-ℓ\ell harmonic, −Δfℓ=λℓfℓ-\Delta f_\ell=\lambda_\ell f_\ell. Expanding ∥∇2f+fI∥22\lVert\nabla^2f+fI\rVert_2^2 gives (λℓ2−4λℓ+3)∥fℓ∥22(\lambda_\ell^2-4\lambda_\ell+3)\lVert f_\ell\rVert_2^2. Orthogonality of distinct degrees finishes the proof. □\square

Since the first remaining eigenvalue is λ3=15\lambda_3=15,

E(f)≤114∥A∥22≤114⋅34∣S3∣=3π228.\mathcal{E}(f)\leq\frac{1}{14}\lVert A\rVert_2^2\leq\frac{1}{14}\cdot\frac{3}{4}\lvert S^3\rvert=\frac{3\pi^2}{28}.

Consequently

S3(K)≥11π256.(42)S_3(K)\geq\frac{11\pi^2}{56}. \tag*{(42)}

From surface area to volume

Jung’s theorem places a diameter-one body in a ball of radius at most RJ=2/5R_J=\sqrt{2/5}. Choose its centre as the origin. Then p(u)≤RJp(u)\le R_J, and width one implies p(u)=1−p(−u)≥1−RJ=:rJp(u)=1-p(-u)\ge1-R_J=:r_J. Thus the concentric ball of radius rJr_J lies inside KK. Minkowski’s formula yields

4Vol⁡4(K)=∫S3p dS3(K)≥rJS3(K).4\operatorname{Vol}_4(K)=\int_{S^3}p\,\mathrm{d}S_3(K)\ge r_JS_3(K).

Combining this with (42) gives

Vol⁡4(K)≥11π2224(1−2/5)=0.1781370691…(43)\operatorname{Vol}_4(K)\ge\frac{11\pi^2}{224}(1-\sqrt{2/5})=0.1781370691\ldots \tag*{(43)}

The translation used here may differ from the one used to remove the degree-one harmonic; surface area and volume are translation invariant.

The smoothness restriction can be removed by averaging the support function against a smooth approximate identity on the rotation group, then mixing with a vanishing amount of the radius-1/21/2 ball if strict curvature is needed. These operations preserve width one and converge in Hausdorff distance. Continuity of volume and surface area proves the same bounds for every constant-width body.

An explicit improvement of the preceding bound

There are two sources of nonsharpness in the preceding estimate: the curvature eigenvalues need not all have maximal absolute value, and harmonics of degree at least five satisfy a stronger spectral inequality. An elementary great-circle argument shows that these two losses cannot both be too small.

Theorem 5.2 (An explicit spectral surface-area gap). Put

rJ=1−2/5,εS=729π4480000.r_J=1-\sqrt{2/5},\qquad\varepsilon_S=\frac{729\pi}{4480000}.

Every convex body K⊂R4K\subset\mathbb{R}^4 of constant width one satisfies

S3(K)≥11π256+εS,(44)S_3(K)\ge\frac{11\pi^2}{56}+\varepsilon_S, \tag*{(44)}
Vol⁡4(K)≥11π2224rJ+rJεS4>0.17818404.(45)\operatorname{Vol}_4(K)\ge\frac{11\pi^2}{224}r_J+\frac{r_J\varepsilon_S}{4}>0.17818404. \tag*{(45)}

The improvement over (5.2) exceeds 4.69⋅10−54.69\cdot10^{-5}; a large gap to the upper constructions remains.

Proof. First use a smooth support p=1/2+fp=1/2+f and remove its degree-one part. Write A=∇2f+fIA=\nabla^2f+fI, so its three eigenvalues are in [−1/2,1/2][-1/2,1/2]. Let f3f_3 be the degree-three part and set

A3=∇2f3+f3I,AR=A−A3,Dcurv=3π22−∥A∥22≥0,Z=∥tr⁡AR∥22.A_3=\nabla^2f_3+f_3I,\qquad A_R=A-A_3,\qquad D_{\mathrm{curv}}=\frac{3\pi^2}{2}-\lVert A\rVert_2^2\ge0,\qquad Z=\lVert\operatorname{tr}A_R\rVert_2^2.

Lemma 5.1 gives, degree by degree,

S3(K)−11π256=Dcurv28+∑ℓ=5,7,…(λℓ−15)(λℓ−3)28∥fℓ∥22.S_3(K)-\frac{11\pi^2}{56}=\frac{D_{\mathrm{curv}}}{28}+\sum_{\ell=5,7,\ldots}\frac{(\lambda_\ell-15)(\lambda_\ell-3)}{28}\lVert f_\ell\rVert_2^2.

On the other hand, Z=∑ℓ≥5, ℓ odd(λℓ−3)2∥fℓ∥22Z=\sum_{\ell\ge5,\ \ell\ \mathrm{odd}}(\lambda_\ell-3)^2\lVert f_\ell\rVert_2^2. For λℓ≥35\lambda_\ell\ge35,

λℓ−1528(λℓ−3)>5224;\frac{\lambda_\ell-15}{28(\lambda_\ell-3)}>\frac{5}{224};

the ratio is increasing and equality holds at degree five. Consequently

S3(K)−11π256≥Dcurv28+5224Z.(46)S_3(K)-\frac{11\pi^2}{56}\ge\frac{D_{\mathrm{curv}}}{28}+\frac{5}{224}Z. \tag*{(46)}

Set g=tr⁡A3=−12f3g=\operatorname{tr}A_3=-12f_3. Then

∥g∥22=67∥A3∥22≤9π27.\lVert g\rVert_2^2=\frac{6}{7}\lVert A_3\rVert_2^2\le\frac{9\pi^2}{7}.

There are 16 degree-three harmonics on S3S^3. For an orthonormal basis YjY_j, the tensor T(u)=∑j∇Yj(u)⊗∇Yj(u)T(u)=\sum_j\nabla Y_j(u)\otimes\nabla Y_j(u) is unchanged by rotations fixing uu, so it is a scalar multiple of the identity on TuS3T_uS^3. Its trace is constant and its integral is 16⋅1516 \cdot15. Since ∣S3∣=2π2|S^3| = 2\pi^2 and the tangent space has dimension three,

T(u)=16⋅153∣S3∣I=40π2I.T(u) = \frac{16 \cdot15}{3|S^3|}I = \frac{40}{\pi^2}I.

Write g=∑jcjYjg = \sum_j c_jY_j. For every unit tangent vector v\mathbf{v}, Cauchy–Schwarz gives

∣∂vg∣2≤∑jcj2∑j∣∂vYj∣2=∥g∥2240π2≤3607.|\partial_{\mathbf{v}}g|^2 \le\sum_j c_j^2\sum_j|\partial_{\mathbf{v}}Y_j|^2 = \|g\|_2^2\frac{40}{\pi^2} \le\frac{360}{7}.

Taking the supremum over v\mathbf{v} proves the global Lipschitz bound

∣∇g∣≤360/7<36/5.(47)|\nabla g| \le\sqrt{360/7}<36/5. \tag*{(47)}

Let a=9/50a=9/50, r=1/40r=1/40, and put

Ωa={u∈S3:∣g(u)∣≤a}.\Omega_a=\{u\in S^3:|g(u)|\le a\}.

On every great circle gg is odd under a half turn, so it has a zero and an antipodal zero. Around these two zeros, the four half-arcs of length r=1/40r=1/40 lie in Ωa\Omega_a, because (36/5)r=a(36/5)r=a. These arcs do not overlap, since r<π/2r<\pi/2. Their total circle length is 4r4r. Averaging over rotations of one fixed great circle and applying Fubini gives the spherical measure estimate

σ(Ωa)≥∣S3∣4r2π=4πr.(48)\sigma(\Omega_a)\ge|S^3|\frac{4r}{2\pi}=4\pi r. \tag*{(48)}

This argument does not require a choice of a common zero for different circles.

For any three eigenvalues in [−1/2,1/2][-1/2,1/2],

∥A∥F2≤12+(tr⁡A)2.\|A\|_F^2\le\frac{1}{2}+(\operatorname{tr}A)^2.

To verify it, maximize ∑λi2−(∑λi)2=−2∑i<jλiλj\sum\lambda_i^2-(\sum\lambda_i)^2=-2\sum_{i<j}\lambda_i\lambda_j on the cube; it is affine in each coordinate separately and its vertex maximum is 1/21/2. Choose b=27/100b=27/100. By Chebyshev’s inequality, ∣tr⁡AR∣≤b|\operatorname{tr}A_R|\le b outside a set of measure at most Z/b2Z/b^2. On the remaining portion of Ωa\Omega_a,

34−∥A∥F2≥d:=14−(a+b)2>0.\frac{3}{4}-\|A\|_F^2\ge d:=\frac{1}{4}-(a+b)^2>0.

Here dd is a positive scalar gap, unrelated to the width parameter in § 2. The deficit is nonnegative everywhere; hence

Dcurv+CZ≥dσ(Ωa),d=19400,C=db2=475729.D_{\mathrm{curv}}+CZ\ge d\sigma(\Omega_a),\qquad d=\frac{19}{400},\qquad C=\frac{d}{b^2}=\frac{475}{729}.

These rational choices obey (5/224)/C=729/21280<1/28(5/224)/C=729/21280<1/28. Combining this inequality with (46) and (48) gives

S3(K)−11π256≥5224C(Dcurv+CZ)≥5b2224(4πr)=729π4480000=εS.S_3(K)-\frac{11\pi^2}{56}\ge\frac{5}{224C}(D_{\mathrm{curv}}+CZ)\ge\frac{5b^2}{224}(4\pi r)=\frac{729\pi}{4480000}=\varepsilon_S.

Combining Jung’s theorem with Minkowski’s volume formula, as above, gives 4Vol⁡4(K)≥rJS3(K)4\operatorname{Vol}_4(K)\ge r_JS_3(K) and proves the volume assertion. We refer to this combination as the Jung–Minkowski estimate. Rotational smoothing preserves width one and converges in the convex-body topology, so continuity of surface area and volume extends the inequalities to arbitrary constant-width bodies. The rational comparisons and the displayed decimal lower endpoint can be checked by the accompanying 192-bit Arb script certify_lower_gap.py; this numerical check is separate from the analytic proof just given. □

Remark 5.3 (The lower-bound constant). The exact right-hand side of (45) equals

0.1781840422363513….0.1781840422363513\ldots.

This improves (43) without using a three-dimensional volume lower bound. It is a lower-bound constant, not an approximation to the unknown minimum. The argument uses the simple rational thresholds a=9/50a=9/50 and b=27/100b=27/100 without optimizing them. Its longer spectral proof records an independent refinement; numerically, the projection bound in Corollary 5.4 is stronger.

A stronger bound from three-dimensional projections

Jiang’s Theorem 1.1 in [6] states that every three-dimensional convex body of constant width one has volume at least 1651/40001651/4000. This external result gives a short improvement of the four-dimensional bound.

Corollary 5.4 (Projection lower bound). Every convex body K⊂R4K \subset\mathbb{R}^{4} of constant width one satisfies

Vol⁡4(K)≥Lproj:=4953π32000(1−2/5)>0.17872203.(49)\operatorname{Vol}_{4}(K) \ge L_{\mathrm{proj}} := \frac{4953\pi}{32000}\left(1-\sqrt{2/5}\right) > 0.17872203. \tag*{(49)}

Proof. Let E⊂R4E \subset\mathbb{R}^{4} be any three-dimensional linear subspace. Orthogonal projection preserves the support function in directions belonging to EE: hK∣E(u)=hK(u)h_{K|E}(u)=h_K(u) for u∈E∩S3u \in E \cap S^{3}. Hence K∣EK|E has constant width one, so Jiang’s theorem gives Vol⁡3(K∣E)≥1651/4000\operatorname{Vol}_{3}(K|E) \ge1651/4000. Cauchy’s surface-area formula [7 Section 1], with ordinary spherical measure, reads

S3(K)=1κ3∫S3Vol⁡3(K∣u⊥) dσ(u),κ3=4π3.S_{3}(K)=\frac{1}{\kappa_{3}}\int_{S^{3}}\operatorname{Vol}_{3}(K|u^{\perp})\,\mathrm{d}\sigma(u), \qquad\kappa_{3}=\frac{4\pi}{3}.

Since ∣S3∣=2π2|S^{3}|=2\pi^{2}, it follows that S3(K)≥(3π/2)(1651/4000)S_{3}(K)\ge(3\pi/2)(1651/4000). The Jung–Minkowski estimate 4Vol⁡4(K)≥(1−2/5)S3(K)4\operatorname{Vol}_{4}(K)\ge(1-\sqrt{2/5})S_{3}(K) from above proves the claim. □

The constant satisfies

0.17872203991039462<Lproj<0.17872203991039463.0.17872203991039462 < L_{\mathrm{proj}} < 0.17872203991039463.

This corollary uses only the stated constant 1651/40001651/4000 from Jiang’s preprint. It does not require extending that paper’s contact-geometry argument to four dimensions.

Discussion

Theorem 4.9 proves that U4(1)U_{4}^{(1)} is not a local volume minimizer, even with all simplex symmetries retained. The proof gives a formula for the deformation and justifies a positive parameter range without quantifying its endpoints. It does not determine an optimal member of this family or an optimal symmetric body.

The spectral bound in Theorem 5.2 and the literature-dependent projection bound in Corollary 5.4 remain well below Vol⁡4(U4(1))≈0.221836\operatorname{Vol}_{4}(U_{4}^{(1)}) \approx0.221836, whose six-decimal rounding is certified in [5 equation (1.4)]. This is the volume of the original body, not a numerical evaluation of the deformed bodies. A useful quantitative descent would need a larger certified gain that justifies its proof’s complexity. Such an optimization is not pursued here. Neither the descent nor the lower bounds decide whether a global minimizer retains simplex symmetry.

Code for checking only the displayed lower-bound constants is available in the computational supplement (manuscript2/lower_bound_checks/).

References

  1. [1]A. Arman, A. Bondarenko, A. Prymak and D. Radchenko, Small volume bodies of constant width with tetrahedral symmetries, SIGMA 21 (2025), 109.DOI
  2. [2]R. Schneider, Convex Bodies: The Brunn–Minkowski Theory, 2nd expanded ed., Cambridge University Press, 2014.
  3. [3]H. Federer, Geometric Measure Theory, Springer, 1969.
  4. [4]A. Prymak, An Endpoint Variational Criterion and a Branch-Coupled Constant-Width Descent from U_n, n ≥ 4, unpublished manuscript, 2026.
  5. [5]H. Wang, Volume Computation and Comparison for Four-Dimensional Bodies of Constant Width, Hexagon preprint hexagon:2610.00561v1, version 1, October 26, 2026.
  6. [6]Y. Jiang, A 0.41275 lower bound for the three-dimensional Blaschke–Lebesgue problem, preprint, arXiv:2610.13964v1, 2026, https://arxiv.org/abs/2610.13964v1.
  7. [7]D. Hug and R. Schneider, Vectorial analogues of Cauchy’s surface area formula, Arch. Math. 122 (2024), 343–352, doi:10.1007/s00013-023-01962-y.DOI

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