Monoidal natural transformation

Suppose that ( C , , I ) {\displaystyle ({\mathcal {C}},\otimes ,I)} and ( D , , J ) {\displaystyle ({\mathcal {D}},\bullet ,J)} are two monoidal categories and

( F , m ) : ( C , , I ) ( D , , J ) {\displaystyle (F,m):({\mathcal {C}},\otimes ,I)\to ({\mathcal {D}},\bullet ,J)} and ( G , n ) : ( C , , I ) ( D , , J ) {\displaystyle (G,n):({\mathcal {C}},\otimes ,I)\to ({\mathcal {D}},\bullet ,J)}

are two lax monoidal functors between those categories.

A monoidal natural transformation

θ : ( F , m ) ( G , n ) {\displaystyle \theta :(F,m)\to (G,n)}

between those functors is a natural transformation θ : F G {\displaystyle \theta :F\to G} between the underlying functors such that the diagrams

           and         

commute for every objects A {\displaystyle A} and B {\displaystyle B} of C {\displaystyle {\mathcal {C}}} (see Definition 11 in [1]).

A symmetric monoidal natural transformation is a monoidal natural transformation between symmetric monoidal functors.

References

  1. ^ Baez, John C. "Some Definitions Everyone Should Know" (PDF). Retrieved 2 December 2014.