buddhakan said:
Popularized treatments of quantum mechanics describe it as applicable to the behavior of submicroscopic particles, while relativity applies to the very large (i.e., astronomical). This seems totally arbitrary to me. Where is the boundary between the 2 domains? Atoms? Neutrons? Quarks? Or is it perhaps the nature/properties of the bodies whose behavior is being described rather than their absolute size which is critical? I realize this may be a meaningless question to the expert but what am I missing?
A bit in line with Fredrik's respons, but with a different perspective; an important disctinction is if you consider the relation between the observer and the system that's observed.
QM, in it's tested domains (ie particle physics) the reference of the observer, is effectively massive. It's the entire laboratory frame, which is working as a fixed background, relative to which the interactions of the small subsystem (atom, or subatomic systems) are examined. This is how the environment, can be more or less fully controlled, and the approximation of the observer beeing a static reference reall does make sense for all practical purposes.
This is not true for cosmological models. Some people argue, for example Smolin, and I fully agree, that for this reason the logic implicit in the quantum framework fails for cosmologial models because the approxiamation of (fixed massive reference) studying a subsystem whose environment are monitored fails. In this view, regular "quantum theories" of the entire universe, talking about the wavefunction of the universe etc, does not make any sense since it's applying a framwork that's probably valid only on small subsystems in a controlled environment, to the entire universe where clearly that assumption is totally wrong.
So the unification of QM and GR not only concernts the quantum mechanics of hypotetical small black holes and such, or extreme high energy particle experiments where small black holes may in theory form, it is also concerned with how to unify the framework valid for isolated subsystems (where the timless dynamical laws determined the future from initial conditions in a timeless statespace) with the cosmologial models where the state space generally is evolving, and the laws can only be assessed at a particular moment in time, and the meaning of timeless laws is lost.
For more input see these talks see
"On the reality of time and the evolution of laws"
and the recent
"Laws and time in cosmology" (which I haven't had time to watch yet myself)
found at
http://pirsa.org/index.php?p=speaker&name=Lee_Smolin
If you understand and agree with the points here, it motivates the quest for a new framework where causal laws are emergent and evolving as per some darwinian scheme, similar to what we have in biology and social interaction models.
/Fredrik