In (enriched) category theory by a cosmos one means a “good place in which to do (enriched) category theory”. Typically what is meant is a base of enrichment (being by default a monoidal category or more generally a bicategory or similar) which carries enough extra structure for intended category-theoretic-constructions (such as enriched functor categories, etc.) to exist in -enriched category theory.
The word is chosen by analogy with the notion of toposes which may be regarded as “a good places to do set theory”.
There are a number of different, inequivalent, definitions of “cosmos” in the literature.
A Bénabou cosmos (see Street 74, p. 1) is a complete and cocomplete (hence bicomplete) closed symmetric monoidal category.
This is the ideal situation for -enriched category theory.
Shulman (2013) introduced an indexed generalization of Bénabou cosmoi, appropriate for studying enriched indexed categories over a base category. Notably, while the definition of Bénabou cosmoi is not “elementary” (it involves infinitary (non-finite) limits and colimits), the indexed version is elementary; the infinitary structure is folded into the indexing base category. The notion of Bénabou cosmoi is recovered as particular cosmoi indexed over Set.
Ross Street has taken a different tack, defining a “cosmos” to be the collection of (enriched) categories and relevant structure for doing category theory, rather than the “base” category over which the enrichment occurs.
Street (1974) defined a (fibrational) cosmos to be a 2-category in which internal fibrations are well-behaved and representable by a structure of “presheaf objects” (later realized to be a special sort of Yoneda structure). Note that while this includes Cat, it does not include VCat for non-cartesian , since internal fibrations are poorly behaved there. The definition is given in Street (1980):
A fibrational cosmos is a 2-category such that
finite limits exist in ;
there is a 2-adjunction ;
each object admits a discrete fibration from satisfying two technical properties.
The objects are the “presheaf objects” that represent fibrations.
Street (1981) instead defines a cosmos to be a 2-category that “behaves like the 2-category - of enriched categories and profunctors”. The precise definition:
A cosmos is a 2-category (or bicategory) such that:
Small (weak, or bi-) coproducts exist.
Each monad admits a Kleisli construction (analogous to the exactness of a topos).
It is locally small-cocomplete, i.e. its hom-categories have small colimits that are preserved by composition on each side.
There exists a small “Cauchy generator”.
These hypotheses imply that it is equivalent to the bicategory of categories and profunctors enriched over some “base” bicategory. (Note the generalization from enrichment over a monoidal category to enrichment over a bicategory.)
Defined in this way, cosmoi are closed under dualization, parametrization and localization, suitably defined.
An infinity-cosmos is a “good place in which to do higher category theory” as axiomatized by Riehl and Verity in their work on the foundations of - and -category theory.
Apparently there is no written account by Jean Bénabou of his definition of cosmos. One finds it recounted in Street 74, p. 1:
“to J. Bénabou the word means ”bicomplete symmetric monoidal category“, such categories being rich enough so that the theory of categories enriched in develops to a large extent just as the theory of ordinary categories.”
Ross Street, Elementary cosmoi I. in Category Seminar, Lecture Notes in Mathematics 420, Springer (1974) [doi:10.1007/BFb0063103]
Ross Street, Cosmoi of internal categories, Transactions of the American Mathematical Society 258 2 (1980) 271-318 [doi:10.2307/1998059]
Ross Street, Cauchy characterization of enriched categories, Rend. Sem. Mat. Fis. Milano 51 (1981): 217-233, Reprints in Theory and Applications of Categories, 4 (2004) 1-16 [tac:tr4, pdf]
Mike Shulman, Enriched indexed categories, Theory and Applications of Categories, 28 21 (2013) 616-695 (tac:28-21)
Last revised on August 22, 2023 at 16:40:09. See the history of this page for a list of all contributions to it.