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PreprintCC BY 4.0arXiv

A Kallin's lemma for polynomials with exponents in a compact convex set and local approximation

Abstract

Let S⊂Bbb R+n be compact and convex with 0∈ S, and let 𝒫S be the algebra spanned by monomials with exponents in ⋃m≥0(mS∩Bbb N0n). We define the associated polynomial hull and prove a Kallin lemma for the union of two sets convex with respect to this algebra. A weighted approximation lemma then shows that, under a sector or ray condition, two admissible monomials generate exactly the functions of the unrestricted algebra that are constant on a specified zero fibre. Applications include an exact density criterion for mixed monomials, a transfer principle for relative perturbations, and density and hull computations on stars of totally real discs.

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BibTeX
@misc{chi2026kallins,
  title = {{A Kallin's lemma for polynomials with exponents in a compact convex set and local approximation}},
  author = {Kieu Phuong Chi and Duong Thi Thuy Van},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.32025},
  eprint = {2610.32025},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.32025},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - A Kallin's lemma for polynomials with exponents in a compact convex set and local approximation
AU  - Kieu Phuong Chi
AU  - Duong Thi Thuy Van
PY  - 2026
DA  - 2026/10/23
PB  - arXiv
DO  - 10.48550/arxiv.2610.32025
UR  - https://arxiv.org/abs/2610.32025
AB  - Let S⊂Bbb R_+^n be compact and convex with 0∈ S, and let 𝒫^S be the algebra spanned by monomials with exponents in ⋃_m≥0(mS∩Bbb N_0^n). We define the associated polynomial hull and prove a Kallin lemma for the union of two sets convex with respect to this algebra. A weighted approximation lemma then shows that, under a sector or ray condition, two admissible monomials generate exactly the functions of the unrestricted algebra that are constant on a specified zero fibre. Applications include an exact density criterion for mixed monomials, a transfer principle for relative perturbations, and density and hull computations on stars of totally real discs.
ER  -