A number of authors have proposed stochastic versions of the
Schrödinger equation, either as effective evolution equations
for open quantum systems or as alternative theories with an
intrinsic collapse mechanism. Here we discuss two directions
for the generalization of these equations. First, we study a
general class of norm preserving stochastic evolution
equations, and show that even after making several
specializations there is an infinity of possible stochastic
Schrödinger equations for which state vector collapse is
provable. Second, we explore the problem of formulating a
relativistic stochastic Schrödinger equation, using a
manifestly covariant equation for a quantum field system based
on the interaction picture of Tomonaga and Schwinger. The
stochastic noise term in this equation can couple to any local
scalar density that commutes with the interaction energy
density, and leads to collapse onto spatially localized
eigenstates. However, as found in a similar model by Pearle,
the equation predicts an infinite rate of energy nonconservation
proportional to δ3(
), arising from the local
double commutator in the drift term.