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Transactions of the American Mathematical Society

Published by the American Mathematical Society since 1900, Transactions of the American Mathematical Society is devoted to longer research articles in all areas of pure and applied mathematics.

ISSN 1088-6850 (online) ISSN 0002-9947 (print)

The 2020 MCQ for Transactions of the American Mathematical Society is 1.48.

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Star-fundamental algebras: polynomial identities and asymptotics
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by Antonio Giambruno, Daniela La Mattina and Cesar Polcino Milies PDF
Trans. Amer. Math. Soc. 373 (2020), 7869-7899 Request permission

Abstract:

We introduce the notion of star-fundamental algebra over a field of characteristic zero. We prove that in the framework of the theory of polynomial identities, these algebras are the building blocks of a finite dimensional algebra with involution $*$.

To any star-algebra $A$ is attached a numerical sequence $c_n^*(A)$, $n\ge 1$, called the sequence of $*$-codimensions of $A$. Its asymptotic is an invariant giving a measure of the $*$-polynomial identities satisfied by $A$. It is well known that for a PI-algebra such a sequence is exponentially bounded and $\exp ^*(A)=\lim _{n\to \infty }\sqrt [n]{c_n^*(A)}$ can be explicitly computed. Here we prove that if $A$ is a star-fundamental algebra, \begin{equation*} C_1n^t\exp ^*(A)^n\le c_n^*(A)\le C_2n^t \exp ^*(A)^n, \end{equation*} where $C_1>0,C_2, t$ are constants and $t$ is explicitly computed as a linear function of the dimension of the skew semisimple part of $A$ and the nilpotency index of the Jacobson radical of $A$. We also prove that any finite dimensional star-algebra has the same $*$-identities as a finite direct sum of star-fundamental algebras. As a consequence, by the main result in [J. Algebra 383 (2013), pp. 144–167] we get that if $A$ is any finitely generated star-algebra satisfying a polynomial identity, then the above still holds and, so, $\lim _{n\to \infty }\log _n \frac {c_n^*(A)}{\exp ^*(A)^n}$ exists and is an integer or half an integer.

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Additional Information
  • Antonio Giambruno
  • Affiliation: Dipartimento di Matematica e Informatica, Università di Palermo, Via Archirafi 34, 90123, Palermo, Italy
  • MR Author ID: 73185
  • ORCID: 0000-0002-3422-2539
  • Email: antonio.giambruno@unipa.it, antoniogiambr@gmail.com
  • Daniela La Mattina
  • Affiliation: Dipartimento di Matematica e Informatica, Università di Palermo, Via Archirafi 34, 90123, Palermo, Italy
  • MR Author ID: 734661
  • ORCID: 0000-0002-0714-1442
  • Email: daniela.lamattina@unipa.it
  • Cesar Polcino Milies
  • Affiliation: Instituto de Matemática e Estatística, Universidade de São Paulo, Caixa Postal 66281, CEP-05315-970, São Paulo, Brazil; and Universidade Federal do ABC, Av. dos Estados 5001, Santo Andre, São Paulo, Brazil
  • MR Author ID: 140680
  • ORCID: 0000-0002-8389-0533
  • Email: polcino@ime.usp.br, polcino@ufabc.edu.br
  • Received by editor(s): April 2, 2018
  • Received by editor(s) in revised form: October 29, 2019, and March 2, 2020
  • Published electronically: August 28, 2020
  • Additional Notes: The first author was partially supported by CNPq proc. 400439/2014-0, the second author was partially supported by GNSAGA of INdAM, and the third author was partially supported by FAPESP, proc. 2015/09162-9 and CNPq proc. 300243/79-0.
  • © Copyright 2020 American Mathematical Society
  • Journal: Trans. Amer. Math. Soc. 373 (2020), 7869-7899
  • MSC (2010): Primary 16R10, 16R50; Secondary 16P90, 16W10
  • DOI: https://doi.org/10.1090/tran/8182
  • MathSciNet review: 4169676