Quantum Mechanics (QM) is the fundamental theory of modern physics. Thus
far, it has successfully been used to describe all processes on scales smaller
than molecules. For systems on the scale of molecules, the complexity of
interacting processes hampers direct analysis using raw QM: however, analyses
via approximations plausible on the scales involved are consistent with
the view that all processes fit in with QM. It has been shown that
the randomness inherent in quantum mechanics cannot be explained away by any
theory of hidden variables
– i.e. internal mechanisms with
deterministic behaviour, that we simply can't see. I am persuaded that the
entire universe is governed by quantum mechanical processes. One stumbling
block remains: we have no fully unified understanding of General Relativity (i.e. gravity) alongside QM. The
theories which manage to combine the two, to greater or lesser degrees, are
known as Quantum Cosmology.
Quantum mechanical discussions in this directory include:
It is my belief that the notation in which modern physics is conducted is old, clunky and in need of revision. In particular, I believe that it is sufficiently clumsy that it is currently hampering the development of better models of the universe and impairing communication between researchers in different fields (c.f. Donald Kennedy's lament here). This belief is, however, only a bunch of hot air until such time as I produce a notation in which it is actually easier to develop such models.
Consequently, while I study QM, I am exploring the mathematical notations
which can do what is required. One example of this is my analysis (dating from
1995) of the position observable in QM, given that
position on a smooth manifold (the domain in which General Relativity says we
must work) is not a linear quantity (i.e. one to which one can apply
scaling and addition). This replaces the orthodox description of observables,
as Hermitian operators on a complex linear space S, with a description as a
measure
, on the space of values of the observable, except that the
measure
maps subsets of this space to projection operators on S, rather
than to real probabilities
; the projection operators yielded by the
measure all commute with one another; and the measure can be used to
integrate
any well-enough-behaved function f from the observable's space
of values to a fixed real linear space U, the integral being a hermitian
operator on S whose eigenvalues lie in U. In particular, when the observable's
space of values is linear, the identity on it can be used as f and its integral
is orthodoxy's hermitian operator.
If a body of given momentum, spin and charge lies entirely within some
region bounded by a Kerr event horizon matching those parameters, then we can
know nothing, in this outside world, about what is going on inside that region.
For a tiny thing like an electron, having it all inside such a tiny region would
entail a huge uncertainty of momentum, which was one of the inputs to what
region of space-time you examined. Still, it suggests a low-level granularity
beyond which one knows one is ignorant of the internals, save only as to their
momentum, spin and charge. When we come to stitch together
charts of a
region of space-time that is
an electron, we can expect to get a full
description of it without needing to use charts smaller than chunks of would-be
event tubes.
I picture an electron as a superposition of solutions to the field
equations, each amounting to a chart of a region of space-time that looks
like
an electron from the outside: all the charts in the superposition give,
internally, solutions of the field equations, and the surrounding universe
reads
them as agreeing on the spin, momentum and charge within the
same
charted region, at least to within the available uncertainty of the
relevant quantities. Such a view of an arbitrary portion of space-time would
make for interesting reading, too, I suspect.

Written by Eddy.