TL;DR
Possibly, but not transparently.
Part of the reason that there is no familiar fundamental law bounding temperature changes is that temperature is an emergent description of a system (historically through the statistical mechanical behavior of atoms and molecules although the definition of temperature has been generalized in ways that can apply to other systems). Temperature isn't a truly fundamental physical quantity.
The answer could be that: (1) there is no limit, (2) that the limit is truly immense, or (3) that the question is ill-defined as it approaches the extremes it is asking about.
The question is also ambiguous about whether it is talking about the biggest change that is possible in our actual universe, or about the biggest change that our laws of physics would permit in any arbitrary universe even if it could never happen in our actual universe because the combination of particles in particular states necessary to make that happen are physically impossible to assemble.
Unlike the speed of light, there is certainly no absolute limit on the maximum rates of temperature change in a physically possible system that has practical engineering implications in directly observable physical systems.
But, in any particular well defined class of physical system that is capable of having a well defined temperature and temperature change, you could calculate the rate temperature change that is possible in that particular class of physical systems. See, post #7 for examples.
For example, you could calculate the maximum rate at which the temperature of a system that starts as a drop of water exposed to extremely high frequency photons with a well defined total energy could change.
Long (more advanced than basic) Answer
At the fundamental level there are particles with mass, kinetic energy, spin, frequency, helicity, polarization, etc. But there are ways to define temperature that are very general even in systems where statistical mechanics understandings of thermodynamics are ill-defined.
For example, one can argue there thermodynamic temperature corresponds to momentum or energy transfer in an interaction of two particles, aggregated in some sensible way for a system of more than two particles.
You could argue that there is some maximum level arising from fundamental particle physics laws that ends up putting some sort of bounds on a before and after state in which temperature is defined in a given time period. You would start with the kind of analysis of post #17 in this thread and tweak it to a situation where temperature is defined at each end and consider variation on it where the temperature chance could be greater.
Part of the answer may hinge on the unresolved question of whether there is a UV (i.e. high energy) fixed point in physics at extremely high energies that is absent in the Standard Model of Particle Physics.
Another is the question of the extent to which space-time is continuous or if the continuity of space and time just a very good approximation of reality that in fact breaks space-time into discrete little chunks of a minimum size, with the conventional laws of physics breaking down as you get very close to that minimum size.
For example, it could be that time is discrete and comes in units of Planck time. If so, the minimum elapsed time between states would be one unit of Planck time, and one could conceivably start infinitesimally close to absolute zero and get arbitrarily high in temperature, e.g., with matter-antimatter annihilation in large enough amounts.
Worse yet, in a highly relativistic system involving immense energies on one side of the temperature change, and very small, near Planck scale, distances, the temporal sequence of the events might be observer or coordinate system dependent, and might not even be absolutely causal or local. If a temperature change happens in a space-like rather than time-like interval, you end up with a division by zero problem no matter how big or small the temperature change actually is, which gives you an infinite temperature change per time, which I suppose would amount to proof that there is no such fundamental limit.
Another approach would be to observe that the largest change in temperature per time almost surely happened at the Big Bang, in a way that is physically impossible to recur, and then to try to quantify it. But, while that can get you arbitrarily close to an answer, the singularity at the Big Bang might defy calculation or suggest a limit that approaches infinity as one gets arbitrarily close to the Big Bang singularity of GR.
There is also a lot of theoretical non-consensus about the sequence of events after the Big Bang in the first part of the first second after the Big Bang. The last time I looked, for example, there were at least
118 competing theories of cosmological inflation and there were also alternative theories to the cosmological inflation paradigm. This matters a lot to this question because the brief period of cosmological inflation, if some version of this theory is correct, is probably the moment at which there was the greatest temperature change in the universe of all time, and hence, more or less by definition, the great possible temperature change.
Another definitional issue is the extent to which the Heisenberg uncertainty principle renders any sufficiently small interval of time in a system that can have temperature changes ill-defined. Heisenberg uncertainty concerns would arise well before a classical GR type Big Bang singularity becomes infinite and mathematically intractable.
More generally, conventional wisdom is that in the vicinity of a classical GR singularity like a black hole or the Big Bang, that classical GR is no longer in its domain of applicability and you can only answer these questions with a theory of quantum gravity that does not exist yet, in a full blow, rigorous form.
In conclusion, then, a reliable answer to this question pushes the boundaries of the domain of applicability of "core theory" (i.e. general relativity plus the Standard Model of Particle Physics) in ways that highlight the internal inconsistencies of "core theory" as we understand it today.