There are at least two approaches to the quantum theory of relativistic strings. One way is to look at a string model as a field theory in two spacetime dimensions. In this case, the string coordinates are reinterpreted as a multiplet of scalar fields defined over the string manifold parametrized by a Lorentzian coordinate mesh . The non-linearity of the Nambu-Goto action can be ``softened'' by assigning an auxiliary metric field over the string manifold, and then writing the action in the Howe-Tucker form [1]. After this reshuffling of variables, the original string model is converted into a local field theory and is quantized through canonical, or path integral methods [2]. Quantum fluctuations around a classical solution eventually give rise to a spectrum of elementary particles, and the string itself acquires the status of fundamental building block of everything in the universe.
On the other hand, one may regard a string as an elementary
physical system by itself, and focus on the geometric and
topological properties of the string manifold.
Vortices in a super-conducting medium [3]
and cosmic strings [4] are two noteworthy
examples of this geometrical approach. Quantum fluctuations
are now interpreted as transitions between different string
configurations. In particular, the quantum propagation kernel
acquires the meaning
of probability amplitude for the string shape to evolve from
an initial configuration, represented by the non
self-intersecting spatial loop
,
to a final, non self-intersecting
configuration
.
Thus, in this functional approach, spatial
deformations of the string shape are mapped into ``translations''
in the space of all possible loop configurations, and our major
concern is to develop a ``Hamiltonian'' theory for the quantum
mechanics of strings in loop space. As a matter of fact,
the main purposes of this paper can be stated as follows:
Stefano Ansoldi
Department of Theoretical Physics
University of Trieste
TRIESTE - ITALY