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An introduction to recursively saturated and resplendent models1

Published online by Cambridge University Press:  12 March 2014

Jon Barwise
Affiliation:
University of Wisconsin, Madison, Wisconsin 53706
John Schlipf
Affiliation:
University of Wisconsin, Madison, Wisconsin 53706

Extract

The notions of recursively saturated and resplendent models grew out of the study of admissible sets with urelements and admissible fragments of L ω1ω, but, when applied to ordinary first order model theory, give us new tools for research and exposition. We will discuss their history in §3.

The notion of saturated model has proven to be important in model theory. Its most important property for applications is that if , are saturated and of the same cardinality then = iff . See, e.g., Chang-Keisler [3]. The main drawback is that saturated models exist only under unusual assumptions of set theory. For example, if 2κ = κ+ then every theory T of L has a saturated model of power κ+. (Similarly, if κ is strongly inaccessible, then every T has a saturated model of power κ.) On the other hand, a theory T like Peano arithmetic, with types, cannot have a saturated model in any power κ with ω ≤ κ ≤ .

One method for circumventing these problems of existence (or rather non-existence) is the use of “special” models (cf. [3]). If κ = Σλ<κ2λ, κ < ω, then every theory T of L has a special model of power κ. Such cardinals are large and, themselves, rather special. There are definite aesthetic objections to the use of these large, singular models to prove results about first order logic.

Type
Research Article
Copyright
Copyright © Association for Symbolic Logic 1976

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Footnotes

2

The first author is an Alfred P. Sloan Fellow.

3

Part of the research for this paper was done while the second author held an NSF Graduate Fellowship at the University of Wisconsin.

1

This paper is essentially the text of an invited hour address presented to the Association on April 25,1975 at its spring meeting in Chicago by the first author. Its preparation was supported by NSF grant GP-43882X.

References

REFERENCES

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