1 Introduction
The notions of observables and states are fundamental to mechanics. In this entry, we shall begin
with the conceptual background to these ideas, then proceed to examine how these notions work in
classical, statistical, and quantum mechanics.
The basis for these notions lies in making numerical measurements on physical systems and
comparing the observed values with predicted theoretical values. The value measured will
depend on the quantity being measured and upon the initial and boundary conditions
imposed on the system. To account for this dependence, we introduce observables and
states—an observable is a mathematical entity in a theory which represents a measurement
which can be made on the physical system described by that theory, and a state is a
mathematical entity which encodes conditions placed on that system. A theory of a system will
provide the set of observables and the set of states for that system, describe how they
evolve with time, and specify how to obtain numerical values by combining states and
observables.
To make this discussion concrete, we may consider an elementary example—the freely
falling body. Here, examples of observables would include the height and velocity of
the object. The state of the system may be specified by stating the initial height and
velocity or by specifying the height at an initial time and at a final time. Given such a
specification, we can then compute the values of velocity and position at any time using these
formulae:
| h − h0 | = g(t − t0)2, | |
|
| v − v0 | = g(t − t0). | | |
The values so obtained may then be compared with experiment.
In addition to the height and velocity, there are other observables such as energy. However, it is
possible to express these observables algebraically in terms of the height and velocity. Note that
this requires use of the equations of motion:
2 Quantum Operators as Observables in Quantum Theories
Remark 2.1. representations of Banach ∗-algebras defined on Hilbert spaces are closely
related to C∗-algebra representations, which provide a useful approach to defining quantum
space-times.
2.1 Quantum operator algebras in quantum field theories: QOA role in QFTs
Important examples of quantum operators are the Hamiltonian operator (or Schrödinger
operator), the position and momentum operators, Casimir operators, unitary operators, and spin
operators. Observable operators are also self-adjoint. More general operators were later defined,
such as Prigogine’s superoperators. The observable corresponding to the Hamiltonian operator of a
closed, conservative system is its energy.
Another development in quantum theories was the introduction of Fréchet nuclear spaces or
“rigged” Hilbert spaces (Hilbert bundles).
2.2 Basic mathematical definitions in QOA
[more to come]
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