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Eisenstein-prime Obstruction Sieve for Monogenicity

Khai-Hoan Nguyen-Dang

TL;DR

This work proves a density-zero obstruction phenomenon for monogenicity within Eisenstein-parameter families of pure fields: for $K_m=\mathbb{Q}(\alpha)$ with $\alpha^n=m$ and square-free $m$, the set of indices with $g(m)>1$ that still satisfy the ABS fixed-sign local solvability condition is vanishingly small. Central to the argument is the Eisenstein-prime obstruction sieve, a three-step process combining local index-form coset rigidity, a one-prime $N$th-power obstruction at Eisenstein primes, and a Chebotarev-based sieve closure that yields a positive-density obstructing set of primes. The authors obtain density-equality results between monogenic and $\alpha$-monogenic fields in the pure family, and provide an explicit monogenic density formula $\delta=\frac{6}{\pi^2}\prod_{p\mid n}\frac{p}{p+1}$, highlighting a density-level local-to-global principle in these Eisenstein families. They extend the framework to scaled Eisenstein families, demonstrate necessary hypotheses via thin-parameter counterexamples, and exhibit positive-density ABS-unobstructed subfamilies with fixed nontrivial index, illustrating the nuanced interaction between local conditions and global monogenicity across parameter spaces.

Abstract

Alpöge--Bhargava--Shnidman showed that even a strengthened \emph{no local obstruction} condition for monogenicity does not force a global power integral basis: in the full spaces of cubic and quartic fields, a positive proportion are non-monogenic yet satisfy this ABS fixed-sign condition. This raises a natural family-level question: does the same phenomenon persist inside one-parameter families, where the local structure varies in a highly constrained way? In this paper we answer this in the negative for the pure fields $K_m=\mathbb Q(α)$ with $α^n=m$ ($n\ge 4$) and $m$ square-free. Writing $g(m)=[\mathcal O_{K_m}:\mathbb Z[α]]$, we prove that the set of square-free $m$ for which $g(m)>1$ but $K_m$ has no ABS local obstruction has natural density $0$. Consequently, in the pure family monogenicity and $α$--monogenicity have the same natural density. The proof isolates a reusable mechanism, which we call the Eisenstein-prime obstruction sieve. The argument is packaged in an abstract template and transfers to other Eisenstein parameter families.

Eisenstein-prime Obstruction Sieve for Monogenicity

TL;DR

This work proves a density-zero obstruction phenomenon for monogenicity within Eisenstein-parameter families of pure fields: for with and square-free , the set of indices with that still satisfy the ABS fixed-sign local solvability condition is vanishingly small. Central to the argument is the Eisenstein-prime obstruction sieve, a three-step process combining local index-form coset rigidity, a one-prime th-power obstruction at Eisenstein primes, and a Chebotarev-based sieve closure that yields a positive-density obstructing set of primes. The authors obtain density-equality results between monogenic and -monogenic fields in the pure family, and provide an explicit monogenic density formula , highlighting a density-level local-to-global principle in these Eisenstein families. They extend the framework to scaled Eisenstein families, demonstrate necessary hypotheses via thin-parameter counterexamples, and exhibit positive-density ABS-unobstructed subfamilies with fixed nontrivial index, illustrating the nuanced interaction between local conditions and global monogenicity across parameter spaces.

Abstract

Alpöge--Bhargava--Shnidman showed that even a strengthened \emph{no local obstruction} condition for monogenicity does not force a global power integral basis: in the full spaces of cubic and quartic fields, a positive proportion are non-monogenic yet satisfy this ABS fixed-sign condition. This raises a natural family-level question: does the same phenomenon persist inside one-parameter families, where the local structure varies in a highly constrained way? In this paper we answer this in the negative for the pure fields with () and square-free. Writing , we prove that the set of square-free for which but has no ABS local obstruction has natural density . Consequently, in the pure family monogenicity and --monogenicity have the same natural density. The proof isolates a reusable mechanism, which we call the Eisenstein-prime obstruction sieve. The argument is packaged in an abstract template and transfers to other Eisenstein parameter families.
Paper Structure (24 sections, 44 theorems, 162 equations)

This paper contains 24 sections, 44 theorems, 162 equations.

Key Result

Theorem 1.1

Fix $n\ge4$ and let $m$ range over square-free integers with $X^n-m$ irreducible over $\mathbb{Q}$. Then the set of parameters $m$ such that $g(m)\ge2$ but $K_m$ has no ABS fixed-sign local obstruction has two-sided natural density $0$.

Theorems & Definitions (92)

  • Theorem 1.1: Theorem \ref{['thm:density-zero-ABS']}
  • Theorem 1.2: Theorem \ref{['thm:density-equality']}
  • Theorem 1.3: Theorem \ref{['thm:scaled-density-zero-merged']}
  • Definition 2.1
  • Theorem 2.2: ABHS representability
  • Theorem 2.3: ABHS: the index form cuts out monogenerators
  • Lemma 2.4: Translation invariance
  • proof
  • Lemma 2.5: Unit wedge implies generation
  • proof
  • ...and 82 more