| Expanders from symmetric codes |
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Annual ACM Symposium on Theory of Computing
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Proceedings of the thiry-fourth annual ACM symposium on Theory of computing
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Montreal, Quebec, Canada
SESSION: Session 11A
table of contents
Pages: 669 - 677
Year of Publication: 2002
ISBN:1-58113-495-9
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Authors
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Roy Meshulam
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Technion, Haifa, Israel and Institute for Advanced Study, Princeton, NJ
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Avi Wigderson
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Hebrew university, Jerusalem, and Institute for Advanced Study, Princeton, NJ
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Downloads (6 Weeks): 1, Downloads (12 Months): 24, Citation Count: 1
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ABSTRACT
(MATH) A set S in the vector space FFpn is "good" if it satisfies the following (almost) equivalent conditions: - S is an expanding generating set of Abelian group FFpn.
- S are the rows of a generating matrix for a linear distance error-correcting code in FFpn.
- All (nontrivial) Fourier coefficients of S are bounded by some &egr; ξ 1 (i.e. the set S is &egr;-biased).
.A good set S must have at least cn vectors (with cρ1). We study conditions under which S is the orbit of only constant number of vectors, under the action of a finite group G on the coordinates. Such succinctly described sets yield very symmetric codes, and "amplifies" small constant-degree Cayley expanders to exponentially larger ones [19, 2].For the regular action (the coordinates are named by the elements of the group G), we develop representation theoretic conditions on the group G which guarantee the existence (in fact, abundance) of such few expanding orbits. The condition is a (nearly tight) upper bound on the distribution of dimensions of the irreducible representations of G, and is the main technical contribution of this paper. We further show a class of groups for which this condition is implied by the expansion properties of the group G itself! Combining these, we can iterate the amplification process above, and give (near-constant degree) Cayley expanders which are built from Abelian components.For other natural actions, such as of the affine group on a finite field, we give the first explicit construction of such few expanding orbits. In particular, we can completely derandomize the probabilistic construction of expanding generators in [2].
REFERENCES
Note: OCR errors may be found in this Reference List extracted from the full text article. ACM has opted to expose the complete List rather than only correct and linked references.
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