The Universe contains much more matter than antimatter, which is proba
bly the result of processes in the early Universe in which baryon numb
er was not conserved. These processes may have occurred during the ele
ctroweak phase transition, when elementary particles first acquired ma
ss(1-4). It is impossible to study directly processes relevant to the
early Universe, because of the extreme energies involved. One is there
fore forced to investigate laboratory systems with analogous phase tra
nsitions. Much of the behaviour of superfluid He-3 is analogous to tha
t predicted within the standard model of the electroweak interaction(5
). Superfluids and liquid crystals have already been used to investiga
te cosmic-string production(6-11); here we describe experiments on He-
3 that demonstrate the creation of excitation momentum (which we call
momentogenesis) by quantized vortices in the superfluid. The underlyin
g physics of this process is similar to that associated with the creat
ion of baryons within cosmic strings, and our results provide quantita
tive support for this type of baryogenesis.