The ground states of even-even Z = N nuclei are determined with the isospin
generalized BCS equations and the HFB equation. The calculations permit th
e simultaneous existence of the following Cooper pairs: pp, nn, pn(T = 1),
and pn(T = 0) where the two nucleons in a pair occupy space-spin orbitals w
hich are related by time reversal, as well as pn(T = 0) where the two nucle
ons are in identical space-spin orbitals. There is a transition from T = 1
Cooper pairs at the beginning of this isotope sequence to T = 0 Cooper pair
s at the end of the sequence. Near the middle of the isotope sequence, ther
e is coexistence of a T = 0 pair superfluid and a T = 1 pair superfluid in
the same wave function. The fluctuation in the particle number is reduced i
f the wave function contains proton-neutron pairing. The fluctuation in the
isospin is eliminated and isospin is conserved if the wave function contai
ns only T = 0 pairing.