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Cartesian restrictions cannot be extracted from almost full input mass


Status and reason for considering this question

The propositions below are proved. They concern every fixed diagonal form of degree rr in rr variables, r≥3r\ge3. They do not settle either target question about SrS_r.

The bounded-fiber criterion would give positive density from a positive fraction of input tuples lying in bounded fibers. Those tuples need not form a Cartesian product. The distinction matters for a new possible method: Croot, Mao, Pohoata, Sheffer, and Yip's weighted entropic sieve, Section 4 assumes independent coordinate laws in Proposition 4.3. Its Theorem 4.1 assumes Cartesian input sets and a uniform bound on every output fiber; the proof uses these hypotheses separately in equations (12)--(14). Theorem 1.7 bounds a B3[g]B_3[g] subset of the first NN cubes by O(g1/9Nexp⁡(−clog⁡N/log⁡log⁡N))O(g^{1/9}N\exp(-c\sqrt{\log N}/\log\log N)). These statements and the relevant proof passages were checked in the full primary text. None asserts bounded typical multiplicity for all triples, or a density estimate for their values.

The next construction shows, within the exact diagonal-form setting, why one cannot automatically replace those hypotheses by high input mass or even by a vanishing relative-entropy deficit.

An almost full set with small Cartesian rectangles

Fix r≥3r\ge3 and nonzero integers a1,…,ara_1,\ldots,a_r, and put

F(x)=∑i=1raixir,g=gcd⁡(r,2),Y=log⁡N10.F(\mathbf x)=\sum_{i=1}^r a_i x_i^r, \qquad g=\gcd(r,2),\qquad Y=\frac{\log N}{10}.

For sufficiently large NN, let

PN={p∈[Y,2Y]:p≡−1(mod2r),p∤a1⋯ar},ℓN=∣PN∣,ΔN=∏p∈PNp.\mathcal P_N=\{p\in[Y,2Y]:p\equiv-1\pmod{2r},\quad p\nmid a_1\cdots a_r\}, \quad \ell_N=|\mathcal P_N|, \quad \Delta_N=\prod_{p\in\mathcal P_N}p.

The prime number theorem in this fixed progression gives

ℓN∼log⁡N10φ(2r)log⁡log⁡N,log⁡ΔN∼Yφ(2r).(1)\ell_N\sim\frac{\log N}{10\varphi(2r)\log\log N}, \qquad \log\Delta_N\sim\frac{Y}{\varphi(2r)}. \tag{1}

In particular, ΔN≤N1/5\Delta_N\le N^{1/5} eventually. Define the output-dependent input restriction

ΓN={x∈[N]r:p∤F(x) for all p∈PN}.\Gamma_N=\{\mathbf x\in[N]^r: p\nmid F(\mathbf x)\text{ for all }p\in\mathcal P_N\}.

Theorem. One has

∣ΓN∣=(1−Or(1log⁡log⁡N))Nr.(2)|\Gamma_N|=\left(1-O_r\left(\frac1{\log\log N}\right)\right)N^r. \tag{2}

Nevertheless, every Cartesian rectangle B1×⋯×Br⊆ΓNB_1\times\cdots\times B_r\subseteq\Gamma_N, with Bi⊆[N]B_i\subseteq[N], satisfies

∏i=1r∣Bi∣≤(1+or(1))Nr(g/r)ℓN.(3)\prod_{i=1}^r|B_i| \le(1+o_r(1))N^r(g/r)^{\ell_N}. \tag{3}

If Br⊆ΓNB^r\subseteq\Gamma_N, the stronger common-set conclusion is

∣B∣≤(1+or(1))N(g/r)ℓN.(4)|B|\le(1+o_r(1))N(g/r)^{\ell_N}. \tag{4}

Thus (3) saves exp⁡(−crlog⁡N/log⁡log⁡N)\exp(-c_r\log N/\log\log N) in volume, and (4) saves such a factor in the root-set size, for some cr>0c_r>0.

Proof. For each selected prime, gcd⁡(r,p−1)=gcd⁡(r,2)=g\gcd(r,p-1)=\gcd(r,2)=g. The power map on Fp\mathbb F_p therefore has fibers of size at most gg, including its fiber at zero. After fixing x2,…,xrx_2,\ldots,x_r, the congruence F=0(modp)F=0\pmod p allows at most gg residue classes for x1x_1. Hence

#{x∈[N]r:p∣F(x)}≤g(N/p+1)Nr−1.\#\{\mathbf x\in[N]^r:p\mid F(\mathbf x)\} \le g(N/p+1)N^{r-1}.

The union bound, (1), and p≥Yp\ge Y prove (2), since ∑p∈PNp−1=Or(1/log⁡Y)\sum_{p\in\mathcal P_N}p^{-1}=O_r(1/\log Y).

For a nonempty rectangle as in the theorem, write si,p=∣Bi mod p∣s_{i,p}=|B_i\bmod p| and Ti,p={aibr:b∈Bi mod p}T_{i,p}=\{a_i b^r:b\in B_i\bmod p\}. The sum T1,p+⋯+Tr,pT_{1,p}+\cdots+T_{r,p} omits zero. Indeed, any choice of these residues has independent representatives in the corresponding BiB_i, and a zero sum would contradict the restriction defining ΓN\Gamma_N. Iterated Cauchy--Davenport therefore gives

∑i∣Ti,p∣≤p+r−2.\sum_i|T_{i,p}|\le p+r-2.

Since ∣Ti,p∣≥si,p/g|T_{i,p}|\ge s_{i,p}/g,

∑isi,p≤g(p+r−2).(5)\sum_i s_{i,p}\le g(p+r-2). \tag{5}

Assign each pp to an index ii for which si,p≤g(p+r−2)/rs_{i,p}\le g(p+r-2)/r. Let Pi\mathcal P_i be the resulting partition and Δi=∏p∈Pip\Delta_i=\prod_{p\in\mathcal P_i}p, allowing Δi=1\Delta_i=1. CRT and interval counting imply

∣Bi∣≤(N+Δi)∏p∈Pig(p+r−2)rp.|B_i|\le (N+\Delta_i) \prod_{p\in\mathcal P_i}\frac{g(p+r-2)}{rp}.

Multiply over ii. Every Δi≤ΔN≤N1/5\Delta_i\le\Delta_N\le N^{1/5}, and

∏p∈PN(1+r−2p)=1+or(1).\prod_{p\in\mathcal P_N}\left(1+\frac{r-2}{p}\right)=1+o_r(1).

This proves (3). Empty rectangles are trivial. If every Bi=BB_i=B, then all the si,ps_{i,p} are equal, so (5) gives the same bound for ∣B mod p∣|B\bmod p| at every prime. Applying CRT once proves (4). Finally g<rg<r, and (1) gives the stated exponential savings. □\square

Vanishing relative entropy is not sufficient for the weighted step

Specialize to F=x3+2y3+4z3F=x^3+2y^3+4z^3. The preceding prime progression is p≡5(mod6)p\equiv5\pmod6, equivalently p≡2(mod3)p\equiv2\pmod3 for the large primes being used. Let UNU_N be uniform on [N]3[N]^3, and let μN=UN( ⋅∣ΓN)\mu_N=U_N(\,\cdot\mid\Gamma_N). If εN=1−∣ΓN∣/N3\varepsilon_N=1-|\Gamma_N|/N^3, then exactly

D(μN∥UN)=−log⁡(1−εN)=O(1/log⁡log⁡N)=o(1).(6)D(\mu_N\Vert U_N)=-\log(1-\varepsilon_N) =O(1/\log\log N)=o(1). \tag{6}

Here DD is relative entropy, with natural logarithms. The identity

D(μN∥UN)=(∑i=13H((μN)i)−H(μN))+∑i=13D((μN)i∥Unif⁡[N])(7)D(\mu_N\Vert U_N) =\left(\sum_{i=1}^3H((\mu_N)_i)-H(\mu_N)\right) +\sum_{i=1}^3D((\mu_N)_i\Vert\operatorname{Unif}[N]) \tag{7}

shows that the total correlation and all marginal entropy deficits also tend to zero; HH denotes Shannon entropy with the same logarithm.

Define nonnegative weights

mp(x)=p 1p∣F(x),KN(x)=∏p∈PN(1+mp(x)).m_p(\mathbf x)=p\,1_{p\mid F(\mathbf x)},\qquad K_N(\mathbf x)=\prod_{p\in\mathcal P_N}(1+m_p(\mathbf x)).

Cubing permutes Fp\mathbb F_p, so F=0(modp)F=0\pmod p has exactly p2p^2 solutions. Fixing any one coordinate leaves precisely pp solutions in the other two. Thus mpm_p has mean one and each one-coordinate marginal mean is one. CRT gives

ΔN−3∑x mod ΔNKN(x)=2ℓN.\Delta_N^{-3}\sum_{\mathbf x\bmod\Delta_N}K_N(\mathbf x)=2^{\ell_N}.

Every residue vector has (N/ΔN)3(1+O(ΔN/N))(N/\Delta_N)^3(1+O(\Delta_N/N)) representatives in the box, uniformly. Positivity of the weights permits summing these relative errors, yielding

EUNKN=(1+O(ΔN/N))2ℓN,EμNKN=1.(8)\mathbb E_{U_N}K_N=(1+O(\Delta_N/N))2^{\ell_N}, \qquad \mathbb E_{\mu_N}K_N=1. \tag{8}

The latter identity holds because every factor is one on ΓN\Gamma_N.

Consequently a product-law lower bound cannot automatically extend to correlated laws in the form

EμKN≥2ℓNexp⁡(−CD(μ∥UN))\mathbb E_\mu K_N\ge 2^{\ell_N}\exp(-C D(\mu\Vert U_N))

with fixed CC: (6) and (8) contradict it. By (7), replacing the entropy penalty by marginal deficits plus total correlation does not repair this assertion. This example tests such an extension; it does not contradict a theorem stated for independent coordinates.

Consequence for the density problem

A set of bounded-fiber input tuples of size cNrcN^r, if obtained, could be intersected with ΓN\Gamma_N at a cost of only o(Nr)o(N^r) tuples. Thus the positive-density criterion remains viable on these non-Cartesian restrictions. Conversely, (3)--(4) show that high input mass alone cannot supply the Cartesian hypothesis required by the cited bounded-multiplicity sieve. No estimate for the actual integer fibers of FF, and no new infinitude case, follows from this construction.