An Introduction to String Field Theory
An Introduction to String Field Theory
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弦场论简介
DOI:
10.1111/j.1749-6632.1987.tb40382.x
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发表时间:
1987
期刊:
影响因子:
--
通讯作者:
G. West
中科院分区:
文献类型:
--
作者:
G. West
One of the most appealing aspects of the field theoretic formulation of elementary particle interactions is that it very naturally incorporates general symmetry properties such as Lorentz and gauge invariance. Furthermore, nonperturbative effects arising from spontaneous symmetry breaking or from the underlying topological structure of the theory are most easily accommodated within this framework. Indeed, the usual formulation and understanding of the standard model is almost unthinkable outside of field theory. Therefore, it is quite natural to attempt a similar formulation for string theories because with the recent discovery of anomaly cancellations,' these have emerged as serious candidates for a completely unified description of all the interactions including gravitation.' In the string case, there is perhaps even stronger motivation for a gauge-invariant field theoretic description because one of its more remarkable properties is the automatic appearance of massless gauge particles (in particular, the graviton) without the explicit introduction of some fundamental principle akin to Einstein's general coordinate invariance or the principle of equivalence. Presumably, part of this mystery is due to the fact that these theories were formulated in the physical light-cone gauge, thereby masking any general underlying gauge symmetry. The formulation of a completely gauge-invariant action for the interacting string would hopefully lead to a deeper understanding of how and why these theories work and, ultimately, what the underlying principle actually is. Furthermore, without such a formulation, it would seem unlikely that the question of compactification to a four-dimensional "real" world could be dynamically understood because this requires an understanding of the vacuum structure of the theory. Ordinary field theory is based upon the Newtonian concept of point particles whose motion is described by one-dimensional world lines, x ~ ( T ) , parametrized by the evolution parameter (time) T (see FIGURE 1). In principle, one could set up particle interactions in terms of these first quantized world lines without explicit reference to a field and thereby calculate all S-matrix elements. Typically, this is not what is done; instead, one introduces a local field 4(x) whose Fourier components represent the creation or destruction of particles of a given momentum. In this formalism, the scattering of particles is ascribed to local interactions among the various fields. As the simplest possible example of this duality between a world-line and field formulation, I shall examine (below) the case of a free relativistic point particle and show how the